AbstractSimilar 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 geomagnetic 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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    Title :

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


    Contributors:

    Published in:

    Publication date :

    1993-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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