RHESSI/GOES Observations of the Nonflaring Sun from 2002 to 2006

Details RHESSI/GOES Observations of the Nonflaring Sun from 2002 to 2006 RHESSI/GOES Observations of the Nonflaring Sun from 2002 to 2006

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009apj...697...94m&link_type=abstract

The Astrophysical Journal, Volume 697, Issue 1, pp. 94-99 (2009).

Astronomy and Astrophysics

Astronomy

14

Sun: Corona, Sun: X-Rays, Gamma Rays

Scientific paper

In this work, we obtain the temperature (T) and emission measure (EM) for solar X-ray emission, using RHESSI and GOES data, at times for which there are no solar flares. Approximately 8700 time intervals during the RHESSI mission, from launch until 2006 August, are analyzed. We find that high-temperature emission, in the temperature range of 5-10 MK, is typically present during active times. When comparing temperature measurements, we find that RHESSI temperature measurements are consistently higher than GOES measurements, with smaller EM for RHESSI, but with values for the two instruments that are not necessarily well correlated.

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