Physics
Scientific paper
Apr 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sosyr..45..135k&link_type=abstract
Solar System Research, Volume 45, Issue 2, pp.135-145
Physics
Scientific paper
The main characteristics of the PENGUIN-M instrument are given. The instrument has been operating aboard the CORONAS-PHOTON spacecraft (SC) launched into orbit on January 30, 2009. The instrument includes the PENGUIN-MD detector unit (PMD) and the PENGUIN-ME electronic unit (PMD). The purpose of the experiment is to measure the degree of linear polarization of X-ray radiation from solar flares in the energy range of 20-150 keV and to obtain energy spectra of X-ray radiation from solar flares in the energy range of 2-500 keV. The paper describes the instrument, calibration procedure, and in-flight adjustment, and contains the first results of measurements.
Arkhangelsky Andrey I.
Bessonov M. V.
Buslov A. S.
Dergachev Valentin A.
Glyanenko Alexander S.
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