Effects of a wavy neutral sheet on cosmic ray anisotropies

Details Effects of a wavy neutral sheet on cosmic ray anisotropies Effects of a wavy neutral sheet on cosmic ray anisotropies

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..453k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 453-456 (SEE N85-34729 23-92)

Computer Science

Numerical Analysis

Anisotropy, Cosmic Ray Showers, Diffusion Coefficient, Galactic Cosmic Rays, Heliosphere, Magnetic Equator, Neutral Sheets, Numerical Analysis, Polarity, Solar Magnetic Field, Solar Wind, Models, Reversing, Solar Cycles, Three Dimensional Models

Scientific paper

The authors present the first results of their 3-D numerical code calculating cosmic ray anisotropies. The code includes diffusion, convection, adiabatic cooling, and drift in an interplanetary magnetic field model containing a wavy neutral sheet. They find that the 3-D model can reproduce all the principal observations for a resonable set of parameters.

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