Physics of auroral phenomena : proceedings of the 34th Annual seminar, Apatity, 01 - 04 March, 2011 / [ed.: A. G. Yahnin, A. A. Mochalov]. - Апатиты : Издательство Кольского научного центра РАН, 2011. - 231 с. : ил.

Simulation o fthe transport ofsolarprotons through the atmosphere in the 13 December 2006 GLE Fig. 8. On this picture a simulated NM response function on protons, a proton ground level spectra and their product are numbered 1, 3 and 2 respectively. References [1] Vashenyuk E.V, Bazilevskaya G.A, Makhmutov V.S, et al,Proc. 30 ICRC, Merida, Mexico, 2007, 1, 221-224. [2] Vashenyuk E.V, Balabin Yu.V, Gvozdevsky B.B, Schur L.I.Geomagnetism and Aeronomia, 2008,48 (4), 1-7, [3] Vashenyuk E.V, Balabin Yu.V, and Gvozdevsky B.B. Proc. 21-st ECRS, Kosice, Slovakia, 2009, 264-268. [4] Desorgher L. PLANETOCOSMICS Software User Manual, Univ.of Bern, 2005. [5] Agostinelli et a l, Geant4 a simulation toolkit, Nuclear Instruments and Methods in Physics Research, Section A. 506, P.250-303, 2003. [6] Bazilevskaya G.A, M.B. Krajnev, V.S. Makhmutov et a l. Geomagnetism and aeronomy, 2003, 43, N.4, 442-452. [7] A.N. Charakhchyan, Investigation of stratosphere cosmic ray intensity fluctuations induced by processes on the Sun, Soviet Physics Uspekhi, 1964, 7 (3), 358-374. [8] V.S. Makhmutov, G.A. Bazilevskaya, et a l, JASR 2007,39(8), 1460-1463 [9] Maurchev E.A, B.B. Gvozdevsky, Yu.V. Balabin, E.V. Vashenyuk. Modeling of the response function of a neutron monitor. Proc. of 33 Apatity’s Seminar Phys. of Auroral Phenomena. Preprint PGI Apatity, .2011, 83-86. [10] C. Pioch, V. Mares, E.V. Vashenyuk, Yu.V. Balabin, W. Ruehm. Measurement of cosmic ray neutrons with Bonner sphere spectrometer and neutron monitor at 79° N, Nucl. Instr. and Meth. A 2010, doi:10.1016/j.nima.2010.10.030