RHESSI Observations of Continuous Solar X-Ray Emission from 3 to 10 keV

Details RHESSI Observations of Continuous Solar X-Ray Emission from 3 to 10 keV RHESSI Observations of Continuous Solar X-Ray Emission from 3 to 10 keV

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.7604h&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #76.04; Bulletin of the American Astronomical Society, Vol. 34, p.776

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The RHESSI spacecraft, launched 5 February 2002, provides imaging spectroscopy of solar x-ray emission from 3 keV to 15 MeV. In addition to its high spatial and spectral resolution (2.3 arcsec and ~ 1 keV respectively), RHESSI also has exceptional sensitivity at low energies. This sensitivity has enabled it to observe continuous x-ray emission from the non-flaring Sun at energies from 3 to ~ 10 keV. This paper presents preliminary observations of the spatial and spectral characteristics of this emission.

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