Correlation and spectral analysis of daily solar radio flux |
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Authors: | Mohamed El-Raey Phillip Scherrer |
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Institution: | 1. Space Sciences Laboratory, and Radio Astronomy Laboratory, University of California, Berkeley, Calif., U.S.A. 2. Institute of Plasma Research, Stanford University, Stanford, Calif., U.S.A.
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Abstract: | Correlation and spectral analysis of solar radio flux density and sunspot number near the maximum of the sunspot cycle has indicated the existence of - long period amplitude modulation of the slowly varying component (SVC) of radio emission
- coronal storage over a period of the order of three solar rotations
- fast decay (one solar rotation period or less) of gyromagnetic emissions from radio sources
- shift in location of chromospheric sources compared to those of either the upper corona or the photosphere.
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