Analysis of geomagnetic field data and cosmic rays variations during periods of increased solar activity
Vestnik KRAUNC. Fiziko-matematičeskie nauki, no. 3 (2016), pp. 40-46 Cet article a éte moissonné depuis la source Math-Net.Ru

Voir la notice de l'article

We performed analysis of the cosmic rays variations and studied features of geomagnetic field variations during periods of increased solar activity. The paper applies a new methods of modeling and analysis of the data developed by the authors based on wavelet transform and neuron networks. In this paper we allocated anomalous changes in cosmic rays that occurred some hours before geomagnetic storms.
Keywords: geomagnetic activity, cosmic rays, wavelet transform.
@article{VKAM_2016_3_a5,
     author = {O. V. Mandrikova and T. L. Zalyaev and I. S. Solovev and S. Yu. Khomutov},
     title = {Analysis of geomagnetic field data and cosmic rays variations during periods of increased solar activity},
     journal = {Vestnik KRAUNC. Fiziko-matemati\v{c}eskie nauki},
     pages = {40--46},
     year = {2016},
     number = {3},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/VKAM_2016_3_a5/}
}
TY  - JOUR
AU  - O. V. Mandrikova
AU  - T. L. Zalyaev
AU  - I. S. Solovev
AU  - S. Yu. Khomutov
TI  - Analysis of geomagnetic field data and cosmic rays variations during periods of increased solar activity
JO  - Vestnik KRAUNC. Fiziko-matematičeskie nauki
PY  - 2016
SP  - 40
EP  - 46
IS  - 3
UR  - http://geodesic.mathdoc.fr/item/VKAM_2016_3_a5/
LA  - ru
ID  - VKAM_2016_3_a5
ER  - 
%0 Journal Article
%A O. V. Mandrikova
%A T. L. Zalyaev
%A I. S. Solovev
%A S. Yu. Khomutov
%T Analysis of geomagnetic field data and cosmic rays variations during periods of increased solar activity
%J Vestnik KRAUNC. Fiziko-matematičeskie nauki
%D 2016
%P 40-46
%N 3
%U http://geodesic.mathdoc.fr/item/VKAM_2016_3_a5/
%G ru
%F VKAM_2016_3_a5
O. V. Mandrikova; T. L. Zalyaev; I. S. Solovev; S. Yu. Khomutov. Analysis of geomagnetic field data and cosmic rays variations during periods of increased solar activity. Vestnik KRAUNC. Fiziko-matematičeskie nauki, no. 3 (2016), pp. 40-46. http://geodesic.mathdoc.fr/item/VKAM_2016_3_a5/

[1] Toptygin I.N., Space Rays in Interplanetary Magnetic Fields, Nauka, M, 1983, 301 pp.

[2] Ruffolo D.,, “Transport and acceleration of energetic charged particles near an oblique shock”, Astrophys. J., 1999, no. 515, 787-800 | DOI

[3] Belov, A. V et al., “Cosmic ray anisotropy before and during the passage of major solar wind disturbances”, Adv. Space Res., 31:4 (2003), 919-924 | DOI

[4] Vecchio et al., “Insights on Cosmic Ray Modulation through a Joint Use of Nonstationary Data-Processing Methods”, Advances in Astronomy, 2012 | DOI

[5] Mandrikova O.V., Solovev I.S, Zalyaev T.L., “Methods of analysis of geomagnetic field variations and cosmic ray data”, Earth Planet Space, 66 (2014) | DOI

[6] Mandrikova O.V., Zalyaev T.L., “Modelirovanie variatsiy kosmicheskikh luchey i vydelenie anomaliy na osnove sovmeshcheniya veyvlet-preobrazovaniya s neyronnymi setyami”, Tcifrovaya obrabotka signalov, 2015, no. 1, 11-16

[7] Paschalis P. et al., “Artificial Neural Network Approach of Cosmic Ray Primary Data Processing”, Solar Physics, 182:1 (2013), 303-318 | DOI

[8] Mandrikova O.V. et al,, “Analysis of the Earth’s magnetic field variations on the basis of a wavelet-based approach”, Digit Signal Process, 23 (2013), 329-339 | DOI | MR

[9] Chui, C.K., An introduction in wavelets, Academic Press, New York, 1992, 264 pp. | MR

[10] Levin B. R., Teoreticheskie osnovy statisticheskoy radiotekhniki, Sov. radio, M., 1975, 392 pp. | MR