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III. Active Regions

  • R. Falciani
Extract

During the past three years arguments related to the AR physics can be found in the proceedings of the following meetings: Chromospheric Diagnostics and Modelling, NSO Sacramento Peak, 1984 (I); The Hydromagnetics of the Sun, Noordwijkerout, ESA, 1984 (II); Solar and Stellar Physics, Titisee, 1987 (III). Many aspects concerning the high activity levels of AR’s can also be found in the proceedings of large number of meetings organized on solar flares. Microwave mapping is reported in Section VII. Some results are also reported in Section II.

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References
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I: Chromospheric Diagnostic and Modelling, NSO, Sacramento-Peak, Lites, (ed), 1984.
II: The Hydrodynamics of the Sun, Noordwijkerout, ESA, SP 220, 1984.
III: Solar and Stellar Physics, Titisee, 1987.
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0251-107X
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