A Preliminary comparison of the Flares as seen by SDO-EVE-ESP and GOES XRS

Details A Preliminary comparison of the Flares as seen by SDO-EVE-ESP and GOES XRS A Preliminary comparison of the Flares as seen by SDO-EVE-ESP and GOES XRS

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh23a1833g&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH23A-1833

Astronomy and Astrophysics

Astrophysics

[7519] Solar Physics, Astrophysics, And Astronomy / Flares

Scientific paper

We present the results of a study comparing the thermal phase of solar flares observed in the soft X-Ray wavelengths seen by two independent instruments, the GOES-XRS and the SDO-EVE-ESP instrument. Comparison parameters studied include the soft X-ray magnitude as well as the timing of this peak emission, the rise time from initiation to peak and flare duration. While the GOES XRS instrument has 30+ years of heritage studying many of these solar flare characteristics, the new ESP instrument, a quadrant detector, has the added ability of being able to locate flares on the solar disk. This flare location technique and its precision from the ESP measurement will also be discussed.

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