Physics
Scientific paper
Apr 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975svphu.114..382i&link_type=abstract
(Uspekhi Fizicheskikh Nauk, vol. 114, Oct. 1974, p. 382, 383.) Soviet Physics - Uspekhi, vol. 17, Mar.-Apr. 1975, p. 807-809. Tr
Physics
Interplanetary Medium, Magnetic Signatures, Magnetohydrodynamic Flow, Solar Flares, Solar Wind, Astronomical Models, Chromosphere, Cosmic Rays, Diurnal Variations, Forbush Decreases, Geos 2 Satellite, Shock Wave Propagation
Scientific paper
The theory of second-order discontinuities has been applied to magnetic-field and plasma measurements by spacecraft to model the structure of interplanetary flows from chromospheric flares. Refinements are suggested for the model proposed by Hundhausen in 1972. Measurements of magnetic-field intensity, electrons, and energetic protons by the Geos 2 spacecraft and of the cosmic-ray intensity at Irkutsk are considered. The present level of knowledge of the structure of plasma flows can be used for further research on the interplanetary medium and for refining our conceptions of the cosmic and geophysical effects of the solar wind.
No associations
LandOfFree
Structure of the typical nonstationary stream of interplanetary plasma from direct measurements 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 Structure of the typical nonstationary stream of interplanetary plasma from direct measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of the typical nonstationary stream of interplanetary plasma from direct measurements will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-949521