Hostname: page-component-77c89778f8-rkxrd Total loading time: 0 Render date: 2024-07-23T00:33:40.410Z Has data issue: false hasContentIssue false
  • English
  • Français

MHD Aspects of Coronal Transients

Published online by Cambridge University Press:  14 August 2015

U. Anzer
U. Anzer*
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Munich

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

If one defines coronal transients as events which occur in the solar corona on rapid time scales (≲ several hours) then one would have to include a large variety of solar phenomena: flares, sprays, erupting prominences, X-ray transients, white light transients, etc. Here we shall focus our attention on the latter two phenomena; solar flares have been discussed at great length in a recent Skylab workshop and IAU Colloqium No. 44 was devoted to the study of prominences. Coronal transients, in the narrower sense, were first seen with the instruments on board of Skylab, both in the optical and the X-ray part of the spectrum.

Type
Part IV. Solar Transient Phenomena Affecting the Corona and Interplanetary Medium: - Theoretical Considerations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 263 - 277
Copyright
Copyright © Reidel 1980 

References

Anzer, U.: 1978, Solar Phys. 57, pp 111–118 Google Scholar
Dryer, M., Wu, S.T., Steinolfson, R.S., Wilson, R.M.: 1979, Astrophys. J. 227, pp. 10059–1071CrossRefGoogle Scholar
Dulk, G.A., McLean, D.J.: 1978, Solar Phys. 57, pp. 279–295 CrossRefGoogle Scholar
Dulk, G.A., Smerd, S.F., MacQueen, R.M., Gosling, J.T., Magun, A., Stewart, R.T., Sheridan, K.V., Robinson, R.D., Jaques, S.: 1976, Solar Phys. 49, pp. 369–394 Google Scholar
Gergely, T., Kundu, M., Poland, A.I., Munro, R.H.: 1979, Astrophys. J. (submitted) Google Scholar
Gosling, J.T., Hildner, E., MacQueen, R.M., Munro, R.H., Poland, A.I., Ross, C.L.: 1974, J. Geophys. Res. 79, pp. 4581–4587 Google Scholar
Hildner, E.: 1977, L.D. de Feiter Memorial STIP Syposium (Tel Aviv) Google Scholar
Mouschovias, T.Ch., Poland, A.I.: 1978, Astrophys. J. 220, pp. 675–682 CrossRefGoogle Scholar
Nakagawa, Y., Wu, S.T., Tandberg-Hanssen, E.: 1975, Solar Phys. 41, pp. 387–396 Google Scholar
Pneuman, G.W.: 1978, IAU Colloquium No. 44, Physics of Solar Prominences (Jensen, E., Maltby, P., Orrall, F.Q., Eds.), pp. 281–301 Google Scholar
Pneuman, G.W.: 1979, Preprint MPI-PAE/Astro 170, to appear in Solar Phys.Google Scholar
Rust, D.M., Hildner, E.: 1976, Solar Phys. 48, pp. 381–387 Google Scholar
Rust, D.M., Webb, D.F.: 1977, Solar Phys. 54, pp. 403–417 CrossRefGoogle Scholar
Steinolfson, R.S., Nakagawa, Y.: 1976, Astrophys. J., 207, pp. 300–307 CrossRefGoogle Scholar
Steinolfson, R.S., Wu, S.T., Dryer, M., Tandberg-Hanssen, E.: 1978, Astrophys. J. 225, pp. 259–274 CrossRefGoogle Scholar
Van Tend, W.: 1979, Solar Phys. 61, pp. 89–93 Google Scholar
Webb, D.F., Krieger, A.S., Rust, D.M.: 1976, Solar Phys. 48, pp. 159–186 Google Scholar
Wu, S. T., Dryer, M., Nakagawa, Y., and Han, S. M.: 1978, Astrophys. J. 219, pp. 324–335.Google Scholar