NDLI: Effects of solar magnetic field on cosmic rays

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Effects of solar magnetic field on cosmic rays

Content Provider	NASA Technical Reports Server (NTRS)
Author	Stekolnikov, N. V. Goncher, G. A. Lyakhova, A. K. Kolomeets, E. V. Slyunyaeva, N. V.
Copyright Year	1985
Description	Aspects of the problem of galactic cosmic ray propagation, including inversion of the solar total magnetic field and an analysis of data related to the heliomagnetic cycle are discussed. It is noted that the global structure of the solar magnetic field results in an additional flux of galactic cosmic rays generated by curvature and gradient drifts. An analysis of heliomagnetic cycle data shows that the latitudinal gradient results in a N-S asymmetry, with the amplitude of the effect growing with depth in the atmosphere. The inversion of the solar total magnetic field, drift effects, and other space distributions are found to contribute to a 22-year cycle of solar activity.
File Size	227928
Page Count	4
File Format	PDF
Alternate Webpage(s)	http://archive.org/details/NASA_NTRS_Archive_19850026537
Archival Resource Key	ark:/13960/t9t19wc62
Language	English
Publisher Date	1985-08-01
Access Restriction	Open
Subject Keyword	Space Radiation Cosmic Ray Showers Magnetic Field Inversions Modulation Galactic Cosmic Rays Convective Flow Rigidity Kinetic Energy Solar Cycles Diffusion Coefficient Curvature Solar Magnetic Field Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science
Content Type	Text
Resource Type	Article

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