Abstract
A review is given of the activities of the working group on small scale features at the 2nd SORO Workshop on Elba, 27 September-1 October 1993. The small scale and filamentary structure of the solar transition region, and possibly also the corona, was pointed out. The reported observations furthermore demonstrated that the upper solar atmosphere is strongly dynamical, containing rapidly flowing gas and with features changing with time. Theoretical concepts and simulations of conditions in the transition region and corona were presented and discussed. Finally some ideas on future observations and modelling were put forward.
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Hansteen, V. and Wikstøl Ø.: 1994, Astronomy and Astrophysics, accepted.
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© 1994 Springer Science+Business Media Dordrecht
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Kjeldseth-Moe, O. (1994). Working Group 1: Small Scale Features. In: Fleck, B., Noci, G., Poletto, G. (eds) Mass Supply and Flows in the Solar Corona. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0930-7_23
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DOI: https://doi.org/10.1007/978-94-011-0930-7_23
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4401-1
Online ISBN: 978-94-011-0930-7
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