Fields and plasmas in the outer solar system

Details Fields and plasmas in the outer solar system Fields and plasmas in the outer solar system

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ssrv...23..217s&link_type=abstract

(COSPAR, IAU, IUGG, IUPAP, and URSI, International Symposium on Solar Terrestrial Physics, Innsbruck, Austria, May 29-June 3, 19

Astronomy and Astrophysics

Astronomy

30

Interplanetary Magnetic Fields, Magnetohydrodynamic Stability, Rarefied Plasmas, Solar System, Solar Wind, Spaceborne Astronomy, High Speed, Shock Wave Propagation, Solar Activity Effects, Solar Wind Velocity

Scientific paper

The most significant data on fields and plasmas in the outer solar system, based on observations by Pioneer 10 and 11, are reviewed. Attention is given to (1) corotating shocks and the evolution of high speed solar wind streams, (2) the effect of the changing structure of the interplanetary medium on energetic particles, (3) the propagation of flare-generated shocks through the outer solar system, (4) radial gradients in the solar wind and interplanetary field, and (5) the dependence of the interplanetary sector structure on heliographic latitude.

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