On possible correlations in the photospheric magnetic field

Details On possible correlations in the photospheric magnetic field On possible correlations in the photospheric magnetic field

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...83..191w&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 83, March 1983, p. 191-194.

Physics

Data Correlation, Northern Hemisphere, Photosphere, Solar Magnetic Field, Southern Hemisphere, Atmospheric Turbulence, Convective Flow, Correlation Coefficients, Data Reduction, Dynamo Theory, Magnetic Measurement, Turbulence Effects

Scientific paper

A correlation analysis is performed upon the rate of change of the photospheric magnetic field in the north and south hemispheres of the sun. Both active region logs and data obtained from the daily Mount Wilson magnetograms are employed, and the analysis is performed for all available days, as well as for days in which active regions are near central meridian. The result of the analysis shows no correlation between these changes and it is concluded that local convective turbulence is more important than dynamo processes with regard to the appearance of individual active regions.

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