Solar-wind recurrence as a function of heliolatitude

Details Solar-wind recurrence as a function of heliolatitude Solar-wind recurrence as a function of heliolatitude

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56..872b&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, July-Aug. 1979, p. 872-875. In Russian.

Physics

Solar Physics, Solar Rotation, Solar Wind Velocity, Correlation, Latitude, Scintillation, Spectroheliographs, Statistical Analysis

Scientific paper

A statistical analysis of the heliolatitudinal recurrence of the solar wind is performed. The results demonstrate that the dependence of the solar-wind velocity correlation period on heliolatitude is consistent with concepts of differential solar rotation and that solar-wind streams participate in the differential rotation of the sun. It is shown that interplanetary scintillation provides a possible means for studying solar-wind recurrence at high heliolatitudes, which are not well accessible for other methods.

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