Rotation Rates of Soft X-ray Coronal Structures

Details Rotation Rates of Soft X-ray Coronal Structures Rotation Rates of Soft X-ray Coronal Structures

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..359k&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.359-362.

Physics

3

Scientific paper

Characteristics of rotation of large-scale coronal structures are investigated by using soft X-ray synoptic charts constructed by daily Yohkoh soft X-ray images. An autocorrelation technique was used in order to obtain the rotation periods of the soft X-ray structures for every five degrees in the latitude. The analysis shows that the rotation periods in the northern hemisphere are different from those of the southern hemisphere. The rotation periods of active regions are also different from those of quiet coronal structures in he low latitudinal range. It is suggested that these differences influenced the heliospheric structure in the analyzed period.

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