Using Solar-Minimum Polar Coronal Activity to Predict the Magnitude of the Following- Cycle Maximum

Details Using Solar-Minimum Polar Coronal Activity to Predict the Magnitude of the Following- Cycle Maximum Using Solar-Minimum Polar Coronal Activity to Predict the Magnitude of the Following- Cycle Maximum

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh21a0323a&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SH21A-0323

Physics

7509 Corona, 7536 Solar Activity Cycle (2162)

Scientific paper

Observations of the Fe XIV solar corona have been obtained for the past three solar activity cycles at the Sacramento Peak site of the National Solar Observatory with the 40-cm coronagraph and the photoelectric coronal photometer. This study compares the properties of these observations near the poles near solar minimum with the maximum sunspot number of the following solar cycle. Preliminary results indicate that the number of coronal bright regions near the poles near solar minimum may be inversely correlated with the maximum amplitude of the following solar cycle. Using these results from previous cycles, a prediction will be made of the maximum sunspot number for cycle 24.

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