Dynamics of the penetration boundaries of solar protons during a strong magnetic storm

Details Dynamics of the penetration boundaries of solar protons during a strong magnetic storm Dynamics of the penetration boundaries of solar protons during a strong magnetic storm

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..348g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 348-351 (SEE N85-34991 23-93)

Computer Science

1

Boundaries, Earth Magnetosphere, Magnetic Storms, Penetration, Solar Atmosphere, Solar Cosmic Rays, Solar Protons, Solar Storms, Charged Particles, Energetic Particles, Nuclear Vulnerability, Solar Corpuscular Radiation

Scientific paper

The variations in the equatorial penetration boundary of solar protons with Ep = 0.9 to 8.0 MeV during a strong magnetic storm of April 3 to 5, were analyzed. The dynamics of this boundary is compared with the dynamics of the outer trapping boundary of electrons with Ee = - 0.3 to 0.6 MeV. The solar-proton penetration and the structure of the real magnetic field are studied. The unique data on the thin structure of development of a magnetospheric substorm were obtained for the first time.

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