Solar wind turbulence models evaluated via observations of Doppler RMS phase fluctuation and spectral broadening in the inner corona

Details Solar wind turbulence models evaluated via observations of Doppler RMS phase fluctuation and spectral broadening in the inner corona Solar wind turbulence models evaluated via observations of Doppler RMS phase fluctuation and spectral broadening in the inner corona

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978dsnpr..44..197b&link_type=abstract

In its The Deep Space Network p 197-202 (SEE N78-24212 15-12)

Physics

Doppler Effect, Solar Wind, Turbulence, Turbulence Models, Deep Space Network, Electron Density (Concentration), Flux (Rate), Models, Solar Corona

Scientific paper

Doppler noise observations in the inner corona are shown to demonstrate that Doppler noise is proportioned to integrated electron density. Similarly, spectral broadening in the inner corona is seen to be proportional to integrated density. It is concluded that the particle flux models are in disagreement with the experimental observations of Doppler noise to date, and hence are unlikely to be representative of actual solar wind processes.

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