Volume scattering model for interpretation of solar radar experiments

Details Volume scattering model for interpretation of solar radar experiments Volume scattering model for interpretation of solar radar experiments

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..149..413c&link_type=abstract

Solar Physics, vol. 149, no. 2, p. 413-416

Astronomy and Astrophysics

Astronomy

7

Irregularities, Radar Astronomy, Radar Measurement, Radar Scattering, Solar Corona, Solar Radar Echoes, Stellar Models, Backscattering, Heliosphere, Magnetohydrodynamic Turbulence, Magnetohydrodynamic Waves, Mathematical Models, Solar Atmosphere, Solar Wind, Solar Wind Velocity

Scientific paper

It is shown that solar radar experiments carried out at lambda = 8 m can be explained on the assumption that the reflected signal is formed as a result of multiple volume scattering on large-scale (about 1 km) irregularities of the outer corona. The region of effective scattering is located at the heliocentric distance r approximately equal twice the solar radius, i.e., considerably higher than the region of surface mirror reflection. Measured characteristics of reflected signals are in good agreement with the theoretical model.

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