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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2008, Volume 88, Issue 7, Pages 483–485
(Mi jetpl236)
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This article is cited in 8 scientific papers (total in 8 papers)
GRAVITY, ASTROPHYSICS
New method for estimating the absolute flux and energy spectrum of solar cosmic rays based on neutron-monitor data
G. F. Krymsky, V. G. Grigor'ev, S. A. Starodubtsev Shafer Institute of Cosmophysical Research and Aeronomy, Yakut Research Center, Siberian Branch, Russian Academy of Sciences, pr. Lenina 31, Yakutsk, 677980, Russia
Abstract:
A new method is described for estimating the absolute flux of solar cosmic rays based on the data from a single neutron monitor. The method is capable of yielding the energy spectrum at the isotropic phase of a solar flare using the available data from the currently operable worldwide network of cosmic-ray stations. The method is based on the determination of the effective momentum or energy for which the particle flux derived from the neutron-monitor count rate is weakly sensitive to small variations in the exponent of the power-law spectrum. A comparison of the calculations with direct space-borne measurements and calculations by other authors based on the data from the neutron-monitor network shows their satisfactory agreement for the last ground-level enhancement of solar cosmic rays observed on December 13, 2006.
Received: 29.07.2008
Citation:
G. F. Krymsky, V. G. Grigor'ev, S. A. Starodubtsev, “New method for estimating the absolute flux and energy spectrum of solar cosmic rays based on neutron-monitor data”, Pis'ma v Zh. Èksper. Teoret. Fiz., 88:7 (2008), 483–485; JETP Letters, 88:7 (2008), 411–413
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https://www.mathnet.ru/eng/jetpl236 https://www.mathnet.ru/eng/jetpl/v88/i7/p483
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Abstract page: | 229 | Full-text PDF : | 85 | References: | 35 |
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