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On the Fluctuations in the Solar Flux at cm-Wavelengths Monitored on Small Areas of the Sun's Disk

Published online by Cambridge University Press:  14 August 2015

W. Hirth
W. Hirth*
Affiliation:
Radioastronomisches Institut der Universität Bonn, Auf dem Hügel 71, 53 Bonn, Germany

Abstract

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We discuss the relatively broad spectrum of fluctuations in flux which is observed at cm-wavelengths when tracking a small area on the Sun's disk. The distribution of power P over the frequencies ω of fluctuations can be approximated by a power-law where α ≃ 2; often a continuous “curvature” is superimposed and a “turnover” frequency is indicated at about ω/2π ≃ 10−3 Hz. Considering the phases of different Fourier components of the time series measured, a significant linear correlation is found between phases of neighbouring frequencies.

Type
Session I - Quiet Sun
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 65 - 68
Copyright
Copyright © Reidel 1980 

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