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[en] Interplanetary magnetic field data from the different satellites obtained during the period 1963-1973 at 1 A.U. and compiled by J. King have been analysed in heliocentric ecliptic coordinates. The peculiarities of the background interplanetary magnetic field (BIMF) are discussed in relation to the orinetation of the solar system in the Galaxy and the variable helioefficiency of the planets. The results of the direct cosmic experiments are evidence of the solar activity being a complex phenomenon of the solar system as a whole. (Auth.)
Source
Dryer, M. (National Oceanic and Atmospheric Administration, Boulder, CO (USA). Space Environment Lab.); Tandberg-Hanssen, E. (National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center) (eds.); International Council of Scientific Unions. Special Committee on Solar-Terrestrial Physics; Committee on Space Research. (COSPAR), 75-Paris (France); 577 p; ISBN 90-277-1163-1; 
; 1980; p. 167-172; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 91 on solar and interplanetary dynamics; Cambridge, MA, USA; 27 - 31 Aug 1979
; 1980; p. 167-172; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 91 on solar and interplanetary dynamics; Cambridge, MA, USA; 27 - 31 Aug 1979