Evolution of the structure of the interplanetary medium within the limits of the Mars orbit

Details Evolution of the structure of the interplanetary medium within the limits of the Mars orbit Evolution of the structure of the interplanetary medium within the limits of the Mars orbit

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45.1335v&link_type=abstract

(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia

Physics

Interplanetary Medium, Long Term Effects, Mars (Planet), Solar Activity, Cosmic Rays, Diurnal Variations, Interplanetary Magnetic Fields, Milky Way Galaxy, Terrestrial Planets

Scientific paper

An analysis of variable helioefficiency (or solar-activity efficiency) for Mercury, Venus, the earth, and Mars is used to consider the double-helical structure of the interplanetary medium. The study of helioefficiency is based on an investigation of diurnal values of Sp for 1911-1970. Data on the behavior of cosmic rays at various phases of the 22-year cycle and on interplanetary magnetic fields near the earth's orbit suggest that the double-helical structure reflects the structure of the solar magnetosphere within the Mars orbit.

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