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"url": "http://jsoc.stanford.edu/",
"date_range": "2012-08-30T11:00 to 2012-09-05T23:59"
},
{
"name": "171 Filter",
"common_name": "AIA 171",
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"sensor": "AIA",
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],
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],
"keywords": [
"Corona",
"Coronal Mass Ejections",
"Earth Science",
"Heliophysics",
"Hyperwall",
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"Solar Activity",
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"recommended_pages": [],
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{
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"url": "https://svs.gsfc.nasa.gov/13859/",
"page_type": "Produced Video",
"title": "Why Does NASA Observe The Sun in Different Colors?",
"description": "The Solar Dynamics Observatory, or SDO, was launched on Feb. 11, 2010, and began collecting science data a few months later. With two imaging instruments – the Atmospheric Imaging Assembly and the Helioseismic and Magnetic Imager, which were designed in concert to provide complementary views of the Sun – SDO sees the Sun in more than 10 distinct wavelengths of light, showing solar material at different temperatures. SDO also measures the Sun’s magnetic field and the motion of solar material at its surface, and, using a technique called helioseismology, allows scientists to probe deep into the Sun's interior, where the Sun’s complex magnetic fields sprout from. And with more than a decade of observation under its belt, SDO has provided scientists with hundreds of millions of images of our star. || ",
"release_date": "2021-06-18T12:00:00-04:00",
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"alt_text": "Music credits: “Swirling Blizzard” and “Endless Swirl” by Laurent Dury [SACEM] from Universal Production Music Watch this video on the NASA Goddard YouTube channel.Complete transcript available.",
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{
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"title": "Animation of USPS Stamps Featuring NASA's Solar Dynamic Observatory",
"description": "The U.S. Postal Service illuminates the light and warmth of our nearest star by highlighting these stunning images of the Sun on stamps. These images come from NASA’s Solar Dynamics Observatory, a spacecraft launched in February 2010 to keep a constant watch on the Sun.The Sun is the only star that humans are able to observe in great detail, making it a vital source of information about the universe. The Solar Dynamics Observatory lets us see the Sun in wavelengths of ultraviolet light that would otherwise be invisible to our eyes. Each black-and-white image is colorized to the bright hues seen here.The stamps highlight different features on the Sun that help scientists learn about how our star works and how its constantly churning magnetic fields create the solar activity we see. Sunspots, coronal holes and coronal loops, for example, can reveal how those magnetic fields dance through the Sun and its atmosphere. Observing plasma blasts and solar flares can help us better understand and mitigate the impact of such eruptions on technology in space.The Sun Science stamps are being issued as Forever stamps, which will always be equal in value to the current First-Class Mail 1-ounce price. || ",
"release_date": "2021-06-17T16:00:00-04:00",
"update_date": "2023-05-03T13:44:05.905629-04:00",
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{
"id": 11095,
"url": "https://svs.gsfc.nasa.gov/11095/",
"page_type": "Produced Video",
"title": "August 31, 2012 Magnificent CME",
"description": "On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly toward Earth, but did connect with Earth's magnetic environment, or magnetosphere, with a glancing blow. causing aurora to appear on the night of Monday, September 3. || ",
"release_date": "2012-09-04T14:00:00-04:00",
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