Interplanetary sector structure and the helliomagnetic equator

Details Interplanetary sector structure and the helliomagnetic equator Interplanetary sector structure and the helliomagnetic equator

Oct 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ap%26ss..24..371s&link_type=abstract

Astrophysics and Space Science, Volume 24, Issue 2, pp.371-383

Astronomy and Astrophysics

Astrophysics

71

Scientific paper

The magnetohydrodynamics of solar-wind flow lead logically to the formation of one warped annular neutral surface that apparently extends from ≈ 2 r &sun; (solar radii) to the boundary of the heliosphere. The most likely asymptotic configuration for this neutral sheet intersects the heliomagnetic equatorial plane along four corotating arcs. The observer sees a reversal of magnetic polarity on each crossing of the neutral surface, and so interprets each reversal as the crossing of a sector boundary.

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