Magnetic and thermal energies in the solar wind

Details Magnetic and thermal energies in the solar wind Magnetic and thermal energies in the solar wind

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...40..231d&link_type=abstract

Solar Physics, vol. 40, Jan. 1975, p. 231-234. Research supported by the Consiglio Nazionale delle Ricerche.

Physics

Magnetic Fields, Plasma Flux Measurement, Satellite Observation, Solar Flux Density, Solar Wind, Thermal Energy, Equipartition Theorem, Spatial Distribution, Standard Deviation, Statistical Distributions

Scientific paper

Data obtained by the Vela 3/IMP 3, Explorer 34, and HEOS 1 spacecraft on the proton thermal energy and the magnetic energy density in the solar wind are compared. The analysis indicates that, on the average, there is a linear relationship between these parameters, which implies the equipartition of energy between the plasma and the magnetic field. The data from Vela 3/IMP 3 deviate from those obtained by Explorer 34 and HEOS 1, and explanations for this are proposed.

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