Physics
Scientific paper
Nov 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981kosis..19..869v&link_type=abstract
Kosmicheskie Issledovaniia, vol. 19, Nov.-Dec. 1981, p. 869-875. In Russian.
Physics
Cosmic Rays, Satellite Observation, Solar Activity Effects, Solar Wind, Flux Quantization, Interplanetary Medium, Mars Probes, Prognoz Satellites, Temporal Distribution
Scientific paper
Electron fluxes with energies not less than 40 keV were measured by Prognoz 3 and Mars 7 in January 1974. The behavior of the fluxes was studied as a function of the solar wind velocity and the parameters of the interplanetary magnetic field. Data on proton fluxes with energies of 1-5 MeV were also analyzed. It is shown that electrons are subject to a greater degree than protons to modulation by high-velocity solar wind fluxes at radial distances up to 1.5 AU from the sun. Electron flux gradients at distances up to 1.5 AU from the sun are obtained, and the origin of electron fluxes in the interplanetary medium is considered.
Kuzhevskii B. M.
Shestopalov I. P.
Spirkova E. S.
Vakulov P. V.
Vologdin N. I.
No associations
LandOfFree
Cosmic ray modulation by high-velocity solar-wind fluxes studied on the basis of measurements from the Prognoz-3 satellite and the Mars-7 probe in January 1974 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Cosmic ray modulation by high-velocity solar-wind fluxes studied on the basis of measurements from the Prognoz-3 satellite and the Mars-7 probe in January 1974, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic ray modulation by high-velocity solar-wind fluxes studied on the basis of measurements from the Prognoz-3 satellite and the Mars-7 probe in January 1974 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-744467