The global solar wind and predictions for Pioneers 10 and 11

Details The global solar wind and predictions for Pioneers 10 and 11 The global solar wind and predictions for Pioneers 10 and 11

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975georl...2...75s&link_type=abstract

Geophysical Research Letters, vol. 2, Mar. 1975, p. 75-77.

Physics

6

Interplanetary Magnetic Fields, Meridional Flow, Pioneer 10 Space Probe, Pioneer 11 Space Probe, Prediction Analysis Techniques, Solar Wind Velocity, Magnetic Flux, Mass Transfer, Pressure Gradients, Synoptic Measurement

Scientific paper

The dependence on latitude of the azimuthal component of the interplanetary magnetic field generates a meridional pressure gradient which, in turn, generates a meridional flow. This flow has observable consequences in the equatorial plane, although the meridional velocity itself may be zero in this plane. Analytic estimates of these observables - the mass flux, azimuthal and radial magnetic flux, density, and spiral angle - are made in the range of 1 to 12 AU.

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