Imaging Hard X-ray Flares with HESSI

Details Imaging Hard X-ray Flares with HESSI Imaging Hard X-ray Flares with HESSI

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sp51a10s&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SP51A-10

Physics

7519 Flares, 7554 X Rays, Gamma Rays, And Neutrinos, 7594 Instruments And Techniques

Scientific paper

The High Energy Solar Spectroscopic Imager (HESSI) is expected to be launched in early to mid 2001. Its high purity Ge detectors will obtain time-tagged event lists of numerous x-ray and gamma-ray flares. The phase-calibrated profiles constructed from these data can be used to reconstruct images by several techniques. Examples of broad-band (20-30 keV) images of flares in the 10-100 keV range using 5 or 6 methods with a variety of angular and temporal resolutions will be presented. The reliability of the imaging techniques will be assessed through the use of internal consistency checks and comparisons with context data.

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