Observations of recurrent high-velocity solar wind streams in declining phase of solar activity cycle 21 using wide-angle ion energy spectrometer aboard Prognoz-9 satellite

Details Observations of recurrent high-velocity solar wind streams in declining phase of solar activity cycle 21 using wide-angle ion energy spectrometer aboard Prognoz-9 satellite Observations of recurrent high-velocity solar wind streams in declining phase of solar activity cycle 21 using wide-angle ion energy spectrometer aboard Prognoz-9 satellite

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rpsct...1...41g&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 41 (SEE N87-29547 24-12) Transl. into ENGLISH from Kosmicheskiye Issle

Computer Science

Secular Variations, Solar Activity Effects, Solar Cycles, Solar Wind, Solar Wind Velocity, Mass Spectrometers, Prognoz Satellites, Satellite-Borne Instruments, Spacecraft Trajectories, Wide Angle Lenses

Scientific paper

Solar wind measurements made on the Prognox-9 satellite during the period from July 1983 to February 1984 in the declining phase of solar cycle 21 afforded a possibility for checking the reliability of conclusions concerning long-period variations of solar wind properties drawn on the basis of earlier experiments. Measurements of the plasma ion component were made by the modulation method using the D-137A ion energy spectrometer. The velocity of some of the solar wind streams attained 700 to 800 km/s. The data demonstrate the renewal of the regular structure of high velocity streams in the solar wind in the declining phase, as predicted earlier on the basis of solar wind measurements in the preceding cycle, indicating that the presence of recurrent high-velocity streams in the declining phases of the 11-year solar cycles is a regular feature of such cycles.

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