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

Astronomy and Astrophysics – Astronomy

Scientific paper

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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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