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Titlebook: Coronal Magnetic Energy Releases; Proceedings of the C Arnold O. Benz,Albrecht Krüger Conference proceedings 1995 Springer-Verlag Berlin He

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Initial results from the Nobeyama Radiobeliograph,observations, which contain a last part of the maximum phase of the solar cycle 22, it was possible to obtain almost every aspect of solar activity at 17 GHz. They include two X-class flares, tens of M-class flares, hundreds of flares from the very initial phase through the late decay phase, or from
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Non-linear data analysis and statistical techniques in solar radio astronomy, from turbulence theory is an appropriate method to find out some scaling behavior of fluctuations in time. More generally, the wavelet analysis, which is some generalization of the power spectrum, exhibits information on the location as well as the size of hidden characteristic features. Applying b
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