A reexamination of the radial dependence of weak interplanetary scintillation

Details A reexamination of the radial dependence of weak interplanetary scintillation A reexamination of the radial dependence of weak interplanetary scintillation

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979dsnpr..50..119b&link_type=abstract

In its The Deep Space Network p 119-123 (SEE N79-22140 13-12)

Physics

Deep Space Network, Electron Density (Concentration), Electron Trajectories, Interplanetary Medium, Scintillation, Solar Wind, Radial Distribution, Solar Corona, Solar Physics, Weak Energy Interactions

Scientific paper

The power law radial dependence of the scintillation index is examined.
The signal path integration shows total radial dependence of
approximately the closet approach distance to the power of 1/1.5. It was
concluded that most manifestation of columnar solar wind turbulence are
proportional to signal path integrated electron density.

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