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Titlebook: Solar and Stellar Flares; Proceedings of the 1 Bernhard M. Haisch,Marcello Rodonò Conference proceedings 1989 Kluwer Academic Publishers 19

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Models of Flaring Loops,for energy transport within the loop structure. Observational evidence suggests a predominant role for high-energy electrons as an energy transport mechanism, and we explore the consequences of such a scenario in some detail, focusing on radiation signatures in the soft X-ray, hard X-ray, and EUV wa
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Stellar Flare Spectral Diagnotics: Present and Future, atmospheric response, mass motions, microflaring, statistics and recurrence of flares, flare activity and stellar interior. We review some of these diagnostics (from photometry, optical, and ultraviolet spectroscopy at medium- and high-spectral resolution, X-ray, and radio observations). Specific d
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Simultaneous Multi-Frequency Imaging Observations of Solar Microwave Bursts,observations have been made of bursts which are optically thin at both frequencies, or optically thick at the lower frequency. In the latter case the source structure may differ at the two frequencies, but the two sources usually seem to be related. However, this is not always true of simultaneous 6
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Radio Emission from Stellar Flares,releases of magnetic energy. The main sources of such flares are late-type Main-Sequence stars, classic close binaries, X-ray binaries, and pre-Main-Sequence stars..We summarize the interpretations of these observations in terms of the various incoherent and coherent emission mechanisms. The possibl
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Mass Motions Associated with Solar Flares,chromospheric flare ribbons, remote chromospheric flare patches, flare loops, flaring arches, surges, erupting filaments and some expanding coronal features. Interrelationships between these phenomena are discussed and illustrations of each are presented.
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