Energy spectrum of radio waves emitted by Venera 10 in the radio occultation of the circumsolar medium, and determination of plasma turbulence characteristics

Details Energy spectrum of radio waves emitted by Venera 10 in the radio occultation of the circumsolar medium, and determination of plasma turbulence characteristics Energy spectrum of radio waves emitted by Venera 10 in the radio occultation of the circumsolar medium, and determination of plasma turbulence characteristics

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978kosis..16..419e&link_type=abstract

Kosmicheskie Issledovaniia, vol. 16, May-June 1978, p. 419-428. In Russian.

Physics

5

Energy Spectra, Plasma Turbulence, Radio Occultation, Solar Wind, Venera Satellites, Decametric Waves, Ecliptic, Fast Fourier Transformations, Normal Density Functions, Radio Signals, Radio Spectra, Signal To Noise Ratios, Solar Wind Velocity

Scientific paper

Data are presented on the behavior of the energy spectrum of radio waves in a radio occultation experiment. The radio emission bandwidths are determined, along with the frequency dependence of the spectral energy density. The variation of these quantities as a function of the angular distance between the instrument and the sun is studied. It is shown that for angular distances greater than 2 degrees, the wings of the spectra may be approximated by a power law with an exponent of 2.7. For angular distances less than 1.5 degrees, the shape of the spectrum becomes nearly Gaussian.

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