Latitude-dependent nonlinear high-speed solar wind streams

Details Latitude-dependent nonlinear high-speed solar wind streams Latitude-dependent nonlinear high-speed solar wind streams

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jgr....80.2023s&link_type=abstract

Journal of Geophysical Research, vol. 80, June 1, 1975, p. 2023-2029.

Astronomy and Astrophysics

Astronomy

5

Magnetohydrodynamic Flow, Plasma Interactions, Rotating Plasmas, Solar Rotation, Solar Wind Velocity, Astronomical Models, Latitude, Radial Flow, Scintillation, Solar Longitude, Stream Functions (Fluids)

Scientific paper

A perturbation expansion of the global (not limited to the equatorial plane) equations of motions is described for the case of hydrodynamic flow, beyond the critical point, of a polytropic single fluid. A global model for the interaction between high- and low-speed streams in the solar wind is then developed, assuming nearly radial flow in the solar wind. It is shown that the disappearance of streams above 40 deg N is not necessary to explain a weakening of stream interactions and thus the disappearance of scintillations at high solar latitudes.

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