Mathematics
Scientific paper
Dec 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aifo.reptq.....&link_type=abstract
M.S. Thesis Air Force Inst. of Tech., Wright-Patterson AFB, OH. School of Engineering.
Mathematics
Mathematical Models, Radio Emission, Regression Analysis, Solar Activity, Statistical Correlation, Histograms, Prediction Analysis Techniques, Solar Flux
Scientific paper
Using a statistical regression model, a relationship was found between the area of solar active regions (bright in hydrogen-alpha. Lambda = 6562.8 A in the visible) and their 10.7 cm radio emission. Data used in this analysis were the brightness-area histograms obtained from the Solar Observing Optical Network (SOON) and daily drift scans obtained from the Algonguin Radio Observatory, Ottawa, Canada. This data, for the period 1 May through 16 July 1978, was used to develop the following relationship: Algonguin Scan Peak Value = .88782838 + .00025237604 (Calibrated SOON Area) with a correlation coefficient, r, of .88509. Future models for perdicting the 10.7 cm solar flux are theorized based on the established relationship.
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