Seasonal and solar activity changes of F-region electron density, electron temperature and protonospheric heat flux during the declining part of sunspot cycle 20

Details Seasonal and solar activity changes of F-region electron density, electron temperature and protonospheric heat flux during the declining part of sunspot cycle 20 Seasonal and solar activity changes of F-region electron density, electron temperature and protonospheric heat flux during the declining part of sunspot cycle 20

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ijrsp..16..251p&link_type=abstract

Indian Journal of Radio and Space Physics (ISSN 0367-8393), vol. 16, June 1987, p. 251-256.

Physics

Space Physics

Electron Energy, F Region, Ionospheric Electron Density, Proton Belts, Solar Activity Effects, Sunspots, Annual Variations, Heat Flux, Incoherent Scatter Radar

Scientific paper

The daytime measurements of electron temperature (Te) and concentration (Ne) from incoherent scatter radar at Millstone Hill are analyzed for the period Jan. 1968-Dec. 1973. These data cover the solar maximum and a major portion of declining part of the sunspot cycle 20. The purpose of the analysis was to look for the seasonal and solar activity changes of F-region Ne, Te and protonospheric heat flux during the declining part of the sunspot cycle 20 and also to compare the present results with the earlier results during the rising part of this sunspot cycle. It is found that while there is no major difference in the seasonal behavior of F-region Ne and Te between the rising and the declining parts of the sunspot cycle 20, the variation of daytime heat flux shows significant asymmetry between the rising and the declining phases of this sunspot cycle.

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