Rigidly rotating component of the solar corona

Details Rigidly rotating component of the solar corona Rigidly rotating component of the solar corona

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ncimb..25..513a&link_type=abstract

Nuovo Cimento, Sezione B, vol. 25 B, Feb. 11, 1975, p. 513-520.

Physics

1

Autocorrelation, Line Spectra, Solar Corona, Solar Magnetic Field, Solar Rotation, Cross Correlation, Latitude, Luminous Intensity, Periodic Variations, Solar Atmosphere, Spectrum Analysis, Time Series Analysis

Scientific paper

Autocorrelation analyses of green-line intensity data for the period 1947-70 at latitudes up to plus or minus 60 deg have been performed to determine the recurrence period of the time series, interpreted as the synodic rotation period of the corona at a given latitude. Long-lived coronal structures have been shown to exist, with the following characteristics: (1) rigid rotation up to plus or minus 60 deg latitude, and (2) correlation with the large-scale solar magnetic pattern. These features develop essentially as longitudinally persistent phenomena, close to the boundaries of the solar magnetic sectors.

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