A method for determining corotating interaction regions in the equatorial plane of the heliosphere from solar wind velocity data

Details A method for determining corotating interaction regions in the equatorial plane of the heliosphere from solar wind velocity data A method for determining corotating interaction regions in the equatorial plane of the heliosphere from solar wind velocity data

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jgr....9113689o&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 91, Dec. 1, 1986, p. 13689-13693.

Physics

5

Corotation, Equatorial Regions, Heliosphere, Solar Wind Velocity, Computerized Simulation, Lines Of Force, Shock Waves, Streamlining, Wave Generation

Scientific paper

An Euler-Lagrange coordinate transformation is applied to a computed solar wind velocity data set to obtain fluid streamlines which are also magnetic field lines. Plotting these lines for high-resolution simulation data provides detailed information about the time variation of corotating interaction regions in the equatorial plane of the heliosphere.

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