The spiral structure of the interplanetary magnetic field

Details The spiral structure of the interplanetary magnetic field The spiral structure of the interplanetary magnetic field

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976georl...3..561p&link_type=abstract

Geophysical Research Letters, vol. 3, Sept. 1976, p. 561-564.

Physics

2

Interplanetary Magnetic Fields, Magnetic Field Configurations, Pioneer 10 Space Probe, Solar Wind Velocity, Data Reduction, Long Term Effects, Radial Distribution, Solar Corona, Spatial Distribution, Spirals, Wind Effects, Wind Velocity Measurement

Scientific paper

The Pioneer 10 data concerning the heliocentric radial variation of the interplanetary magnetic field are examined. Incorporating the systematic increase in solar wind velocity observed during the mission leads to much improved agreement between the usual Parker Archimedean spiral and the data. The effects of correlations between short-period fluctuations of speed and azimuthal field are discussed. It is concluded that during the period under study they did not substantially affect the average magnetic field.

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