Small-Scale Structure of Thermal X-Ray Background of the Solar Corona and Microflares in the Photon Energy Range of 3-16 keV
- Авторлар: Mirzoeva I.K.1
-
Мекемелер:
- Space Research Institute
- Шығарылым: Том 44, № 1 (2018)
- Беттер: 92-101
- Бөлім: Space Plasma
- URL: https://journals.rcsi.science/1063-780X/article/view/186643
- DOI: https://doi.org/10.1134/S1063780X18010117
- ID: 186643
Дәйексөз келтіру
Аннотация
The small-scale structure of the thermal X-ray background of the solar corona and microflares in the photon energy range from 3 to 16 keV according to the RHESSI data obtained on March–April 2003 is analyzed. The study of the reduction in the X-ray intensity in this spectral range is continued. A reduction and, in some cases, an increase in the X-ray intensity of the thermal background of the solar corona and microflares in narrow subranges of the X-ray spectrum of the quiet Sun are revealed in the photon energy range of 3–11 keV.
Авторлар туралы
I. Mirzoeva
Space Research Institute
Хат алмасуға жауапты Автор.
Email: colombo2006@mail.ru
Ресей, Moscow, 117997
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