Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-30T12:42:53.708Z Has data issue: false hasContentIssue false
  • English
  • Français

Diagnostics of EUV Spectral Emission from Boron-like Ions

Published online by Cambridge University Press:  12 April 2016

Jianfang Peng  and
Anil K. Pradhan
Jianfang Peng
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA
Anil K. Pradhan
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA

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.

Recent developments of EUV diagnostics from transitions in Boron-like ions, C II, N III, O IV, Ne VI, Mg VIII, Al IX, Si X, and S XII, are discussed based on new atomic data (Zhang, Graziani & Pradhan (1994)) and systematic theoretical calculations of line intensity ratios (Peng & Pradhan 1995). The available EUV and UV lines which are good temperature and density diagnostics are summarized. Possible applications of these lines to the investigation of the physical conditions in astrophysical objects are proposed.

Type
XIII. Plasma Diagnostics
Information
International Astronomical Union Colloquium , Volume 152: Astrophysics in the Extreme Ultraviolet , 1996 , pp. 589 - 593
Copyright
Copyright © Kluwer 1996

References

Blum, R.D., & Pradhan, A.K. 1992, ApJS, 80, 425 CrossRefGoogle Scholar
Dankworth, W. & Trefftz, E. 1978, A&A, 65, 93 Google Scholar
Hayes, M.A. & Nussbaumer, 1984, A&A, 134, 193 Google Scholar
Hayes, M.A. & Nussbaumer, 1983, A&A, 124, 279 Google Scholar
Hayes, M.A. 1992, J. Phys. B, 25, 2649 Google Scholar
Hummer, D.G., Berrington, K.A., Eissner, W., Pradhan, A.K., Saraph, H.E. & Tully, J.A. 1993, A&A, 279, 298 Google Scholar
Luo, D. & Pradhan, A.K. 1990, Phys. Rev. A, 41, 165 CrossRefGoogle Scholar
Lennon, D.J., Dufton, P.L., Hibbert, A., Kingston, A.E. 1985, ApJ, 294, 200 CrossRefGoogle Scholar
Keenan, F.P., Conlon, E.S., Bowden, D.A., Dwivedi, B.N. & Widing, 1994a, Solar Phys., 149, 137 CrossRefGoogle Scholar
Keenan, F.P., Warren, G.A., Doyle, J.G., Berrington, K.A., Kingston, A.E. 1994b, Solar Phys., 150, 61 Google Scholar
Keenan, F.P., Foster, V.J., Reid, R.H.G., Doyle, J.G., Zhang, H.L. & Pradhan, A.K. 1994, private communicationGoogle Scholar
Merkelis, G., Vilkas, M.J., Gaigalas, G. & Kisieulros, R. 1994, Physica Scripta, submittedGoogle Scholar
O’shea, E., Foster, V.J., Keenan, F.P., Doyle, J.G., Reid, R.H.G., Zhang, H.L., & Pradhan, A.K. 1995, A&AS, submittedGoogle Scholar
Peng, J.F. & Pradhan, A.K. 1995, A&AS, submittedGoogle Scholar
Peng, J.F. & Pradhan, A.K. 1994, ApJ, 432, L123 Google Scholar
Zhang, H.L., Graziani, M. & Pradhan, A.K. 1994, A&A, 283, 319 Google Scholar
Stafford, R.P., Hibbert, A., & Bell, K.L. 1993, MNRAS, 260, L11 CrossRefGoogle Scholar