Exponential anisotropy of solar cosmic rays

Details Exponential anisotropy of solar cosmic rays Exponential anisotropy of solar cosmic rays

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4r.335b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 335-338 (SEE N85-34729 23-92)

Mathematics

1

Neutrons, Propagation, Scattering, Solar Cosmic Rays, Solar Flares, Boltzmann Transport Equation, Interplanetary Magnetic Fields, Interplanetary Space, Mathematical Models, Sun

Scientific paper

On 16 February 1984 a flare on the Sun's invisible disk produced a
large, highly anisotropic solar particle event. A technique, in which
interplanetary scattering parameters are determined purely from the form
of the particle anisotropy, is applied to energetic particle data from
neutron monitors and the ICE spacecraft.

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