THE SUN

Firstly, there would be no need of freezers or air conditioners any more. Everything on earth would completely freeze. Secondly, assuming that earth is still orbiting at the same distance, earth will find itself out of the habitable zone of the Sun, thus slowly but surely wiping out all life on it. Thirdly, stocks of solar energy companies would completely tank as extremely less sunlight will reach earth's surface. Fourthly, as there would be extreme scarcity of sunlight, plants in order to perform photosynthesis would probably turn blackish or darkish green in order to absorb as much incident sunlight as possible. Lastly, as sun's gravitational pull would greatly reduce, outer planets of the solar system, namely Uranus and Neptune may drift away into space.

Discover how current science missions are revealing the mysteries of the Sun There is the Sun we know. It rises and sets at predictable times. It provides us light and warmth. But the Sun is so much more. Ground-based and space borne observatories have shown us that the Sun emits at all electromagnetic wavelengths. Spacecraft probing interplanetary space have detected magnetized fountains of charged particles emanating from the Sun’s multi-million degree corona. Seeing the Sun through polarized lenses, we know it is pervaded by magnetic fields. On the tenth anniversary of the Solar Dynamics Observatory, join Mark Cheung, senior staff physicist at the Lockheed Martin Advanced Technology Center, for an exploration of how the latest fleet of science missions from NASA and the National Science Foundation are revealing the mysteries of the Sun. See the Sun in all its true colors (from radio waves to X-rays), learn about its temper tantrums (solar storms), and experience the magnetic bond between the Sun and Earth. Let us learn to live with our star, and learn how our newfound wisdom guides us to finding habitable planets around other stars. The Exploring Space Lecture Series is made possible by the generous support of Aerojet Rocketdyne and United Launch Alliance. See More: airandspace.si.edu/event-series/exploring-space-lectures

Cameras aboard the United Launch Alliance Atlas V rocket captured the launch and deployment of the ESA/NASA Solar Orbiter on Feb. 9, 2020. About 20 hours later, the Schmidt telescope at Calar Alto, Spain was used to captured footage of it in the night sky. -- Solar Orbiter launches on historic mission to study the sun's poles: https://www.space.com/solar-orbiter-atlas-v-rocket-launch-success.html Credit: United Launch Alliance / ESA / mash mix by Space.com's Steve Spaleta (http://www.twitter.com/stevespaleta)

Earth’s magnetic field protects life on Earth from the intense radiation and titanic amounts of energetic material our Sun blasts in every direction. However, astronauts and satellites in space, future explorers travelling to the Moon and Mars, and infrastructure on Earth such as power grids and communication systems remain vulnerable to these violent outbursts. For this reason, ESA is planning to send a satellite to monitor the ‘side’ of our Sun, from a gravitationally stable position known as the fifth Lagrange point. From here, the Lagrange satellite will detect potentially hazardous solar events before they come into view from Earth, giving us advance knowledge of their speed, direction and chance of impact. ★ Subscribe: http://bit.ly/ESAsubscribe and click twice on the bell button to receive our notifications. Check out our full video catalog: http://bit.ly/SpaceInVideos Follow us on Twitter: http://bit.ly/ESAonTwitter On Facebook: http://bit.ly/ESAonFacebook On Instagram: http://bit.ly/ESAonInstagram On Flickr: http://bit.ly/ESAonFlickr We are Europe's gateway to space. Our mission is to shape the development of Europe's space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related. Copyright information about our videos is available here: http://www.esa.int/spaceinvideos/Terms_and_Conditions #ESA #Lagrange #SpaceSafety

On February 9, 2020, the European Space Agency’s Solar Orbiter spacecraft launched from Cape Canaveral Florida on top of an Atlas V 411 spacecraft. The spacecraft’s mission is to fly inside the orbit of Mercury, on a tilted orbit that takes it above and below the Sun, capturing images of the Sun’s poles for the first time. This is just a year and a half after the launch of NASA’s Parker Solar Probe, which will fly even closer. Together, the two spacecraft will measure the Sun from every angle up close, providing detailed images and insights of our closest star, to help understand how it creates and controls the giant bubble of plasma that surrounds the entire Solar System. Our Book is out! https://www.amazon.com/Universe-Today-Ultimate-Viewing-Cosmos/dp/1624145442/ Audio Podcast version: ITunes: https://itunes.apple.com/us/podcast/universe-today-guide-to-space-audio/id794058155?mt=2 RSS: https://www.universetoday.com/audio Weekly email newsletter: https://www.universetoday.com/newsletter Weekly Space Hangout: https://www.youtube.com/channel/UC0-KklSGlCiJDwOPdR2EUcg/ Astronomy Cast: https://www.youtube.com/channel/UCUHI67dh9jEO2rvK--MdCSg Support us at https://www.patreon.com/universetoday More stories at https://www.universetoday.com/ Twitch: https://twitch.tv/fcain Twitter: https://twitter.com/universetoday Facebook: https://www.facebook.com/universetoday Instagram - https://instagram.com/universetoday Team: Fraser Cain - @fcain / [email protected] Karla Thompson - @karlaii / https://www.youtube.com/channel/UCEItkORQYd4Wf0TpgYI_1fw Chad Weber - [email protected] References: https://sci.esa.int/web/solar-orbiter/-/liftoff-for-solar-orbiter-esa-s-mission-to-face-the-sun-up-close https://www.esa.int/Science_Exploration/Space_Science/Solar_Orbiter http://www.esa.int/ESA_Multimedia/Videos/2019/10/Solar_Orbiter_s_journey_around_the_Sun http://www.esa.int/Science_Exploration/Space_Science/Ulysses_overview https://solarsystem.nasa.gov/missions/ulysses/in-depth/ https://www.nasa.gov/content/solar-orbiter-overview https://sci.esa.int/web/solar-orbiter/-/51169-what-drives-the-solar-wind-and-where-does-the-coronal-magnetic-field-originate-from https://sci.esa.int/web/solar-orbiter/-/51170-how-do-solar-transients-drive-heliospheric-variability https://sci.esa.int/web/solar-orbiter/-/51171-how-do-solar-eruptions-produce-energetic-particle-radiation-that-fills-the-heliosphere https://sci.esa.int/web/solar-orbiter/-/51172-how-does-the-solar-dynamo-work-and-drive-connections-between-the-sun-and-the-heliosphere https://sci.esa.int/web/solar-orbiter/-/51217-instruments http://parkersolarprobe.jhuapl.edu/The-Mission/index.php https://www.eso.org/public/outreach/eduoff/vt-2004/mt-2003/mt-mercury-orbit.html https://www.esa.int/Enabling_Support/Space_Engineering_Technology/Paint_it_black_Stone_Age_sunscreen_for_Solar_Orbiter https://www.esa.int/Enabling_Support/Space_Engineering_Technology/Solar_Orbiter_s_shield_takes_Sun_s_heat

You’re looking at the highest resolution image that has ever been taken of our Sun, using the brand new Daniel K Inouye Solar Telescope in Maui. These lighter regions are convection cells, blobs of hot gas the size of Texas which have carried heat from deep below the surface of the Sun, releasing it into space. The darker lines are cooler regions, where the material is sinking back down into Sun. This image is just a demonstration of the incredible power of this 4-meter observatory, which will join NASA’s Parker Solar Probe and ESA’s Solar Orbiter in ushering in the golden age of solar astronomy. Our Book is out! https://www.amazon.com/Universe-Today-Ultimate-Viewing-Cosmos/dp/1624145442/ Audio Podcast version: ITunes: https://itunes.apple.com/us/podcast/universe-today-guide-to-space-audio/id794058155?mt=2 RSS: https://www.universetoday.com/audio Weekly email newsletter: https://www.universetoday.com/newsletter Weekly Space Hangout: https://www.youtube.com/channel/UC0-KklSGlCiJDwOPdR2EUcg/ Astronomy Cast: https://www.youtube.com/channel/UCUHI67dh9jEO2rvK--MdCSg Support us at https://www.patreon.com/universetoday More stories at https://www.universetoday.com/ Twitch: https://twitch.tv/fcain Twitter: https://twitter.com/universetoday Facebook: https://www.facebook.com/universetoday Instagram - https://instagram.com/universetoday Team: Fraser Cain - @fcain / [email protected] Karla Thompson - @karlaii / https://www.youtube.com/channel/UCEItkORQYd4Wf0TpgYI_1fw Chad Weber - [email protected] References: https://www.nso.edu/inouye-solar-telescope-first-light/ https://www.universetoday.com/144814/destructive-super-solar-storms-hit-us-every-25-years-or-so/ https://www.nasa.gov/mission_pages/stereo/news/stereo_astronauts.html https://www.nso.edu/telescopes/dkist/dkist-telescope/m1/ https://spie.org/news/1432-large-off-axis-mirrors-key-to-giant-astronomical-telescope?SSO=1 https://www.nso.edu/telescopes/dkist/fact-sheets/resisting-the-heat/ https://www.nso.edu/telescopes/dkist/dkist-telescope/tma/

You'll often hear people say that the Sun has about 5 billion years left to live before it runs out of fuel. But where does that number come from? It's quite a simple back of the envelope calculation but there are 7 key things we need to know before we can do that... For more on why E=mc2 see this article from Ethan Seigel: https://www.forbes.com/sites/startswithabang/2016/05/27/why-does-emc2/ To find out more on helioseismology and how we "listen to the Sun" check out this lecture: https://www.youtube.com/watch?v=wqwGljLDcjM 02:08 - the calculation of the lifetime of the Sun 05:23 - how we know the mass of the Sun 07:54 - how we know the distance between the Earth and the Sun 08:39 - how we measure the brightness of the Sun 09:44 - why E=mc2 11:04 - how we know the Sun is powered by nuclear fusion 13:35 - how we measured the mass difference between 4 Hydrogen atoms and 1 Helium atom 16:58 - how we know the core of the Sun is where nuclear fusion takes place (helioseismology) 19:02 - how we know how old the Solar System (and therefore the Sun) is ----- You can pre-order my book ' Space: 10 Things You Should Know' as a hardback (UK only) or e-book (worldwide): http://bit.ly/SpaceDrBecky ----------- Follow me on Twitter: https://twitter.com/drbecky_ And on Instagram: https://www.instagram.com/drbecky_s/ Don't forget to subscribe and click the little bell icon to be notified when I post a new video! ------ Dr Becky Smethurst is an astrophysicist researching galaxies and supermassive black holes at Christ Church at the University of Oxford. http://drbecky.uk.com

This Space Weather News forecast sponsored in part by Millersville University: https://www.millersville.edu/swen Space Weather has been calming down over the past few days since a solar storm hit Earth at the turn of the month. However, more fast solar wind is coming, which could give us another chance for aurora at high latitudes into the weekend, with views possibly extending down to mid-latitudes for a short while. Although sunspot 2757 has now rotated to the Sun's farside, we do have two new bright regions rotating into Earth-view on the Sun's east limb. These regions are helping to keep radio propagation on Earth's dayside in the marginal range. Expect solar flux to remain in the low 70s this week. GPS users should continue to enjoy good GPS reception on Earth's dayside thanks to a spotless Sun, but on Earth's nightside, GPS reception could get a little dicey near dawn and dusk, and anywhere near aurora once the solar storm hits. Learn the details of the coming fast solar wind, catch up on aurora photos from the recent storm, and see what else our Sun has in store! Want early access to these forecasts, tutorials on Space Weather, & more? Visit: https://patreon.com/SpaceweatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see links in my previous forecasts. I am saving this space for links to the aurora field report pictures highlighted this week: Aurora Photography: Teresa Cooper, Finland: https://twitter.com/Teresacooper/status/1222942313770557445 Hamza Khalifa, Sweden: https://twitter.com/hmkhalifa1985/status/1224106256333524993 Chalakorn P-S, Boden, Sweden: https://twitter.com/Chalakorn_ps/status/1224454712553959425 Bernardus Johannes, Laukvik, Lofoten, Norway: https://twitter.com/NLPLNO/status/1224032576085598208 Adrien Mauduit, Senja, Norway: https://twitter.com/NightLights_AM/status/1223060638139928576 I Need Space, Tromsø, Norway: https://twitter.com/INSVideos/status/1222845688851156994 Chris Cogan, Lairg Scotland: https://twitter.com/cogie_s/status/1223797150812966913 James Rowley-Hill, Glandale Skye, Scotland: https://twitter.com/chunder10/status/1222959383853912066 Live Aurora Network, Kirkjufell, Iceland: https://twitter.com/LiveAuroraNetw1/status/1222505553727033347 Notanee Bourassa, Regina, Saskatechewan, Canada: https://twitter.com/DJHardwired/status/1223480505565270016 Siv Heang, Calgary, Alberta, Canada: https://twitter.com/hoodoos84/status/1223056133885067264 Daniel Neal, Fairbanks, Alaska, USA: https://twitter.com/DLNphotos/status/1222250265383821312

Like our Facebook Page - https://www.facebook.com/astrobyte Astronomers have just released the highest-resolution image of the sun. Taken by the Daniel K. Inouye Solar Telescope in Maui, it gives us an unprecedented view of our nearest star and brings us closer to solving several long-standing mysteries. The new image demonstrates the telescope’s potential power. It shows off a surface that’s divided up into discrete, Texas-size cells, like cracked sections in the desert soil. You can see plasma oozing off the surface, rising high into the solar atmosphere before sinking back into darker lanes. “We have now seen the smallest details on the largest object in our solar system,” says Thomas Rimmele, the director of DKIST. The new image was taken December 10, when the telescope achieved first light. It is still technically under construction, with three more instruments set to come online. You're looking at the highest resolution observation of the Sun's surface ever taken. Collected over a period of 10 minutes, the footage from the Daniel K Inouye Telescope shows features as small as 18 miles in size. So, what does all this activity actually represent? The vicious movement of heat on a near-unimaginable scale. The National Solar Observatory (NSO) gives some staggering context: "The movie shows the turbulent, 'boiling' gas that covers the entire sun. The cell-like structures – each about the size of Texas – are the signature of violent motions that transport heat from the inside of the sun to its surface. Hot solar material (plasma) rises in the bright centers of 'cells,' cools off and then sinks below the surface in dark lanes in a process known as convection. In these dark lanes we can also see the tiny, bright markers of magnetic fields. Never before seen to this clarity, these bright specks are thought to channel energy up into the outer layers of the solar atmosphere called the corona. These bright spots may be at the core of why the solar corona is more than a million degrees!"

ESA’s mission to the Sun, Solar Orbiter, is due for launch on an Atlas V 411 from Cape Canaveral, Florida on 9 February 23:03 EST / 04:03 GMT / 05:03 CET on 10 Feb.   Equipped with a suite of ten scientific instruments, Solar Orbiter will capture the first images of the Sun’s poles and make detailed observations of solar activity. Its specially designed heatshield is capable of enduring temperatures of more than 500ºC. Solar Orbiter is a space mission of international collaboration between ESA and NASA. The spacecraft has been developed by Airbus. Learn more Solar Orbiter: http://bit.ly/ESASolarOrbiter ★ Subscribe: http://bit.ly/ESAsubscribe and click twice on the bell button to receive our notifications. Check out our full video catalog: http://bit.ly/SpaceInVideos Follow us on Twitter: http://bit.ly/ESAonTwitter On Facebook: http://bit.ly/ESAonFacebook On Instagram: http://bit.ly/ESAonInstagram On Flickr: http://bit.ly/ESAonFlickr We are Europe's gateway to space. Our mission is to shape the development of Europe's space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out http://www.esa.int/ESA to get up to speed on everything space related. Copyright information about our videos is available here: http://www.esa.int/spaceinvideos/Terms_and_Conditions #ESA #SolarOrbiter #WeAreAllSolarOrbiters

A new spacecraft is journeying to the Sun to snap the first pictures of the Sun’s north and south poles. Solar Orbiter, a collaboration between ESA (the European Space Agency) and NASA will have its first opportunity to launch from Cape Canaveral on Feb. 7, 2020, at 11:15 p.m. EST. Launching on a United Launch Alliance Atlas V rocket, the spacecraft will use Venus’ and Earth’s gravity to swing itself out of the ecliptic plane — the swath of space, roughly aligned with the Sun’s equator, where all planets orbit. From there, Solar Orbiter's bird’s eye view will give it the first-ever look at the Sun's poles. Read more: https://www.nasa.gov/feature/goddard/2020/new-mission-will-take-first-peek-at-sun-s-poles Music credits: “Oxide” and “Virtual Tidings” by Andrew Michael Britton [PRS], David Stephen Goldsmith [PRS]; “Progressive Practice” by Emmanuel David Lipszc [SACEM], Franck Lascombes [SACEM], Sebastien Lipszyc [SACEM]; “Political Spectrum” by Laurent Dury [SACEM] from Universal Production Music. Credit: NASA's Goddard Space Flight Center Holly Gilbert (NASA/GSFC): Scientist Teresa Nieves-Chinchilla (Catholic University of America): Scientist Chris St. Cyr (NASA/GSFC): Scientist Joy Ng (USRA): Producer Tom Bridgman (GST): Data Visualizer Adriana Manrique Gutierrez (USRA): Animator Chris Smith (USRA): Animator Joy Ng (USRA): Animator Lisa Poje (USRA): Animator Krystofer Kim (USRA): Animator Brian Monroe (USRA): Animator Miles S. Hatfield (Telophase): Writer This video is public domain and along with other supporting visualizations can be downloaded from NASA Goddard's Scientific Visualization Studio at: https://svs.gsfc.nasa.gov/13527 If you liked this video, subscribe to the NASA Goddard YouTube channel: https://www.youtube.com/NASAGoddard Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASAGoddard · Flickr http://www.flickr.com/photos/gsfc

There’s a wind that emanates from the Sun. It blows not like a soft whistle but like a hurricane’s scream. Made of electrons, protons and heavier ions, the solar wind courses through the solar system at roughly 1 million mph (1.6 million kph), barreling over everything in its path. Yet through the wind’s roar, NASA’s Parker Solar Probe hears the small chirps, squeaks and rustles that hint at the origin of this mysterious and ever-present wind. The spacecraft’s FIELDS instrument can eavesdrop on the electric and magnetic fluctuations caused by plasma waves. The Parker Solar Probe it can “hear” when the waves and particles interact with one another, recording frequency and amplitude information about these plasma waves that scientists could then play as sound waves. And it results in some striking sounds. Solar wind sounds playlist: https://soundcloud.com/jhu-apl/sets/sounds-of-the-solar-wind Learn more about the Sounds of the Solar Wind: https://www.jhuapl.edu/FeatureStory/200114 More on solar wind sound from the Parker Solar Probe: http://parkersolarprobe.jhuapl.edu/News-Center/Show-Article.php?articleID=139

This SFN Sponsored by Mova Globes: http://bit.ly/deepastronMOVAGlobes Get GREAT Telescope Gear from a GREAT company OPT Telescopes (aff link): http://bit.ly/2Wq0BO8 Ever wonder what’s going to happen to the outer planets of our solar system when the Sun turns into a red giant star? Will they survive or will the get flung out into space? Will Jupiter, Saturn and Neptune evaporate? This week astronomers found some clues to these questions from observations of a white dwarf that appears to have a planet at least twice as large as the star itself. #WhiteDwarfStar #DeathOfSun #SpaceFanNews Join our Chat on Discord here: https://discord.gg/nqGpvtK Like this content? Please consider becoming a patron: https://patreon.com/DeepAstronomy Follow DeepAstronomy on Twitter: @DeepAstronomy Like DeepAstronomy on Facebook: https://www.facebook.com/DeepAstronomy/

Scientists have revealed the results of the Parker Solar Probe’s first two flybys of the Sun, and LIGO has a new instrument called the quantum vacuum squeezer! Hosted by: Caitlin Hofmeister SciShow has a spinoff podcast! It's called SciShow Tangents. Check it out at http://www.scishowtangents.org ---------- Support SciShow by becoming a patron on Patreon: https://www.patreon.com/scishow ---------- Huge thanks go to the following Patreon supporters for helping us keep SciShow free for everyone forever: Kevin Carpentier, Eric Jensen, Matt Curls, Sam Buck, Christopher R Boucher, Avi Yashchin, Adam Brainard, Greg, Alex Hackman, Sam Lutfi, D.A. Noe, Piya Shedden, Scott Satovsky Jr, Charles Southerland, Patrick D. Ashmore, charles george, Kevin Bealer, Chris Peters ---------- Like SciShow? Want to help support us, and also get things to put on your walls, cover your torso and hold your liquids? Check out our awesome products over at DFTBA Records: http://dftba.com/scishow ---------- Looking for SciShow elsewhere on the internet? Facebook: http://www.facebook.com/scishow Twitter: http://www.twitter.com/scishow Tumblr: http://scishow.tumblr.com Instagram: http://instagram.com/thescishow ---------- Sources: https://www.nature.com/articles/d41586-019-03665-3 https://www.nasa.gov/press-release/first-nasa-parker-solar-probe-results-reveal-surprising-details-about-our-sun https://www.nasa.gov/mission_pages/iris/multimedia/layerzoo.html http://parkersolarprobe.jhuapl.edu/The-Mission/index.php#introduction http://news.mit.edu/2019/ligo-reach-quantum-noise-wave-1205 Images: https://svs.gsfc.nasa.gov/12911 http://parkersolarprobe.jhuapl.edu/The-Mission/index.php#Where-Is-PSP https://svs.gsfc.nasa.gov/30481 https://svs.gsfc.nasa.gov/12704 https://svs.gsfc.nasa.gov/13113 https://svs.gsfc.nasa.gov/20299 https://svs.gsfc.nasa.gov/13105 https://svs.gsfc.nasa.gov/11086 https://commons.wikimedia.org/wiki/File:Initial_and_Enhanced_LIGO_schematics.png

This Solar Storm Forecast is sponsored in part by 3ric Johanson: http://instagram.com/scubist Space weather this week remains on the quiet side, but we are continuing to see a slight boost in the solar flux due to emergence of small bright regions in Earth view. Some of these regions are at high latitudes, which is indicative of the new solar cycle trying to take hold. These regions dont last too long, but their constant presence is enough to boost radio propagation and keep it in the marginal range. This boost is expected to continue throughout this week. In addition, we have a weak coronal hole rotating through the Earth-strike zone, which will bring a weak fast solar wind stream, likely causing aurora at high latitudes. However, it will not be enough to bump us anywhere close to solar storm levels so mid-latitude aurora photographers will just have to sit this one out. GPS users should find this weak storm helps to stabilize the upper atmosphere so their GPS reception should remain pretty robust, even at low latitudes. As always, be careful with GPS reception anywhere near aurora, especially near the dawn-dusk terminators. Learn the details of the coming fast solar wind, see when yet another fast wind stream is coming, and find out what else our Sun has in store! Want early exclusive views of these forecasts and more? Join my Patreon community: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

You can buy Universe Sandbox 2 here: http://amzn.to/2yJqwU6 Or get a shirt: https://teespring.com/stores/whatdamath Hello and welcome! My name is Anton and in this video, we will talk about new discoveries coming from the Parker Solar Probe. Papers: http://www.nature.com/articles/s41586-019-1818-7 https://www.nature.com/articles/s41586-019-1813-z https://www.nature.com/articles/s41586-019-1818-7 https://www.nature.com/articles/s41586-019-1818-7 Support this channel on Patreon to help me make this a full time job: https://www.patreon.com/whatdamath Space Engine is available for free here: http://spaceengine.org Enjoy and please subscribe. Twitter: https://twitter.com/WhatDaMath Facebook: https://www.facebook.com/whatdamath Twitch: http://www.twitch.tv/whatdamath Bitcoins to spare? Donate them here to help this channel grow! 1GFiTKxWyEjAjZv4vsNtWTUmL53HgXBuvu The hardware used to record these videos: CPU: https://amzn.to/2LZFQCJ Video Card: https://amzn.to/2M1W26C Motherboard: https://amzn.to/2JYGiQQ RAM: https://amzn.to/2Mwy2t4 PSU: https://amzn.to/2LZcrIH Case: https://amzn.to/2MwJZz4 Microphone: https://amzn.to/2t5jTv0 Mixer: https://amzn.to/2JOL0oF Recording and Editing: https://amzn.to/2LX6uvU Thank you to all Patreon supporters of this channel Specifically, great thanks to the following members: Morrison Waud Vlad Manshin Mark Teranishi TheHuntress Daniel Rosvall Ralph Spataro Lilith Dawn Albert B. Cannon Greg Lambros adam lee Jer Henry Spadoni Nick Dolgy Konrad Kummli UnexpectedBooks.com J Carter Gabriel Seiffert Shinne George Williams Jakub Glos Johann Goergen Lyndon Riley LS Greger Jake Salo Michael Tiganila Lauren Smith Olegas Budnik Dave Blair Sander Stols Kai Raphahn Sergio Ruelas Arikkat Unnikrishnan Steven Becky Tracy Burgess Gordon Cooper Steve Wotton Jayjay Volz Anataine Deva Honey Suzanne Lyons Daniel Coleman Matthew Lazear xyndicate Steven Aiello

Launched in 2018, NASA’s Parker Solar Probe spacecraft, with instruments developed and built by UC Berkeley, has now travelled closer to the sun than any other mission in history, actually penetrating the sun’s atmosphere, to investigate highly charged magnetic field. Now, that data has allowed solar physicists to map the source of a major component of the solar wind that continually peppers Earth’s atmosphere, while revealing strange magnetic field reversals that could be accelerating these particles toward our planet. These accelerated particles interact with Earth’s magnetic field, generating the colorful northern and southern lights but also potentially damaging the electrical grid and telecommunications networks on the surface, threatening orbiting satellites and perhaps endangering astronauts in space. The more solar physicists understand about the magnetic environment of the sun and how it flings solar wind particles out toward the planets, the better they will be able to predict events to prevent damage. “There was a major space weather event in 1859 that blew out telegraph networks on Earth and one in 1972 that set off naval mines in North Vietnam, just from the electrical currents generated by the solar storm,” said Stuart Bale, a University of California, Berkeley, professor of physics and lead author of an article about new results from the probe’s FIELDS experiment. “We’re much more of a technological society than we were in 1972, the communications networks and the power grid on Earth are extraordinarily complex, so big disturbances from the sun are potentially a very serious thing. If we could predict space weather, we could shut down or isolate parts of the power grid, or shut down satellite systems that might be vulnerable.” (Cont'd...) (Full Story: https://news.berkeley.edu/2019/12/04/parker-probe-traces-solar-wind-to-its-source-on-suns-surface/) Video by Roxanne Makasdjian and Stephen McNally (Animations and images courtesy of: NASA/JHUAPL, NASA GSFC/CIL/Brian Monroe, NASA GSFC/CIL/Krystofer Kim, Johns Hopkins University/APL/Steve Gribben) http://news.berkeley.edu/ http://www.facebook.com/UCBerkeley http://twitter.com/UCBerkeley http://instagram.com/ucberkeleyofficial

Parker Solar Probe - NASA's mission to touch the Sun - has revealed new discoveries about our star. Principal Investigators for some of the mission's instruments share their excitement about this new science.

NASA's Parker Solar Probe mission has returned unprecedented data from near the Sun, culminating in new discoveries published on Dec. 4, 2019, in the journal Nature. Among the findings are new understandings of how the Sun's constant outflow of material, the solar wind, behaves. Seen near Earth -- where it can interact with our planet's natural magnetic field and cause space weather effects that interfere with technology -- the solar wind appears to be a relatively uniform flow of plasma. But Parker Solar Probe's observations reveal a complicated, active system not seen from Earth. Music Credit: Smooth as Glass by The Freeharmonic Orchestra Read more: https://www.nasa.gov/feature/goddard/2019/nasas-parker-solar-probe-sheds-new-light-on-the-sun/ Video Credit: NASA's Goddard Space Flight Center Karen Fox (ADNET): Writer Sarah Frazier (ADNET): Writer Genna Duberstein (USRA): Producer Genna Duberstein (USRA): Editor Chris Smith (USRA): Narrator Adriana Manrique Gutierrez (USRA): Animator Jonathan North (USRA): Animator Scott Wiessinger (USRA): Animator Adam Szabo (NASA/GSFC): Scientist Russ Howard (NRL): Scientist Dave McComas (SwRI): Scientist Stuart Bale (University of California, Berkeley): Scientist Justin Kasper (University of Michigan): Scientist Nour Raouafi (Johns Hopkins University/APL): Scientist Eric Christian Ph.D. (NASA/HQ): Scientist Adam Szabo (NASA/GSFC): Project Support Please give credit for this item to: NASA's Goddard Space Flight Center This video is public domain and along with other supporting visualizations can be downloaded from the Scientific Visualization Studio at: http://svs.gsfc.nasa.gov/13282 If you liked this video, subscribe to the NASA Goddard YouTube channel: http://www.youtube.com/NASAExplorer Follow NASA’s Goddard Space Flight Center · Instagram http://www.instagram.com/nasagoddard · Twitter http://twitter.com/NASAGoddard · Twitter http://twitter.com/NASAGoddardPix · Facebook: http://www.facebook.com/NASA.GSFC · Flickr http://www.flickr.com/photos/gsfc

Stars such as our Sun burn hydrogen in their cores for most of their lives. Once they run out of this fuel, they puff up into red giants, becoming hundreds of times larger and engulfing nearby planets. As shown in this animation, in the case of the Solar System this will include Mercury, Venus, and even Earth, which will all be consumed by the red-giant Sun in about 5 billion years. Eventually, Sun-like stars lose their outer layers, leaving behind only a burnt-out core, a white dwarf. Such stellar remnants can still host planets, and many of these stars exist in our galaxy. However, until 2019, scientists had never found evidence of a surviving giant planet around a white dwarf. The detection of a Neptune-like exoplanet at WDJ0914+1914 may be the first of many orbiting such stars. More information and download options: http://www.eso.org/public/videos/eso1919c/ Credit: ESA/Hubble (M. Kornmesser & L. L. Christensen)

This episode of Space Weather News is sponsored in part by 3ric Johanson: http://instagram.com/scubist Happy Thanksgiving! Space Weather remains unsettled this week as we have some more fast solar wind from a southern hemisphere coronal hole hitting Earth in the next day or so. Although this fast wind will be pretty weak overall, it should keep us at unsettled conditions through the weekend. It will also bring aurora shows to high latitudes in through the weekend before settling down. Although the aurora never made it very far south during the previous solar storm last week, we do have the Unicorn meteor shower to thank for the bolide that exploded over southern Wisconsin a few days ago. As reports continue to surface, it turns out that this bolide was seen by many people over a large geographical range. Though most sightings were in Wisconsin, there have been multiple reports in places like California, South Dakota, and Ontario Canada! Learn the details of the coming fast solar wind, watch the new cycle 25 bright region peek up through the coronal hole and boost solar flux back into the marginal range for radio propagation, and see what else our Sun has in store for us! Want to see this forecast earlier than the public release? Join my Patreon Community: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Field Reporting & Aurora Photos: Notanee Bourassa, Regina, Saskatchewan, Canada: https://twitter.com/DJHardwired/status/1199212280132489217 Ollie Taylor, Durness, Scotland: https://twitter.com/OllieTPhoto/status/1198278462185902081 EK3, Madison Wisconsin, USA: https://twitter.com/EK14MeV/status/1198502507531649024 AOSSRooftopCameras, University of Wisconsin, USA: https://www.youtube.com/watch?time_continue=10&v=5uMOH2TXbpA&feature=emb_logo Jenny Thiele: https://twitter.com/jenny_thiele/status/1199368271008583681 American Meteor Society: https://www.youtube.com/watch?v=zTjtv0-w2EE Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

The continuously expanding solar wind begins in our Sun and doesn’t stop until after it reaches the edge of the heliosphere. NASA Science: http://science.nasa.gov/

We speak to Prof Richard Harrison about the European Space Agency's Solar Orbiter mission, which will observe the Sun close up and examine how the heliosphere impacts both Earth and the rest of the Solar System.

Let's talk about science! Watch the third episode of our #EZScience series to learn about an essential part of our lives: the Sun. Discover how spacecraft such as NASA’s Parker Solar Probe are exploring the wonders of our closest star. ABOUT THE SERIES: In our #EZScience video series with the National Air and Space Museum, NASA's associate administrator for science Dr. Thomas Zurbuchen and Museum director Dr. Ellen Stofan talk about the latest in planetary science and exploration. Learn more: https://www.nasa.gov/ezscience

The international Hinode solar-observing satellite captured the transit of Mercury as it passed between Earth and the Sun on Nov. 11, 2019. Transits like this can be used to measure the distance between Earth and the Sun. Hinode is a joint endeavor by the Japan Aerospace Exploration Agency (JAXA), National Astronomical Observatory of Japan (NAOJ), European Space Agency, United Kingdom Space Agency and NASA. These images were taken with Hinode's X-Ray Telescope (XRT), which observes the solar atmosphere at millions of degrees. Additional movies from the XRT are available from the Harvard-Smithsonian Center for Astrophysics and JAXA. Image credit: JAXA/NASA/SAO/Montana State University/NAOJ

Welcome to Amazing Space Videos - This video of one month of solar activity was created using images from NASA SDO - almost 3000 separate photos were used. A few facts about the Sun FACTS ABOUT THE SUN The Sun accounts for 99.86% of the mass in the solar system. It has a mass of around 330,000 times that of Earth. It is three-quarters hydrogen and most of its remaining mass is helium. Over one million Earth’s could fit inside the Sun. If you were to fill a hollow Sun with spherical Earths, somewhere around 960,000 would fit inside. However, if you squashed those Earths to ensure there was no wasted space then you could fit 1,300,000 Earths inside the Sun. The surface area of the Sun is 11,990 times that of Earth. One day the Sun will consume the Earth. The Sun will continue to burn for about 130 million years after it burns through all of its hydrogen, instead burning helium. During this time it will expand to such a size that it will engulf Mercury, Venus, and Earth. When it reaches this point, it will have become a red giant star. The energy created by the Sun’s core is nuclear fusion. This huge amount of energy is produced when four hydrogen nuclei are combined into one helium nucleus. The Sun is almost a perfect sphere. Considering the sheer size of the Sun, there is only a 10 km difference in its polar and equatorial diameters – this makes it the closest thing to a perfect sphere observed in nature. The Sun is travelling at 220 km per second. It is around 24,000-26,000 light-years from the galactic centre and it takes the Sun approximately 225-250 million years to complete one orbit of the centre of the Milky Way. The Sun will eventually be about the size of Earth. Once the Sun has completed its red giant phase, it will collapse. It’s huge mass will be retained, but it will have a volume similar to that of Earth. When that happens, it will be known as a white dwarf. It takes eight minutes for light reach Earth from the Sun. The average distance from the Sun to the Earth is about 150 million km. Light travels at 300,000 km per second so dividing one by the other gives you 500 seconds – eight minutes and twenty seconds. This energy can reach Earth in mere minutes, but it takes millions of years to travel from the Sun’s core to its surface. The Sun is halfway through its life. At 4.5 billion years old, the Sun has burned off around half of its hydrogen stores and has enough left to continue burning hydrogen for another 5 billion years. Currently the Sun is a yellow dwarf star. The distance between Earth and Sun changes. This is because the Earth travels on a elliptical orbit path around the Sun. The distance between the two ranges from 147 to 152 million km. This distance between them is one Astronomical Unit (AU). The Sun rotates in the opposite direction to Earth with the Sun rotating from west to east instead of east to west like Earth. Find out more here: https://theplanets.org/the-sun/ Twitter: https://twitter.com/AmazingSpace2 Google+ : http://goo.gl/1WCBn9

Welcome to Amazing Space Videos - A totally unique view of our Sun: A complete month of solar activity as captured by NASA's Solar Dynamics Observatory (SDO). The SDO captures an image every 12 seconds in multiple wavelengths - this video shows wavelength 304 and shows every image taken by the satellite during a one month period. Thanks for watching - why not support this channel and help us grow. https://www.youtube.com/channel/UCakgsb0w7QB0VHdnCc-OVEA/join Subscribe For More Videos Like This: http://www.youtube.com/user/ouramazingspace?sub_confirmation=1 See my latest videos : https://www.youtube.com/user/ouramazingspace/videos Bringing you the BEST Space and Astronomy videos online. Showcasing videos and images from the likes of NASA,ESA,Hubble etc. Join me on Facebook: https://www.facebook.com/spaceisamazing Twitter: https://twitter.com/AmazingSpace2 Google+ : http://goo.gl/1WCBn9 Music by Keving Macleod http://incompetech.com/music/royalty-free/

This episode of Weather News is sponsored in part by 3ric Johanson: http://instagram.com/scubist A new sunspot has emerged on the Earth-facing disk and it has been firing a bunch of mini-solar flares, which could be causing just a tiny bit of noise on the dayside amateur radio bands. As of yet it hasnt launched any solar storms towards Earth, but we are watching it closely. We also have a coronal hole in the southern hemisphere that will be rotating into the Earth-strike zone within the next day or so. Aurora photographers at high latitudes might also be in for some fun as we could get sporadic aurora shows over the next few days from the coming fast solar wind. However, the chances of mid-latitude aurora is pretty fleeting. Despite this new activity, solar flux will remain in the high 60's with poor radio propagation in general on Earth's dayside and GPS reception should remain good, even at low latitudes. Learn the details of the new active region, what to expect with the coming fast solar wind, and see what else the Sun has in store. Want early access to these forecasts and more? Join me at: http://patreon.com/spaceweatherwoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

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Get a 14 day free trial with Shopify using this link: https://www.shopify.com/realengineering Real Engineering Notebook: https://standard.tv/collections/real-engineering New streaming platform: https://watchnebula.com/ Vlog channel: https://www.youtube.com/channel/UCMet4qY3027v8KjpaDtDx-g Patreon: https://www.patreon.com/user?u=2825050&ty=h Facebook: http://facebook.com/realengineering1 Instagram: https://www.instagram.com/brianjamesmcmanus Reddit: https://www.reddit.com/r/RealEngineering/ Twitter: https://twitter.com/thebrianmcmanus Discord: https://discord.gg/s8BhkmN Get your Real Engineering shirts at: https://standard.tv/collections/real-engineering Credits: Writer/Narrator: Brian McManus Editor: Stephanie Sammann (https://www.stephanie-sammann.com/) Animator: Mike Ridolfi (https://www.moboxgraphics.com/) Sound: Graham Haerther (https://haerther.net/) Thumbnail: Simon Buckmaster https://twitter.com/forgottentowel References: [1] https://directory.eoportal.org/web/eoportal/satellite-missions/content/-/article/sdo [2] https://science.nasa.gov/science-news/science-at-nasa/2014/23jul_superstorm/ [3] https://science.nasa.gov/science-news/science-at-nasa/2008/06may_carringtonflare [4] http://www.hydroquebec.com/learning/notions-de-base/tempete-mars-1989.html [5] https://www.nasa.gov/topics/earth/features/sun_darkness.html [6] https://www.rpi.edu/dept/phys/ScIT/InformationStorage/faraday/magnetism_a.html [7] https://www.scientificamerican.com/article/geomagnetic-storm-march-13-1989-extreme-space-weather/ [8] https://www.sciencedirect.com/science/article/pii/B9780128124413000161 [9] https://www.nerc.com/comm/PC/Geomagnetic%20Disturbance%20Task%20Force%20GMDTF%202013/GMD%20Planning%20Guide_approved.pdf [10] https://www.swpc.noaa.gov/impacts/space-weather-and-gps-systems [11] https://ieeexplore.ieee.org/document/6281595 [12] https://www.allaboutcircuits.com/textbook/alternating-current/chpt-9/practical-considerations-transformers/ [13] https://www.gao.gov/assets/700/696140.pdf [14] https://relays.weebly.com/electromechanical-relays.html [15] https://catalog.hathitrust.org/Record/005695782 [16] https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2011SW000715#swe481-fig-0004 Thank you to AP Archive for access to their archival footage. Music by Epidemic Sound: http://epidemicsound.com/creator Songs: Atomic Numbers 2 - August Wilhelmsson Timepass - Marten Moses Stay Near - Luwaks A Key Figure - David Celeste The Night Lights - Rippled Stone Reflective Mood - Heath Cantu Thank you to my patreon supporters: Adam Flohr, Henning Basma, Hank Green, William Leu, Tristan Edwards, Ian Dundore, John & Becki Johnston. Nevin Spoljaric, Jason Clark, Thomas Barth, Johnny MacDonald, Stephen Foland, Alfred Holzheu, Abdulrahman Abdulaziz Binghaith, Brent Higgins, Dexter Appleberry, Alex Pavek, Marko Hirsch, Mikkel Johansen, Hibiyi Mori. Viktor Józsa, Ron Hochsprung

This episode of Weather News is sponsored in part by 3ric Johanson: http://instagram.com/scubist Want early access to these forecasts and more? Join me at: http://patreon.com/spaceweatherwoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

The sun is our great ball of energy at the centre of the solar system... But what would happen if it was double the size? In this video, Unveiled discovers why having more of the sun might not be such a good thing... Any why we should be very thankful that Earth is positioned exactly where it is in space; at exactly the right distance away from the sun to allow for life to thrive! This is Unveiled, giving you incredible answers to extraordinary questions! Find more amazing videos for your curiosity here: What If Humanity Built a Dyson Sphere in the Solar System? - https://www.youtube.com/watch?v=fI9DZv3hWqg What's Hiding on the Dark Side of the Moon? - https://www.youtube.com/watch?v=JPRmbP3xWl8 Are you constantly curious? Are you a fiend for facts? Then subscribe for more from Unveiled ► https://goo.gl/GmtyPv #Space #SolarSystem #Sun #Solar #WhatIf

This episode of Weather News is sponsored in part by 3ric Johanson: http://instagram.com/scubist Our Sun remains quiet this week, but a promise of a solar storm is rotating into view! A familiar set of coronal holes have survived their passage on the backside of the Sun and are returning. The last time these holes crossed the Earth-strike zone they sent us some fast solar wind that caused a G1 solar storm and brought aurora deep into mid-latitudes. We will get another chance very soon to see if they can do it again! Meanwhile, solar flux remains low so radio propagation is still poor on the dayside of Earth. However, the low solar flux is contributing to decent GPS reception, even at low latitudes. Learn more about the returning coronal holes, when we should expect another solar storm, how the local satellite environment is doing, and what else our Sun has in store. Want early access to these forecasts and more? Join me at: http://patreon.com/spaceweatherwoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

Declassified Vietnam War files are showing researchers the unpredictable nature of the Sun and helping them work toward predicting the next big solar storm. » Subscribe to Seeker! http://www.youtube.com/subscription_center?add_user=dnewschannel » Watch more Focal Point! | https://bit.ly/2Z7LHgi Traveling at the near-speed of light, energetic particles shooting out from the Sun can zip through space, smack into our planet’s atmosphere, and cause incredible disruptions. And one of the biggest impacts we know of happened during the tail end of the Vietnam War. On this episode of Focal Point, we hear from Delores Knipp, a space weather scientist and former officer in the U.S. Air Force who uncovered a war mystery that is now connected to a major solar event. And Howard Singer, the chief scientist at the NOAA Space Weather Prediction Center. In 1972, a solar flare, or solar storm, traveled at about 2,800 kilometers per second, which was seven times faster than the norm, and it carried tremendous magnetic field, and mass with it. A dozen sea mines exploded and everyone chalked it up to Vietnam warfare, but it was actually the solar flares. The bits of Sun slammed into the Earth’s magnetosphere within 15 hours and triggered the sea mines. So how much do we know about solar flares and what's the chance another event could happen again? Learn more on this episode of Focal Point. #SolarStorm #SolarFlares #Science #VietnamWar #Seeker #FocalPoint Read More: A 1972 solar storm triggered a Vietnam War mystery https://www.colorado.edu/today/2018/11/12/1972-solar-storm-triggered-vietnam-war-mystery “On Aug. 4, 1972, U.S. military pilots flying south of Haiphong harbor in North Vietnam saw something unexpected. More than two dozen sea mines suddenly—and without apparent explanation—exploding in the water.” Understanding the Magnetic Sun https://www.nasa.gov/feature/goddard/2016/understanding-the-magnetic-sun “The sun's magnetic field is responsible for everything from the solar explosions that cause space weather on Earth – such as auroras – to the interplanetary magnetic field and radiation through which our spacecraft journeying around the solar system must travel.” Space Weather Frequently Asked Questions https://www.swpc.noaa.gov/content/space-weather-faq-frequently-asked-questions “Space weather is noticed mostly by its effects on Earth. After a great solar flare in 1859, telegraph operators discovered that currents from the intense aurora borealis was flowing through their systems, causing their telegraph keys to melt and stick in position.” Sign Up For The Seeker Newsletter Here - http://bit.ly/1UO1PxI ____________________ Seeker inspires us to see the world through the lens of science and evokes a sense of curiosity, optimism and adventure. Visit the Seeker website https://www.seeker.com/ Subscribe now! https://www.youtube.com/user/DNewsChannel Seeker on Twitter http://twitter.com/seeker Seeker on Facebook https://www.facebook.com/SeekerMedia/ Seeker http://www.seeker.com/

This episode of Weather News is sponsored in part by 3ric Johanson: http://instagram.com/scubist Our Sun calms down this week as region 2745 rotates off the west limb and on to the backside. We are dealing with a slight enhancement due to some mildly fast solar wind that could bump us to active conditions over the next few days, but only at high latitudes. On a more exciting front, a returning set of coronal holes rotates into view, which could bump us to storm levels with some decent fast solar wind in about 10 days. This should give aurora photographers something to anticipate. Unfortunately, the bright regions that were sandwiched between these coronal holes have decayed severely. They will not boost the solar flux much, if at all, for amateur radio operators and emergency responders. This means radio propagation will remain poor on Earth's dayside for at least another week or (likely) more. At least the quiet Space Weather means GPS users can expect great reception on Earth's dayside and at low latitudes over the next week. Want early bird viewing of these forecasts? Go to: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

This episode of Weather News is sponsored in part by 3ric Johanson: http://instagram.com/scubist This week our Sun gives us one more reason to believe Solar Cycle 25 is coming! Another new cycle sunspot, this time in the southern hemisphere has not only appeared in Earth view, but it has lingered! It even managed to fire off a couple of B-class flares before going quiet. This may be the first "real" activity that can be officially assigned to the upcoming Solar Cycle 25. In addition to this great news, we also have multiple coronal holes that have (or will be) rotating in through the Earth-strike zone this week. One of them sent strong enough fast wind our way to cause aurora clear down to Wyoming. The next burst of fast wind should hit around Monday into Tuesday. As for solar flux, its in the dumper and will continue to remain in the high 60s for the remainder of the week. This means radio propagation on Earth's dayside continues to be poor for emergency responders and amateur radio operators. However, the low solar flux and low solar activity means GPS reception on the dayside of Earth will continue to be great this week. Learn more about the new cycle sunspot and see what else our star has in store this week. Want early bird viewing of these forecasts? Go to: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

This episode of Space Weather News sponsored in part by 3ric Johanson: http://instagram.com/scubist Our Sun may be quiet, but Space Weather is not! This past week we had a meteor (bolide) explode over the skies near Puerto Rico in a spectacle equivalent to a 3-5 kiloton detonation! The size of this meteor was about the same as the meteor that created the new impact crater on Mars so that should give us all pause. On top of that, there is going to be a total solar eclipse over the South Pacific and South America on July 2nd. Be sure to watch your skies if you are in the region and check online, live solar telescope feeds, if you arent! If you are a radio communicator or use GPS/GNSS and are in the path of totality on July 2, you might experience some glitches in your comms or reception as the moon's shadow passes over you, so be aware. As for the weather from our star, the solar wind will likely remain disturbed over the next few days, but it should be minor. Also, some bright regions return to Earth view here in the next few days so radio propagation could bump back to the low end of marginal on Earth's dayside. Learn the details of this week's events. I have included links to the predictions of the solar corona for the eclipse from my colleagues at Predictive Science Inc. as well as links to the fantastic field reporting of the meteor blast near Puerto Rico, below. For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Predictive Science Eclipse Predictions: http://www.predsci.com/corona/jul2019eclipse/pb.php http://www.predsci.com/corona/jul2019eclipse/home.php Field Reporting for the Meteor: Frankie Lucena: https://twitter.com/frankie57pr/status/1143323684406534146 Peter Brown: https://twitter.com/pgbrown/status/1143264346837082112 Ernesto Guido: https://twitter.com/comets77/status/1143546624532275201 YE Quanzhi: https://twitter.com/Yeqzids/status/1143275764118253569 ATLAS Project: https://twitter.com/fallingstarIfA/status/1143700124226347008 Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

The Swedish 1-Meter telescope captured amazing imagery of the Sun in 2016. -- Sun's Pulsing 'Skin' in Incredible Detail: https://www.space.com/animation-shows-sun-photosphere-pulsing.html Credit: Space.com / imagery: Swedish 1-Meter telescope & NASA/GSFC / produced & edited by Steve Spaleta

Go to http://www.curiositystream.com/joescott to get 30 days of CuriosityStream for free. It's awesome. Do it. The sun is a solar flare machine, constantly spitting out waves of charged particles in all directions. Sometimes these hit Earth. Luckily we're protected by a strong magnetic field that directs the particles to the poles, which we experience as the Northern Lights, or Aurora Borealis. But from time to time, the sun erupts in a massive superflare, also known as a CME or Coronal Mass Ejection. These can push our magnetic shield to its limits and actually cause electrical problems on the ground. One of the worst instances of a CME striking the Earth occurred in 1859. It disrupted the telegraph system and sent sparks flying out of switchboards. It became known as the Carrington Event and begs the question - what if it happened today? Support me on Patreon! http://www.patreon.com/answerswithjoe Get cool nerdy t-shirts at http://www.answerswithjoe.com/shirts Interested in getting a Tesla? Use my referral link and get discounts and perks: https://ts.la/joe74700 Become a channel member and get access to exclusive livestreams and content here: https://www.youtube.com/channel/UC-2YHgc363EdcusLIBbgxzg/join Follow me at all my places! Instagram: https://instagram.com/answerswithjoe Snapchat: https://www.snapchat.com/add/answerswithjoe Facebook: http://www.facebook.com/answerswithjoe Twitter: https://www.twitter.com/answerswithjoe LINKS LINKS LINKS: Carrington Event animation: https://www.youtube.com/watch?v=dVS4Q4VgDxk http://blogs.discovermagazine.com/d-brief/2019/06/12/sun-star-superflare/#.XQFIVI97mUk https://www.history.com/news/a-perfect-solar-superstorm-the-1859-carrington-event, https://io9.gizmodo.com/how-the-carrington-event-let-telegraphs-run-on-aurora-p-1686759750 http://www.solarstorms.org/NewsPapers/d1989c.pdf https://www.airspacemag.com/space/the-invisible-killers-11257197/ https://science.nasa.gov/science-news/science-at-nasa/2005/27jan_solarflares/ https://www.space.com/33687-solar-storm-cold-war-false-alarm.html

This episode of Space Weather News sponsored in part by 3ric Johanson: http://instagram.com/scubist Description coming momentarily... For early access to this forecast and more visit: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Noctilucent Cloud Field Reporting: Paul Smith, Freedom, Oklahoma: http://spaceweathergallery.com/indiv_upload.php?upload_id=154110 Zach Schierl, Cedar Breaks National Monument, Utah: http://spaceweathergallery.com/indiv_upload.php?upload_id=154018 Ed Brooks, San Francisco, CA: http://spaceweathergallery.com/indiv_upload.php?upload_id=154061 Knut Schäffner, Germany: http://spaceweathergallery.com/indiv_upload.php?upload_id=153996 Sylvain, Paris, FRANCE http://spaceweathergallery.com/indiv_upload.php?upload_id=154195 Forrest Hamilton, Deacon, Indiana: http://spaceweathergallery.com/indiv_upload.php?upload_id=154182 Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

This mini-course is made by and for patrons of Patreon. Without their generous support, this course wouldnt be possible. Come join the community and help choose the topic of the next course! http://patreon.com/SpaceWeatherWoman

This Solar Storm Forecast sponsored in part by 3ric Johanson: http://instagram.com/scubist Two familiar bright regions rotate back into Earth-view this week, but they arent quite as active as they were the last time we saw them. No longer classified as sunspots, nevertheless, these regions are still boosting the solar flux, which means radio propagation is back into the marginal range on Earth's dayside for emergency responders and amateur radio operators. We also have a stealthy solar storm that has launched towards Earth. Couple that with the small pockets of fast solar wind in this "coronal hole, bright region oreo cookie sandwich" and we could see unsettled to active conditions on and off throughout this whole week. Learn more about how these bright regions might affect you, catch up on aurora photos from recent solar storms, and see what else our Sun has in store! To get early access to these forecasts plus more see: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images in this video see the links in my previous forecasts. I am saving this space for links to the aurora field reporter photos highlighted this week. Aurora Field Reporter Photography: Matt Deamer, Isle of Skye, Scotland: https://twitter.com/Matt2901/status/1127014550644170752 Live Aurora Newtwork, Iceland: https://twitter.com/LiveAuroraNetw1/status/1133038617058775050 Will Dunn, Collingwood, Ontario, Canada: https://twitter.com/WDPhotography3/status/1127215151197949953 Scott Rock, Southampton, Ontario, Canada: https://twitter.com/scottrockphoto/status/1127146890225692672 Jeff Adams, Red Deer, Alberta, Canada: https://twitter.com/jeffmadams/status/1127181604768501760 John Barnes, Central Alberta, Canada: https://twitter.com/Johnny_B500/status/1129956179927429120 Steph Edgar-Cassin Weyburn, Saskatchewan, Canada: https://twitter.com/stephedgar87/status/1129295763736006656 Tom Warner, Flight over Hudson Bay: https://twitter.com/warnerimages/status/1128737176647237632 Jenny Hagan, near Laporte, Saskatchewan, Canada: https://twitter.com/LostInSk/status/1128199342169382912 Cynthia Salgado, Saskatchewan, Canada: https://twitter.com/peeta333/status/1128387479772516352 Bruce McCurdy, Edmonton, Alberta, Canada: https://twitter.com/BruceMcCurdy/status/1128224734448013312 Deb Maluk, Sandy Lake, Manitoba, Canada: https://twitter.com/dmaluk1/status/1128267517141471232 Brendon, Wyoming-Colorado border, USA: https://twitter.com/brendonme/status/1128307123065118720 Carl Jones, Grand Forks, North Dakota, USA: https://twitter.com/northflwx/status/1128210205861392384 Isaac, Lily Pond, Michigan, USA: https://twitter.com/ID_Photo_Graphy/status/1128284544493289472 Paul Stewart, Timaru, New Zealand: https://twitter.com/astrostew/status/1128250986068230144 Paul, Southland, New Zealand: https://twitter.com/Chasingnatureph/status/1128203789121478656 https://twitter.com/Chasingnatureph/status/1128232624357380096 David Clearwater, Kuana Southland, New Zealand: https://twitter.com/five15design/status/1128265464621092864 Benjamin Alldridge, Tasmania: https://twitter.com/norks/status/1127235886817484800 Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

When the Sun first formed, there were no planets to see it rise until gravity formed four planetary siblings. Narrated by Brian Cox. Subscribe: http://bit.ly/BBCEarthSub Watch more: Planet Earth http://bit.ly/PlanetEarthPlaylist Blue Planet http://bit.ly/BluePlanetPlaylist Planet Earth II http://bit.ly/PlanetEarthIIPlaylist Planet Dinosaur http://bit.ly/PlanetDinoPlaylist The Planets This stunningly ambitious series brings to life the most memorable events in the history of the solar system, by using groundbreaking visual effects to tell the thrilling story of all eight planets. Transporting you to the surface of these dynamic worlds to witness the moments of high drama that shaped each one, The Planets reveals how the latest science allows us to unlock their past lives. It pieces together clues of magnificent lost waterfalls on Mars, the mass planetary migrations as they jostled for position early in their history, and even the distant fate of Saturn as one of its moons awakens to form a beautiful water world. Also available: The Planets: Behind the Science Welcome to BBC EARTH! The world is an amazing place full of stories, beauty and natural wonder. Here you'll find 50 years worth of entertaining and thought-provoking natural history content. Dramatic, rare, and exclusive, nature doesn't get more exciting than this. Want to share your views with the team? Join our BBC Studios Voice: https://www.bbcstudiosvoice.com/register This is a page from BBC Studios who help fund new BBC programmes. Service information and feedback: http://bbcworldwide.com/vod-feedback--contact-details.aspx

This forecast generously sponsored by: 3ric Johanson: http://www.instagram.com/scubist Our Sun dims down a bit this week as the two active regions, 2740 and 2741 rotate out of earth-view. These regions are staying active and have even fired a few solar storms on the Sun's backside. Unfortunately, this means we are back to a spotless Sun, which means poor radio propagation on Earth's dayside. These conditions will likely continue over the next week or more before things improve again. As for aurora possibilities, we do have a few small pockets of fast solar wind that will hit over the next few days that could bring unsettled and up to possibly storm conditions at high latitudes. However, aurora views are expected to be elusive, with only a small chance of views at mid-latitudes. Learn the details of the coming fast solar wind, catch up on aurora pics from last week's G1 and G3 storms, and see what else our Sun has in store! For early access to this forecast and more visit: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images in this video see the links in my previous videos. I need to save room for links to the aurora field reporter photos highlighted this week: Aurora Field Reporter Photography: Lone Athanasakis, Denmark: https://twitter.com/Lathanafoto/status/1127040405936193537 https://twitter.com/Lathanafoto/status/1127589131050262529 Nick, Pulpit Hill, Scotland: https://twitter.com/EdgingtonNick/status/1127161181754540032 James Rowley-Hill, Norfolk, UK: https://twitter.com/chunder10/status/1127205285624459264 Funny Face Audrey, Whitehorse, Yukon, Canada: https://twitter.com/audrey19740719/status/1127156867669680133 Ray Majoran, ParkHill, Ontario, Canada: https://twitter.com/RayMajoran/status/1127341910597808128 Team Tanner, Alix, Alberta, Canada: https://twitter.com/dartanner/status/1127582764436377600 https://twitter.com/dartanner/status/1130182461508349953 Notanee Bourassa, west of Penzance, Saskatchewan, Canada: https://twitter.com/DJHardwired/status/1130245573733474304 Verna Mogk, Eastern Manitoba, Canada: https://twitter.com/VernaMogk/status/1128245234486448128 David McColm, Whistler, Alberta, Canada: https://twitter.com/triwhistler/status/1128252712779313153 Jake Stehli, Central Wisconsin, USA: https://twitter.com/eljakeo30/status/1127053235779526658 Derick Wilson, Nucla, Colorado, USA: https://twitter.com/TheUmno/status/1127680267148308480 Kevin Palmer, Sheridan, Wyoming, USA: https://twitter.com/krp234/status/1128217082301075457 Zachary Hargrove, Bismark, North Dakota, USA: https://twitter.com/Zargrove/status/1127253757715259392 Jeff Bryant, Central Oregon, USA: https://twitter.com/ExquisiteOregon/status/1127263644150951938 Stu Tooley, Lake Wanaka, New Zealand: https://twitter.com/five15design/status/1128265464621092864 Les Ladbrook Invercargill, New Zealand: https://twitter.com/five15design/status/1128265464621092864 Shanan Kapene, Foveaux strait, New Zealand: https://twitter.com/five15design/status/1128265464621092864 Sussan Says, Hobart, Tasmania: https://twitter.com/SussanSays/status/1127202933102133248

This forecast generously sponsored by: 3ric Johanson: http://www.instagram.com/scubist The Sun gets crazy busy this week with multiple solar storms that are inbound to earth! We should feel the first of the direct hits sometime May 15 and storing should continue into May 16 and possibly through the 17th before things begin to calm down. All this rukus is due to regions 2740 and 2741 that have been firing non-sotp solar storms ever since before they even came into Earth view. Lucky for aurora photographers, they have already given us G1 and G3 level storms with aurora dipping down as far south as Wyoming and Colorado in the USA. Learn more about these regions, how they are boosting emergency and amateur radio propagation back into the marginal range, and why they could mess with your GPS reception this week! For early access to these forecasts join my Patreon community: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

Explains the source of the Sun's power, the nuclear reactions that give energy and life to our planet. Images from NASA, Jamen Long, Tino Schulz, EFDA-JET, Kelvin Ma https://commons.wikimedia.org/wiki/File:Wendelstein7-X_Torushall-2011.jpg https://en.wikipedia.org/wiki/File:The_JET_magnetic_fusion_experiment_in_1991.jpg https://commons.wikimedia.org/wiki/File:Sun_poster.svg

Sarbani Basu is a Professor in the Department of Astronomy at Yale University. She is also the current Chair of the Department. Dr. Basu received her training in India, and subsequently worked in the U.K. and Denmark before moving to the US to join the Institute for Advance Study, Princeton, NJ. She has been on the faculty of Yale since 2000. Dr. Basu specializes in the study of the Sun and other stars using data on stellar oscillations (star quakes). Her past research was devoted to studying the details of the structure and dynamics of the Sun, which allowed her claim, long before the particle physics community, that the solar neutrino problem was a problem with the standard model of particle physics, not that of astrophysics. Her current research focuses on two separate topics: The first is the study of variations in the Sun over time-scales that are of societal relevance. To this end she uses solar oscillation data to examine changes that take place inside the Sun over periods of years and decades. Her second focus is to study stars, in particular exo-planet hosts, to determine their structure, age and formation histories in order to understand those systems as well as to shed light on the past and future of the Sun and the solar system. This talk was presented at the Westport Astronomical Society on April 16, 2019.

Bonus Footage: I highlight the recently confirmed Mars quake detected by the seismometer (SEIS) on the Insight Lander. This bonus segment originally aired on TMRO Space News, April 24, 2019. Space Weather picks up slightly this week as a remnant coronal hole region rotates through the Earth-strike zone. Because this region is weakening under the influence of a solar minimum Sun, expect only unsettled conditions, with aurora shows limited mostly to high latitudes. Amateur radio operators should also expect poor radio propagation this week, due to our spotless Sun, but GPS users should enjoy decent signal reception, even at low latitudes. Learn the details of the coming fast solar wind, find out when we can expect solar flux to rise again, and see what else our Sun has in store this week. Get early access to these forecasts at: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.

Space Weather quiets down this week though we continue to get hit with sporadic pockets of fast solar wind. Activity could increase at high latitudes, with a brief chance for aurora, but expect only unsettled conditions to persist through the remainder of this week. Aurora photographers may have difficulty catching glimpses of the aurora, but luckily that isn't the only thing in the night sky worth watching. This week, Earth enters the Lyrids meteor shower, which could give us a decent show through April 25. Skywatchers will need to get out of city lights and mind the bright, full moon on the 20th and 21st to maximize chances of seeing the spectacle. Meanwhile, back on the Sun, bright region 2738 is rotating out of view so solar flux should drop back into the low 70s by early next week. This means amateur, shortwave radio, and emergency responders will notice the drop off in communications as we fall back to poor radio propagation on Earth's dayside. However, propagation on 6m due to the Lyrids might actually pick up this week! As for GPS, users should be enjoying decent reception all around the globe easily over the next few days. Learn the details of the Lyrid shower, when solar flux will drop, and what else our Sun has in store this week. For early access to these forecasts & much more see: http://patreon.com/SpaceWeatherWoman For daily and often hourly updates (during active times) visit me on Twitter: https://twitter.com/TamithaSkov For a more in-depth look at the data and images highlighted in this video see these links below. Solar Imaging and Analysis: SDO: http://sdo.gsfc.nasa.gov/data/ Helioviewer: http://www.helioviewer.org/ Flare Analysis: http://www.lmsal.com/solarsoft/latest_events/ Computer Aided CME Tracking CACTUS: http://www.sidc.oma.be/cactus/out/latestCMEs.html GOES Xray: http://www.swpc.noaa.gov/rt_plots/xray_1m.html SOHO: http://sohodata.nascom.nasa.gov/ Stereo: http://stereo.gsfc.nasa.gov/ GONG magnetic field synoptic movie: https://gong.nso.edu/data/magmap/standard_movie.html GONG magnetic field synoptic charts: http://gong.nso.edu/data/magmap/ LMSAL Heliophysics Events HEK http://www.lmsal.com/isolsearch Solar Wind: DISCOVR solar wind: http://www.swpc.noaa.gov/products/real-time-solar-wind ACE Solar Wind: http://www.swpc.noaa.gov/products/ace-real-time-solar-wind NASA ENLIL SPIRAL: https://iswa.gsfc.nasa.gov/IswaSystemWebApp/iSWACygnetStreamer?timestamp=2038-01-23+00%3A44%3A00&window=-1&cygnetId=261 NOAA ENLIL SPIRAL: http://www.swpc.noaa.gov/products/wsa-enlil-solar-wind-prediction Magnetosphere, Ionosphere, Atmosphere: GOES Magnetometer: http://www.swpc.noaa.gov/products/goes-magnetometer Ionosphere D-Region Absorption (DRAP) model: http://www.swpc.noaa.gov/products/d-region-absorption-predictions-d-rap/ Auroral Oval Ovation Products: http://www.swpc.noaa.gov/products/aurora-30-minute-forecast Global 3-hr Kp index: http://www.swpc.noaa.gov/products/planetary-k-index Wing Kp index prediction: http://www.swpc.noaa.gov/products/wing-kp USGS Ground Magnetometers: http://geomag.usgs.gov/realtime/ USGS Disturbance Storm-Time (Dst): http://geomag.usgs.gov/realtime/dst/ NAIRAS Radiation Storm Model: http://sol.spacenvironment.net/raps_ops/current_files/globeView.html Multi-Purpose Space Environment Sites: NOAA/SWPC: http://www.swpc.noaa.gov SOLARHAM: http://www.solarham.net/index.htm Spaceweather: http://spaceweather.com iSWA: http://iswa.gsfc.nasa.gov/iswa/iSWA.html Definition of Geomagnetic Storm, Radiation Storm, and Radio Blackout Levels: http://www.swpc.noaa.gov/NOAAscales/ None of this would be possible without the hard work and dedication of those who have provided all of this data for public use. Images c/o NASA/ESA/CSA (most notably the superb SDO, SOHO, ACE, STEREO, CCMC, JPL & DSN teams, amazing professionals, hobbyists, institutions, organizations, agencies and amateurs such as those at the USAF/HAARP, NICT, NOAA, USGS, Environment Canada, Natural Resources Canada, Intellicast, Catatania, rice.edu, wisc.edu, sonoma.edu ucalgary.ca, rssi.ru, ohio-state.edu, solen.info, and more. Thanks for making Space Weather part of our every day dialogue.