MOSES Radiometric Calibration

Details MOSES Radiometric Calibration MOSES Radiometric Calibration

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.1808r&link_type=abstract

American Astronomical Society, SPD meeting #40, #18.08; Bulletin of the American Astronomical Society, Vol. 41, p.845

Physics

Scientific paper

We present analysis of radiometric calibration data for MOSES, the Multi-Order Solar EUV Spectrograph. MOSES is an EUV imaging spectrograph which uses a spherical grating to feed three rear illuminated CCDs, one for each of the m = 0 and m = ±1 spectral orders of the grating. MOSES was calibrated end-to-end at the EUV radiometric calibration facility at Rutherford Appleton Laboratory, using a well characterized hollow cathode source traceable to the BESSY synchrotron. We analyze these data and present the end-to-end instrument response (DN per incident photon) for each of MOSES three CCD channels. This work was supported in part by a grant from the NASA Solar and Heliospheric Physics LCAS program.

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