A Study of the Background in the HETE Equatorial Orbit

Details A Study of the Background in the HETE Equatorial Orbit A Study of the Background in the HETE Equatorial Orbit

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..662...63b&link_type=abstract

GAMMA-RAY BURST AND AFTERGLOW ASTRONOMY 2001: A Workshop Celebrating the First Year of the HETE Mission. AIP Conference Proceed

Astronomy and Astrophysics

Astronomy

1

Background Radiations, Gamma-Ray Sources, Gamma-Ray Bursts, Spaceborne And Space Research Instruments, Apparatus, And Components, X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

After a year of operation, we have become well acquainted with HETE's in-orbit background. In particular, as it is near solar maximum, we have observed through intense periods of geomagnetic disturbance. We describe the resulting deviations from our mean backgrounds. Aside from these periods, the background has been quite stable over this first year. We compare the averaged background in the WXM and Fregate instruments for the months of March and September, 2001.

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