Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....8910659b&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 89, Dec. 1, 1984, p. 10659-10668. Previously announced in STAR as N84-287
Astronomy and Astrophysics
Astronomy
52
Interplanetary Magnetic Fields, Magnetic Variations, Solar Activity Effects, Astronomical Models, Heliosphere, International Sun Earth Explorer 3, Plasma Density, Solar Activity, Solar Rotation, Solar Wind, Sun, Voyager 1 Spacecraft, Voyager 2 Spacecraft
Scientific paper
The large-scale radial and temporal variations of the interplanetary magnetic field strength B observed by Voyagers 1 and 2 are discussed. Two components of the magnetic field strength were considered: (1) an average component, Bzero, based on solar rotation averages, and (2) a fluctuation component, delta B, expressed by 10- or 24-hour averages of B normalized by the best-fit average field for the corresponding time and distance. Observations of the sector structure, interfaces, and shocks are presented to further describe magnetic field strength.
Behannon Kenneth W.
Burlaga Leonard Francis
Klein Larry W.
Lepping Ronald P.
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