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"title": "Incredible Solar Flare, Prominence Eruption and CME Event (SDO/HMI visible light)",
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"description": "On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME).
In this view in visible light seen by the SDO/HMI instrument, we can't even see the event. This view is provided as a comparison to how dramatic the event appears in extreme ultraviolet light, as seen in 3838 (304 Ångstroms), 3839 (171 Ångstroms), and 3840 (211 Ångstroms), near ultraviolet light, 3841 (1700 Ångstroms), presented a much less impressive event.",
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"funding_sources": [
"NASA Heliophysics"
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"credits": [
{
"role": "Animator",
"people": [
{
"name": "Tom Bridgman",
"employer": "Global Science and Technology, Inc."
}
]
},
{
"role": "Producer",
"people": [
{
"name": "Horace Mitchell",
"employer": "NASA/GSFC"
}
]
},
{
"role": "Scientist",
"people": [
{
"name": "William D. Pesnell",
"employer": "NASA/GSFC"
}
]
}
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"series": [
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],
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"datasets": [
{
"name": "Continuum",
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"platform": "SDO",
"sensor": "HMI",
"type": "Other",
"organizations": [],
"description": "",
"credit": "",
"url": "",
"date_range": "2011/06/07T06:00:00 - 2011/06/07T12:00:00"
}
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"keywords": [
"Coronal Mass Ejections",
"Earth Science",
"Hyperwall",
"Presentation",
"SDO",
"Solar Active Regions",
"Solar Activity",
"Solar Dynamics Observatory",
"Solar Events",
"Solar Filaments",
"Solar Flares",
"Solar Prominences",
"Sun-earth Interactions",
"Visible Light Imaging"
],
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"related": [
{
"id": 4659,
"url": "https://svs.gsfc.nasa.gov/4659/",
"page_type": "Visualization",
"title": "Incredible Solar Flare, Prominence Eruption and CME Event (hydrogen alpha filter)",
"description": "This movie is generated from imagery collected by the NSO GONG network of solar observatories. It is not time-synchronized to the related observations by the Solar Dynamics Observatory (SDO). || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_print.jpg (1024x576) [25.1 KB] || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_searchweb.png (320x180) [20.9 KB] || BBSO_Halpha_2011JuneUh_stand.HD1080i.00187_thm.png (80x40) [2.3 KB] || 1920x1080_16x9_30p (1920x1080) [32.0 KB] || BBSO_Halpha_2011JuneUh_HD1080i_p30.mp4 (1920x1080) [2.8 MB] || BBSO_Halpha_2011JuneUh_HD1080i_p30.webm (1920x1080) [1.2 MB] || 3840x2160_16x9_30p (3840x2160) [32.0 KB] || BBSO_Halpha_2011JuneUh_2160p30.mp4 (3840x2160) [11.4 MB] || ",
"release_date": "2018-06-27T00:00:00-04:00",
"update_date": "2024-04-28T00:10:22.837854-04:00",
"main_image": {
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"filename": "BBSO_Halpha_2011JuneUh.00187_print.jpg",
"media_type": "Image",
"alt_text": "This movie is generated by the raw 2Kx2K imagery. Frames are available as sequentially numbered or time-stamp in file name.",
"width": 1024,
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"pixels": 1048576
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{
"id": 3838,
"url": "https://svs.gsfc.nasa.gov/3838/",
"page_type": "Visualization",
"title": "Incredible Solar Flare, Prominence Eruption and CME Event (304 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), 3840 (211 Ångstroms) and 3841 (1700 Ångstroms). || ",
"release_date": "2011-07-01T10:00:00-04:00",
"update_date": "2024-04-28T00:01:02.896048-04:00",
"main_image": {
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"url": "https://svs.gsfc.nasa.gov/vis/a000000/a003800/a003838/SDO304FullDisk_1080HD_web.png",
"filename": "SDO304FullDisk_1080HD_web.png",
"media_type": "Image",
"alt_text": "These movies present the six hour interval around the event, a one minute per animation frame.",
"width": 320,
"height": 180,
"pixels": 57600
}
},
{
"id": 3839,
"url": "https://svs.gsfc.nasa.gov/3839/",
"page_type": "Visualization",
"title": "Incredible Solar Flare, Prominence Eruption and CME Event (171 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 3838 (304 Ångstroms), 3840 (211 Ångstroms) and 3841 (1700 Ångstroms). || ",
"release_date": "2011-07-01T10:00:00-04:00",
"update_date": "2024-04-28T00:01:05.864739-04:00",
"main_image": {
"id": 484965,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a003800/a003839/SDO171Full_stand.HD1080i.00100.jpg",
"filename": "SDO171Full_stand.HD1080i.00100.jpg",
"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,
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{
"id": 3840,
"url": "https://svs.gsfc.nasa.gov/3840/",
"page_type": "Visualization",
"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). || ",
"release_date": "2011-07-01T10:00:00-04:00",
"update_date": "2024-04-28T22:03:39.656687-04:00",
"main_image": {
"id": 484994,
"url": "https://svs.gsfc.nasa.gov/vis/a000000/a003800/a003840/SDO211Full_stand.HD1080i.00100.jpg",
"filename": "SDO211Full_stand.HD1080i.00100.jpg",
"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
}
},
{
"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). || ",
"release_date": "2011-07-01T10:00:00-04:00",
"update_date": "2024-04-28T22:03:42.271367-04:00",
"main_image": {
"id": 485027,
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"filename": "SDO1700Full_stand.HD1080i.00100.jpg",
"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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