Galactic cosmic ray fluctuation parameter as an indicator of the degree of magnetic field inhomogeneity

Author:

Kozlov V. I.,Kozlov V. V.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Geophysics

Reference14 articles.

1. Aivazyan, S.A., Enyukov, I.S., and Meshalkin, I.D., Prikladnaya statistika. Osnovy modelirovaniya i pervichnaya obrabotka dannykh (Applied Statistics: Modeling Backgrounds and Primary Data Processing), Moscow: Finansy i Statistika, 1983.

2. Belov, A.V. and Gaidash, S.P., Anomalously Low Solar and Geomagnetic Activities in 2007, Geomagn. Aeron., 2009, vol. 49, no. 5, pp. 595–602 [Geomagn. Aeron., (Engl. Transl.) 2009, vol. 49, pp. 566–573].

3. Frik, P.G., Turbulentnost’: podkhody i modeli (Turbulence: Approaches and Models), Moscow: Inst. Komp. Issled., 2003.

4. Ivanov, E.V. and Obridko, V.N., The Cyclic Variations of the CME Velocity, Sol. Phys., 2001, vol. 198, pp. 179–196.

5. Ivanov, E.V., Obridko, V.N., and Shelting, B.D., Large-Scale Structure of Solar Magnetic Fields and Coronal Mass Ejections, Pis’ma Astron. Zh., 1997, vol. 74, no. 2, pp. 273–277.

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