✍ Scribed by Z. Švestka
No coin nor oath required. For personal study only.
Three problems are emphasized in particular: the preflare magnetic field configuration, velocity fields, and the nature of acceleration processes in flares. It is concluded that what we need most urgently are high-resolution hard X-ray, soft X-ray, and EUV-pictures, coronal spectra, and magnetograms with high resolution both in space and time. A space-shuttle equipped with instrumentation of this kind would contribute significantly to our knowledge of the flare process.
The ATM observations during the Skylab mission brought a lot of new information about the flares, and about the pre-flare situations in the Solar corona. But these new observations also raised new problems and some of them are of crucial importance for our understanding of the flare build-up process. * TP abbreviates "paper in these Proceedings".
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