Coronal rotation dependence on the solar cycle phase

Details Coronal rotation dependence on the solar cycle phase Coronal rotation dependence on the solar cycle phase

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...53..179a&link_type=abstract

Solar Physics, vol. 53, July 1977, p. 179-188.

Physics

22

Solar Corona, Solar Cycles, Solar Rotation, Angular Velocity, Solar Activity, Solar Spectra, Sunspots

Scientific paper

The rotation rate of coronal features observed in the green line (5303 A) of Fe XIV during the period 1970 to 1974 is studied. It is found that coronal features associated with solar activity rotate differentially, while those characteristic of years of declining activity (1972 to 1974) rotate almost rigidly. Data on coronal holes is interpreted by means of the rotation rate, and tracking of sunspot migration toward the equator by changes in the rotational behavior of the corona is also considered.

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