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RHESSI Observes 2.2 MeV Line Emission from a Solar Flare

The solar flare at Active Region 10039 on July 23, 2002 exhibits many exceptional high-energy phenomena including the 2.223 MeV neutron capture line and the 511 keV electron-positron (antimatter) annihilation line. In the animation, the RHESSI low-energy channels (12-25 keV) are represented in red and appears predominantly in coronal loops. The high-energy flux appears as blue at the footpoints of the coronal loops. Violet is used to indicate the location and relative intensity of the 2.2MeV emission.

This movie zooms in to AR 10039 to reveal gamma-ray emission regions near the loop structures.    This movie zooms in to AR 10039 to reveal gamma-ray emission regions near the loop structures.
Duration: 29.0 seconds
Available formats:
  640x480 (30 fps) MPEG-1   14 MB
  320x240 (30 fps) MPEG-1   4 MB
  320x240     JPEG         5 KB
  320x240     JPEG         5 KB
  720x480 (29.97 fps) DV           126 MB
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Full-disk view of the Sun, July 22, 2002, from SOHO-MDI.    Full-disk view of the Sun, July 22, 2002, from SOHO-MDI.

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Close-up view of AR 10039 from SOHO-MDI    Close-up view of AR 10039 from SOHO-MDI

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View of AR 10039 in the Hydrogen-Alpha line.    View of AR 10039 in the Hydrogen-Alpha line.

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RHESSI sees low energy emission near the loops.    RHESSI sees low energy emission near the loops.

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High energy emission appears at the loop footpoints.    High energy emission appears at the loop footpoints.

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More high-energy emission at the base of the loops.    More high-energy emission at the base of the loops.

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The 2.2MeV gamma-ray emission is prominent.    The 2.2MeV gamma-ray emission is prominent.

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Emission persists.    Emission persists.

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The 2.2MeV emission fades and the other footpoint appears.    The 2.2MeV emission fades and the other footpoint appears.

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High energy emission drops with some low energy still visible.    High energy emission drops with some low energy still visible.

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Still low-energy emission.  Loops more visible in Hydrogen-Alpha.    Still low-energy emission. Loops more visible in Hydrogen-Alpha.

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The coronal loops glow brightly in TRACE 195 Angstrom band.    The coronal loops glow brightly in TRACE 195 Angstrom band.

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The loops continue to fade in TRACE.    The loops continue to fade in TRACE.

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None    None

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Animation Number:2750
Animators:Tom Bridgman (Lead)
 Marte Newcombe
Studio:SVS
Completed:2003-06-11
Scientists:Robert Lin (University of California, Berkeley)
 Sam Krucker (University of California, Berkeley)
 Gordon J. Hurford (University of California, Berkeley)
 R. J. Murphy (NRL)
 G. H. Share (NRL)
 X.-M. Hua (L-3 Communications Analytics Corporation)
 David M. Smith (University of California, Berkeley)
 Richard A. Schwartz (NASA/GSFC)
 Benzion Kozlovsky (Tel Aviv University)
Writer:William Steigerwald (NASA/GSFC)
Instruments:SOHO/MDI
 RHESSI/X-ray Imaging Spectrometer
 TRACE
Data set:BBSO
Data Collected:BBSO: 2002/07/22T16:22:36-2002/07/23T01:21:45, SOHO/MDI:2002/07/21T23:59:30-2002/07/23T17:35:30, TRACE: 2002/07/23T00:00:59-2002/07/23T03:32:45, RHESSI: 2002/07/23T00:16:00-2002/07/23T01:14:53
Series:Active Region 10039
Video:SVS2003-0004 *
Goddard TV Tapes:G2003-040
 G2003-050
Keywords:
SVS >> Active Region 10039
SVS >> Antimatter
SVS >> Coronal Loop
SVS >> Electron
SVS >> Gamma Ray
SVS >> Positron
DLESE >> Space science
SVS >> Sun
SVS >> X-ray
GCMD >> EARTH SCIENCE >> Sun-earth Interactions >> Solar Activity >> Solar Flares
SVS >> Neutron
 
 
Please give credit for this item to
NASA/Goddard Space Flight Center Scientific Visualization Studio


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