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"title": "Incredible Solar Flare, Prominence Eruption and CME Event (SDO/HMI visible light)",
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"title": "Incredible Solar Flare, Prominence Eruption and CME Event (171 angstroms)",
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{
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"title": "Incredible Solar Flare, Prominence Eruption and CME Event (211 angstroms)",
"description": "On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk.Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events.This image sequence is captured at one minute intervals and designed to play synchronously with animations 3839 (171 Ångstroms), 3838 (304 Ångstroms) and 3841 (1700 Ångstroms). || ",
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"media_type": "Image",
"alt_text": "These movies present the six hour interval around the event, a one minute per animation frame.",
"width": 1920,
"height": 1080,
"pixels": 2073600
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{
"id": 3841,
"url": "https://svs.gsfc.nasa.gov/3841/",
"page_type": "Visualization",
"title": "Incredible Solar Flare, Prominence Eruption and CME Event (1700 angstroms)",
"description": "On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). At this wavelength, very little of the ejected material is visible. However, it is possible to see locations where some of the material is falling back and striking the solar surface.This image sequence is captured at one minute intervals and designed to play synchronously with animations 3839 (171 Ångstroms), 3840 (211 Ångstroms) and 3838 (304 Ångstroms). || ",
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