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.
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Original Russian Text © Yu.D. Kotov, A.S. Glyanenko, A.I. Arkhangel’skii, M.V. Bessonov, A.S. Buslov, V.N. Yurov, V.A. Dergachev, G.A. Matveev, E.M. Kruglov, V.P. Lazutkov, M.I. Savchenko, D.V. Skorodumov, A.G. Pyatigorsky, G.A. Pyatigorsky, I.I. Shishov, E.M. Khilkevich, G.I. Vasilyev, S.Yu. Krutkov, 2011, published in Astronomicheskii Vestnik, 2011, Vol. 45, No. 2, pp. 139–149.
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Kotov, Y.D., Glyanenko, A.S., Arkhangelsky, A.I. et al. Experimental study of parameters of X-ray radiation from solar flares using the PENGUIN-M instrument aboard the CORONAS-PHOTON spacecraft. Sol Syst Res 45, 135–145 (2011). https://doi.org/10.1134/S0038094611020092
- Count Rate
- Solar Flare
- Linear Polarization
- Scattered Radiation