The Hard X-Ray Burst Spectrometer Page

The HXRBS was designed to examine the role of energetic electrons in solar flares by measuring the variations in intensity and energy of the hard X-ray fluxes. Scintillation events in its actively collimated CsI(Na) detector were read out every 128 ms in fifteen energy channels between ~25 to ~500 keV. A circulating memory was able to accumulate relatively brief periods of data during the more intense flares with time resolution down to 1 ms. The full width at half maximum of the field of view was approximately 40 degrees.

HXRBS Event Listings, by year

FTP access to FITS files containing the HXRBS data is available.

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Web Curator: Amy Skowronek
amy@aloha.nascom.nasa.gov
+1 301 286-4713

Responsible NASA official: Joseph B. Gurman, Facility Scientist, Solar Data Analysis Center
gurman@umbra.nascom.nasa.gov
+1 301 286-4767

NASA Goddard Space Flight Center
Solar Physics Branch / Code 682
Greenbelt, MD 20771

Last Modified: 1997 March 31