Temporal evolution of the equatorial K-corona

Details Temporal evolution of the equatorial K-corona Temporal evolution of the equatorial K-corona

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...55..143m&link_type=abstract

Solar Physics, vol. 55, Nov. 1977, p. 143-159.

Physics

7

K Lines, Solar Corona, Solar Magnetic Field, Time Dependence, Harmonic Analysis, Solar Eclipses, Solar Physics

Scientific paper

Variation of the equatorial K-corona radiance at 2.5 solar radii from the sun center was studied on a daily basis during the Skylab mission (May 1973 to February 1974). The radiance data may be divided into three periods, the first characterized by a smooth variation in time, the second by a signal that is neither persistent in the short term nor recurrent from one limb passage to the next, and the third (and longest period) by a signal exhibiting an orderly, periodically increasing intensity. The data may be interpreted as indicating a general simplification of the coronal magnetic field; harmonic analysis of the surface field provides additional information on the evolution of the equatorial K-corona structures.

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