Observations of the solar wind with high temporal resolution

Details Observations of the solar wind with high temporal resolution Observations of the solar wind with high temporal resolution

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20..900z&link_type=abstract

Kosmicheskie Issledovaniia, vol. 20, Nov.-Dec. 1982, p. 900-906. In Russian.

Computer Science

6

High Resolution, Plasma Diagnostics, Satellite Observation, Solar Wind, Space Plasmas, Earth Magnetosphere, Plasma Spectra, Prognoz Satellites, Temporal Resolution

Scientific paper

During 1980-1981, the joint Soviet-Czechoslovakian plasma spectrometer ('Monitor') aboard the Prognoz-8 satellite was used to carry out high-temporal-resolution observations of processes in the solar wind and earth's magnetosphere. The objective of the experiment was to obtain continuous data on basic parameters of the solar wind, i.e., velocity, ion temperature and density, and arrival angles of the flow; as well as to investigate fast variations of the energy spectrum of the ion component of the solar wind in the interplanetary medium and at characteristic boundaries of the earth's magnetosphere. This paper describes the method of the experiment, and discusses first results relating to ion spectra and magnetospheric boundaries.

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