Determination of the pitch-angle distribution and transverse anisotropy of interplanetary particles

Details Determination of the pitch-angle distribution and transverse anisotropy of interplanetary particles Determination of the pitch-angle distribution and transverse anisotropy of interplanetary particles

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..330n&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 330-333 (SEE N85-34729 23-92)

Mathematics

Interplanetary Magnetic Fields, Solar Cosmic Rays, Solar Protons, Solar Wind Velocity, Correlation, Distribution (Property), Mathematical Models, Poisson Density Functions, Solar Wind

Scientific paper

A method to determine the directional differential intensity (d.d.i.),
expressed in terms of spherical harmonics, from sectored particle data,
concurrent interplanetary magnetic field (IMF) and solar wind velocity
is presented.

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