Correlated brightness variations in solar radiative output from the photosphere to the corona

Details Correlated brightness variations in solar radiative output from the photosphere to the corona Correlated brightness variations in solar radiative output from the photosphere to the corona

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995georl..22..655l&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 22, no. 5, p. 655-658

Physics

6

Brightness, Photosphere, Solar Corona, Solar Magnetic Field, Solar Spectra, Solar X-Rays, Correlation, Solar Temperature, Spectrum Analysis, Sunspots, Variations

Scientific paper

Correlated brightness variations are shown to occur in time series of coronal soft X-rays exclusive of prominent active regions, chromospheric ultraviolet radiation, and the photospheric total solar irradiance corrected for sunspot effects. These temporal correlations suggest that upwardly extending magnetic fields may have a large scale impact on the solar atmosphere in addition to their demonstrable role of generating localized active regions. The correlations have implications for improving and extending solar spectrum variability models.

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