Longitudinal structure of quasi-steady equatorial coronal holes near solar minima and their phase reversal

Details Longitudinal structure of quasi-steady equatorial coronal holes near solar minima and their phase reversal Longitudinal structure of quasi-steady equatorial coronal holes near solar minima and their phase reversal

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994adspr..14...77z&link_type=abstract

Advances in Space Research, vol. 14, no. 4, p. (4)77-(4)80

Astronomy and Astrophysics

Astronomy

1

Coronal Holes, Solar Corona, Solar Cycles, Solar Magnetic Field, Solar Rotation, Geomagnetism, Satellite Observation, Solar Wind, Spaceborne Astronomy, Stellar Evolution

Scientific paper

Similar quasi-steady two-peak corotating structures during the descending and/or the minimum phases can be recognized from each series of the even or odd solar cycles. However, the phase of the structure seems to shift a large amount, probably reversing, from one cycle to the next. Such quasi-steady structures were inferred from the geo-magnetic data, and have been confirmed by the coronal and interplanetary observations during the last two solar cycles. The implications about the long-term evolution of the tilted general solar magnetic field are discussed.

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