Dependence of proton fluxes measured by the Mars-7 probe during January-February 1974 on parameters of the interplanetary medium

Details Dependence of proton fluxes measured by the Mars-7 probe during January-February 1974 on parameters of the interplanetary medium Dependence of proton fluxes measured by the Mars-7 probe during January-February 1974 on parameters of the interplanetary medium

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981kosis..19..150m&link_type=abstract

Kosmicheskie Issledovaniia, vol. 19, Jan.-Feb. 1981, p. 150-153. In Russian.

Physics

Interplanetary Medium, Plasma Interactions, Proton Flux Density, Solar Wind Velocity, Energy Spectra, Mars Probes, Particle Acceleration, Pioneer 11 Space Probe, Proton Energy, Space Plasmas

Scientific paper

The relationship between proton fluxes from 1 to 3.5 AU from the sun and characteristics of the interplanetary medium (IM) is studied on the basis of Mars-7 and Pioneer-11 data. Variations of proton intensity are investigated in relation to the characteristics of the IM and the solar wind velocity. Proton intensity is found to increase with distance from the sun, a phenomenon which is believed to be caused by turbulent acceleration.

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