Incredible Solar Flare, Prominence Eruption and CME Event (SDO/HMI visible light)

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). This movie is generated by the raw 2Kx2K imagery. Frames are available as sequentially numbered or time-stamp in file name. On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). This view filtered for the hydrogen-alpha spectral line is collected from ground-based observatories operated by the National Solar Observatory (NSO). 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. Related pages

These movies present the six hour interval around the event, a one minute per animation frame. These are 4Kx4K frames with coded colors. Hyperwall files 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). Related pages

These movies present the six hour interval around the event, a one minute per animation frame. These are 4Kx4K frames with coded colors. Hyperwall files 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). Related pages

These movies present the six hour interval around the event, a one minute per animation frame. These are 4Kx4K frames with coded colors. Hyperwall files 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). Related pages

These movies present the six hour interval around the event, a one minute per animation frame. These are 4Kx4K frames with coded colors. Hyperwall files 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). Related pages