On the cause of observed solar wind velocity variation around Hale type sector boundary

Details On the cause of observed solar wind velocity variation around Hale type sector boundary On the cause of observed solar wind velocity variation around Hale type sector boundary

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986p%26ss...34..861g&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 34, Sept. 1986, p. 861, 862.

Physics

Solar Wind Velocity, Current Sheets, Interplanetary Magnetic Fields, Solar Magnetic Field, Variations

Scientific paper

The concept of a positive gradient in the solar wind velocity with respect to the heliomagnetic latitude and the change in the heliomagnetic latitude of the Earth has been utilized to explain the differences in the solar wind velocity variation around +/- and -/+ IMF sector boundaries in northern and southern heliolatitudes. It is shown that, using a sinusoidal symmetric heliospheric current sheet, one can explain the observed solar wind changes around the Hale and non-Hale types of sector boundaries.

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