Observations of the Sun–Earth system within the CORONAS-F mission (July 31, 2001 to December 6, 2005)

Кузнецов, В. Д.

doi:10.1016/j.jastp.2007.08.013

Cited by 5 publications

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References 11 publications

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“…[42] This paper presents only some of the most important results of the CORONAS-F project. One can find their more detailed description in the reviews [Kuznetsov, 2004[Kuznetsov, , 2005[Kuznetsov, , 2006a[Kuznetsov, , 2006b[Kuznetsov, , 2007Kuznetsov et al, 2004Kuznetsov et al, , 2005Oraevsky and Sobelman, 2002;Oraevsky et al, 2002Oraevsky et al, , 2003] and in the references therein.…”

Section: Discussionmentioning

confidence: 99%

From the geophysical to heliophysical year: The results of the CORONAS-F project

Кузнецов¹

2007

Russ. J. Earth Sci.

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The main and most significant results of the CORONAS-F space project are presented. In the scope of this project observations of solar activity and its impact on the Earth were carried out from July 2001 to December 2005. The remote observation devices studied the localization and morphology of solar activity in the second half of the 23rd solar cycle. High-temperature plasma formations are found and studied in the solar corona, eruptive phenomena, processes of particle acceleration, and atomic and nuclear processes in solar flares are investigated. The devices of the "Solar Cosmic Ray" complex studied manifestations of solar activity in the near-Earth environment, dynamics of the radiation belts of the Earth, and rebuilding of the magnetosphere structure in the periods of magnetic storms caused by active events on the Sun. Results related to the upper atmosphere of the Earth and helioseismology are also presented.

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