Email this article Relationship between the Longitude Distribution of the Heliospheric Characteristics and the GCR Intensity in 2007–2008 and 2014–2015
- Authors: Krainev M.B.1, Bazilevskaya G.A.1, Borkut I.K.2, Mayorov A.G.2
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Affiliations:
- Lebedev Physical Institute
- National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
- Issue: Vol 81, No 9 (2018)
- Pages: 1355-1361
- Section: Interaction of Plasma, Particle Beams, and Radiation with Matter
- URL: https://journals.rcsi.science/1063-7788/article/view/193875
- DOI: https://doi.org/10.1134/S1063778818090156
- ID: 193875
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Abstract
On the basis of the temporal behavior of the galactic cosmic rays and the heliospheric factors observed in 2007–2008 and 2014–2015, their average heliolongitude distributions are formed and compared. In addition to the neutron monitor data, the provisional database of daily average galactic cosmic ray proton intensities measured by the PAMELA satellite-borne experiment in 2006–2015 is used. It is shown that the properties of the heliolongitude distributions in the above periods are substantially different.
About the authors
M. B. Krainev
Lebedev Physical Institute
Author for correspondence.
Email: mkrainev46@mail.ru
Russian Federation, Moscow, 119991
G. A. Bazilevskaya
Lebedev Physical Institute
Email: mkrainev46@mail.ru
Russian Federation, Moscow, 119991
I. K. Borkut
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: mkrainev46@mail.ru
Russian Federation, Moscow, 115409
A. G. Mayorov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: mkrainev46@mail.ru
Russian Federation, Moscow, 115409
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