Titlebook: Solar Magnetic Phenomena; Proceedings of the 3 Arnold Hanslmeier,Astrid Veronig,Mauro Messerotti Conference proceedings 2005 Springer Scien

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On the 24- and 155-Day Periodicity Observed in Solar H, Flares “activity”periods (∼150.–160.). We focus on the separate analysis of the northern and southern solar hemisphere as well as on an energy dependence of the flare events. Our findings suggest that the appearance of the “activity” periods might result due to superposition of two predominant periods of

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He-D3 Polarization Observed in Prominences Locarno. Two different experimental techniques (ZIMPOL and beam exchange method) have been successfully employed to determine all four Stokes components. Both give compatible results. The preliminary results as well as the measurement techniques are reported.

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Solar Flares — Observations and Theory instabilities and particle acceleration process — are described as an indivisible part of the reconnection process. Finally, the interacting-flux flares and two-ribbon flares are used to illustrate some details of flare modeling.

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Physics of Solar Prominences transfer equations are described in some detail. Finally, new models resulting from a combination of magneto-hydrostatics and radiative transfer are outlined and their relevance for observations is discussed.

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Arnold Hanslmeier,Astrid Veronig,Mauro MesserottiIs particularly useful for graduate students and young researchers working in solar physics

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