Scintillation, density and turbulence in the interplanetary medium

Details Scintillation, density and turbulence in the interplanetary medium Scintillation, density and turbulence in the interplanetary medium

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990p%26ss...38..955t&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 38, Aug. 1990, p. 955-960.

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4

Density Distribution, Interplanetary Medium, Scintillation, Solar Flux Density, Solar Wind, Line Of Sight, Magnetohydrodynamic Waves, Plasma Density, Spatial Distribution, Temporal Distribution

Scientific paper

An attempt is made to reconcile the different power laws obtained when relating, on the one hand, interplanetary scintillation (IPS) to solar-wind density and, on the other, density turbulence to density. A numerical experiment was performed using a two-dimensional MHD model to simulate the solar wind in the ecliptic plane and then generating IPS g values by line-of-sight integration through the model solar wind. This simulation showed that any breakdown of the assumptions implicit in comparing a line-of-sight integral with a time average made near earth was insufficient to account for the difference.

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