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A Method for Real-time Gle Modeling : Volume 7, Issue 4 (26/10/2011)

By Vashenyuk, E. V.

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Book Id: WPLBN0004002811
Format Type: PDF Article :
File Size: Pages 6
Reproduction Date: 2015

Title: A Method for Real-time Gle Modeling : Volume 7, Issue 4 (26/10/2011)  
Author: Vashenyuk, E. V.
Volume: Vol. 7, Issue 4
Language: English
Subject: Science, Astrophysics, Space
Collections: Periodicals: Journal and Magazine Collection (Contemporary), Copernicus GmbH
Publication Date:
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications


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Vashenyuk, E. V. (2011). A Method for Real-time Gle Modeling : Volume 7, Issue 4 (26/10/2011). Retrieved from

Description: Polar Geophysical Institute, KSC Russian Academy of Sciences, Apatity, Russia. By now real time systems of data collection of neutron monitor network have been created. The main goal of such systems is early detection of dangerous events of space weather, such as GLE, caused by arrival to the Earth of relativistic solar protons. Characteristics of these particles are determined from the data of the worldwide neutron monitor network by methods of GLE modeling. Traditional GLE modeling requires data of no less than 30–35 stations and takes a long time of computations. We developed a truncated technique of solar proton spectrum determination by data of limited number (20–25) of neutron monitor stations and with a simplified procedure of computations adapted for operative diagnostics of relativistic solar protons just arriving to the Earth. Possibilities of this truncated GLE modeling for the early forecast of radiation-dangerous fluxes of solar particles with moderate energies are also shown.

A method for real-time GLE modeling

Anashin, V., Belov, A., Eroshenko, E., Krjakunova, O., Mavromichalaki, H., Ishutin, I., Sarlanis, C., Souvatsoglo, G., Vashenyuk, E., and Yanke, V.: The ALERT signal of ground level enhancements of solar cosmic rays: physics basis, ways of realization and development, in: Proc. 31th ICRC, Lodz, ID 1104, 2009.; Cramp, L. J., Duldig, M. L., Flueckiger, E. O., Humble, J. E., Shea, M. A., and Smart, D. F.: The October 22, 1989, solar cosmic ray enhancement: an analysis of the anisotropy and spectral characteristics, Geophys. Res., 102, 24237–24248, 1997.; Ellison, D. C. and Ramaty, R.: Shock acceleration of electrons and ions in solar flares, Astrophys. J., 298, 400–408, 1985.; Kaminer, N. S.: About accounts of the barometrical coefficient during cosmic ray flares, Geomagnetism and Aeronomia, 7, 806–809, 1967.; Debrunner, H., Flueckiger, E., and Lockwood, J. A.: Response of Neutron Monitors to Solar Cosmic Ray Events: 8th European Cosmic Ray Symposium, Rome, Book of abstracts, 1984.; McCracken, K. G.: The cosmic ray flare effect 1. Some new methods and analysis, Geophys. Res., 67, 423–434, 1962.; Perez-Peraza, J., Vashenyuk, E. V., Miroshnichenko, L. I., Balabin, Yu. V., and Gallegos-Cruz, A.: Impulsive, Stohastic, and shock wave acceleration of relativistic protons in large solar events of 1989 September 29, 2000 July 14, 2003 October 28, and 2005 January 20, Astrophys. J., 695, 865–873, 2009.; Podgorny, I. M., Balabin, Yu. V., Podgorny, A. I., and Vashenyuk, E. V.: Spectrum of solar flare protons, Atmos. Solar-Terr. Phys., 72, 988–991, doi:10.1016/j. jastp.2010.05.010, 2010.; Shea, M. A. and Smart, D. F.: Possible evidence for a rigidity dependent release of relativistic protons from the solar corona, Space Sci. Rev., 32, 251–271, 1982.; Tsyganenko, N. A.: A magnetospheric magnetic field model with a warped tail current sheet, Planet Space Sci., 37, 5–20, 1989.; Tsyganenko, N. A.: A model of the near magnetosphere with a down-dusk asymmetry: 1. Mathematical structure, Geophys. Res., 107, 1176, doi:10.101029/2001JA000219, 2002.; Vashenyuk, E. V., Balabin, Yu. V., Perez-Peraza, J., Gallegos-Cruz, A., and Miroshnichenko, L. I.: Some features of relativistiс particles at the Sun in the solar cycles 21-23, Adv. Space Res., 38, 411–417, 2006a.; Vashenyuk, E. V., Balabin, Yu. V., and Gvozdevsky, B. B.: Relativistic solar protons in the event of 20 January, 2005. Modeling study, Geomagn. Aeronomy, 46, 449–455, 2006b.; Vashenyuk, E. V., Balabin, Yu. V., Gvozdevsky, B. B., and Schur, L. I.: The characteristics of relativistic solar cosmic rays in the event December 13, 2006, Geomagn. Aeronomy, 48, 249–153, 2008a.; Vashenyuk, E. V., Balabin, Yu. V., and Gvozdevsky, B. B.: Relativistic solar cosmic ray dynamics in large ground level events, in: Proc. 21-st ECRS, Kosice, Slovakia, 9–12 September, 2008., Inst. of Exp. Phys., Slovak Academy of Sci., 264–268, 2009.; Vashenyuk, E. V., Balabin, Yu. V., and Miroshnichenko, L. I.: Relativistic solar protons in the ground level event of 23 February 195


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