Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..462l&link_type=abstract
(Mezhdunarodnyi Seminar po Korpuskuliarnye Potoki Solntsa i Radiatsionnye Poiasa Zemli i Iupitera, 7th, Leningrad, USSR, May 25-
Astronomy and Astrophysics
Astronomy
3
Anisotropic Media, Interplanetary Medium, Solar Cosmic Rays, Solar Protons, Astronomical Models, Conjugate Points, Lines Of Force, Solar Flares, Solar Magnetic Field
Scientific paper
A model is developed to explain the increase in the intensity of solar protons with a long-duration, sign-variable, large-amplitude anisotropy observed by Mars 4, 5 and 7 spacecraft in September 1973. According to the model, solar cosmic ray protons ejected by a flare in the southern hemisphere of the sun, arrive to the point of observation by means of two routes: one flux moves from the sun along the magnetic field lines, first beneath the equatorial plane, then changes direction beyond the earth's orbit, and returns to the sun above the equatorial plane; the second flux from the southern hemisphere moves to the conjugate point of the northern hemisphere along the magnetic field lines of the near zone or diffuses into the solar corona, after which it moves away from the sun above the equatorial plane.
Ignat'ev P. P.
Kontor N. N.
Liubimov G. P.
Pereslegina N. V.
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