Physics
Scientific paper
Nov 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974impm.nasa...45d&link_type=abstract
"In its Interplanet. Medium and Phys. of the Magnetosphere (NASA-TT-F-784) p 45-58 (SEE N75-13707 04-90) Transl. into ENGLISH
Physics
Earth Magnetosphere, Plasma-Electromagnetic Interaction, Solar Wind, Geomagnetism, Magnetic Field Configurations, Magnetic Measurement, Magnetohydrodynamic Flow
Scientific paper
Plasma parameters for modeling of the interaction between the solar wind and the earth's magnetic field are selected on the limited modeling principle (plasma velocity 3 x 10 to the 7th power cm/sec, density 10 to the 13th power cm/3, electron temperature approximately 15 eV). Measurements were made with magnetic probes capable of developing all 3 components inside the magnetic field. The resulting magnetic field charts indicate that a neutral layer forms on the night side in the model experiments. A magnetosphere free of plasma streams is established on the daytime side. A shock wave forms on the boundary of the magnetosphere, its width c/omega0 in accordance with theory, where omega0 is the total Langmuir width.
Dubinin Edouard M.
Managadze George G.
Podgornyy I. M.
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