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Reconstruction of the energy spectrum of electrons accelerated in the April 15, 2002 solar flare based on IRIS X-ray spectrometer measurements


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We reconstruct the energy distribution of electrons accelerated in the April 15, 2002 solar flare on the basis of the data from the IRIS X-ray spectrometer onboard the CORONAS-F satellite. We obtain the solution to the integral equations describing the transformation of the spectrum of X-ray photons during the recording and reconstruction of the spectrum of accelerated electrons in the bremsstrahlung source using the random search method and the Tikhonov regularization method. In this event, we detected a singularity in the electron spectrum associated with the existence of a local minimum in the energy range 40–60 keV, which cannot be detected by a direct method.

Sobre autores

G. Motorina

Central (Pulkovo) Astronomical Observatory

Email: Igor.Koudriavtsev@mail.ioffe.ru
Rússia, Pulkovskoe sh. 65, St. Petersburg, 196140

I. Kudryavtsev

Central (Pulkovo) Astronomical Observatory; Ioffe Institute

Autor responsável pela correspondência
Email: Igor.Koudriavtsev@mail.ioffe.ru
Rússia, Pulkovskoe sh. 65, St. Petersburg, 196140; Politekhnicheskaya ul. 26, St. Petersburg, 194021

V. Lazutkov

Ioffe Institute

Email: Igor.Koudriavtsev@mail.ioffe.ru
Rússia, Politekhnicheskaya ul. 26, St. Petersburg, 194021

M. Savchenko

Ioffe Institute

Email: Igor.Koudriavtsev@mail.ioffe.ru
Rússia, Politekhnicheskaya ul. 26, St. Petersburg, 194021

D. Skorodumov

Ioffe Institute

Email: Igor.Koudriavtsev@mail.ioffe.ru
Rússia, Politekhnicheskaya ul. 26, St. Petersburg, 194021

Yu. Charikov

Ioffe Institute; St. Petersburg State Technical University

Email: Igor.Koudriavtsev@mail.ioffe.ru
Rússia, Politekhnicheskaya ul. 26, St. Petersburg, 194021; Politekhnicheskaya ul. 29, St. Petersburg, 195251

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Declaração de direitos autorais © Pleiades Publishing, Ltd., 2016