Variation of the solar atmospheric rotation over the 11 year cycle

Details Variation of the solar atmospheric rotation over the 11 year cycle Variation of the solar atmospheric rotation over the 11 year cycle

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...45..533e&link_type=abstract

Solar Physics, vol. 45, Dec. 1975, p. 533-542.

Astronomy and Astrophysics

Astronomy

3

Solar Atmosphere, Solar Cycles, Solar Radio Emission, Solar Rotation, Twenty-Seven Day Variation, Microwave Spectra, Power Spectra, Radio Astronomy

Scientific paper

The synodic rotation period and power spectra of solar microwave sources are investigated using accurate data in the interval 1956 to 1970. The variation of the approximate 27-day period is obtained over a complete solar cycle and is thought to be a result of the latitudinal change over the solar cycle of the origins of the radio emissions. High-resolution power spectra have also been obtained and have revealed the existence of a double-peaked line near 160-day period. This line is attributed to changes in either the earth's heliographic latitudes or the earth's inclination to the earth-sun line.

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