Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-12T12:48:56.806Z Has data issue: false hasContentIssue false
  • English
  • Français

Results From Optical and UV Stellar Flare Spectroscopy

Published online by Cambridge University Press:  12 April 2016

Mark S. Giampapa
Mark S. Giampapa*
Affiliation:
Harvard-Smithsonian Center for Astrophysics

Abstract

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.

Optical and ultraviolet spectroscopy can enable the assessment of the physical conditions characterizing a stellar flare atmosphere and thereby potentially elucidate the possible radiative and hydrodynamic transport mechanisms operative during stellar flares. In this review, I present illustrative examples of the spectroscopic diagnostic techniques that can be applied to the analysis of stellar flare spectroscopic data and the resulting inferences concerning stellar flare properties for M dwarf flare events.

Type
Session II: Observed Activity in Red-Dwarfs
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 223 - 235
Copyright
Copyright © Reidel 1983

References

REFERENCES

Baliunas, S. and Raymond, J. 1982, private communication.Google Scholar
Bromage, G. et al. 1982, in preparation.Google Scholar
Butler, C.J., Byrne, P.B., Andrews, A.D. and Doyle, J.G. 1981, MNRAS 197, 815.Google Scholar
Canfield, R.C. et al. 1980, in Solar Flares, ed. Sturrock, P.A. (Boulder: Colorado Associated University Press), p. 451.Google Scholar
Drake, S.A. and Ulrich, R.K. 1980, Ap.J.Suppl., 42, 351.Google Scholar
Giampapa, M.S., 1980, Ph.D. dissertation, University of Arizona, Tucson.Google Scholar
Giampapa, M.S., Linsky, J.L., Schneeberger, T.J. and Worden, S.P. 1978, Ap.J. 226, 144.CrossRefGoogle Scholar
Giampapa, M.S., Worden, S.P. and Linsky, J.L. 1982, Ap.J. 258, 740.Google Scholar
Giampapa, M.S. et al. 1982, in preparation.Google Scholar
Grinin, V.P. 1976, Izv. Krim. Astrofiz. Obs., 60, 179.Google Scholar
Haisch, B.M. et al. 1982, Ap.J. submitted.Google Scholar
Kahler, S. et al. 1982, Ap.J., 252, 239.Google Scholar
Kunkel, W.E. 1970, Ap.J., 161, 503.CrossRefGoogle Scholar
Kurochka, L.N. and Maslennikova, L.B. 1970, Solar Phys., 11, 33.Google Scholar
Kurochka, L.N. and Sitnik, G.F. 1976, Sov. Astron., 19, 590.Google Scholar
Linsky, J.L. et al. 1982, Ap.J., in press.Google Scholar
Machado, M.E. and Linsky, J.L. 1975, Solar Phys., 42, 395.CrossRefGoogle Scholar
Mochnacki, S.W. and Schommer, R.A. 1979, Ap.J. (Letters) 231, L77.Google Scholar
Mochnacki, S.W. and Zirin, H., 1980, Ap.J.(Letters), 239, L27.Google Scholar
Moffett, T.J. and Bopp, B.W. 1976, Ap.J.Suppl. 31, 61.Google Scholar
Moore, R. et al. 1980, in Solar Flares, ed. Sturrock, P. (Boulder: Colorado Associated University Press), p. 341.Google Scholar
Mullan, D.J. 1976, Ap.J., 207, 289.CrossRefGoogle Scholar
Neidig, D.F. 1982, Solar Phys., 78, 225.Google Scholar
Raymer, M. 1979, Ph.D. thesis, University of Colorado, Boulder.Google Scholar
Raymond, J.C., Cox, D.P. and Smith, B.W. 1976, Ap.J., 204, 290.Google Scholar
Robbins, R.R. 1968, Ap.J., 151, 511.CrossRefGoogle Scholar
Schneeberger, T.J., Linsky, J.L., McClintock, W. and Worden, S.P. 1979, Ap.J., 231, 148.CrossRefGoogle Scholar
Sutton, K. 1978, J.Q.S.R.T., 20, 333.Google Scholar
Svestka, Z. 1966, Bull. Astron. Inst. Czech., 17, 137.Google Scholar
Tandberg-Hanssen, E. 1974, Solar Prominences (Boston: Reidel), pp. 70–73.Google Scholar
Wagner, W.J. et al. 1981, Ap.J.(Letters), 244, L123.Google Scholar
Worden, S.P., Schneeberger, T.J. and Giampapa, M.S. 1981, Ap.J.Suppl. 46, 159.Google Scholar