Mason, H. E., Bhatia, A. K., Kastner, S. O., Neupert, W. M., Swartz, M. (1984) Diagnostic application of highly ionized iron lines in the XUV spectrum of a solar flare. Solar Physics, 92 (1). 199-216 doi:10.1007/bf00157246

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Reference Type	Journal (article/letter/editorial)
Title	Diagnostic application of highly ionized iron lines in the XUV spectrum of a solar flare
Journal	Solar Physics
Authors	Mason, H. E.		Author
	Bhatia, A. K.		Author
	Kastner, S. O.		Author
	Neupert, W. M.		Author
	Swartz, M.		Author
Year	1984 (May)	Volume	92
Issue	1
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/bf00157246Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	8917787	Long-form Identifier	mindat:1:5:8917787:9
GUID	0
Full Reference	Mason, H. E., Bhatia, A. K., Kastner, S. O., Neupert, W. M., Swartz, M. (1984) Diagnostic application of highly ionized iron lines in the XUV spectrum of a solar flare. Solar Physics, 92 (1). 199-216 doi:10.1007/bf00157246
Plain Text	Mason, H. E., Bhatia, A. K., Kastner, S. O., Neupert, W. M., Swartz, M. (1984) Diagnostic application of highly ionized iron lines in the XUV spectrum of a solar flare. Solar Physics, 92 (1). 199-216 doi:10.1007/bf00157246
In	(1984, May) Solar Physics Vol. 92 (1) Springer Science and Business Media LLC

	Kastner, S. O., Neupert, W. M., Swartz, M. (1974) Solar-flare emission lines in the range from 66 to 171 A; transitions in highly ionized iron. The Astrophysical Journal, 191. 261pp. doi:10.1086/152963
	*Kastner, S. O., Neupert, W. M., Swartz, M. (1974) On helium-like 1s2l?1snl? transitions in solar flare spectra. Solar Physics, 36 (1). 121-128 doi:10.1007/bf00151552*
	*Neupert, W. M., Swartz, M. (1970) Resonance and Satellite Lines of Highly Ionized Iron in the Solar Spectrum Near 1.9 Å. The Astrophysical Journal, 160. doi:10.1086/180557*
	*Neupert, W.M., Swartz, M., Kastner, S.O. (1973) Solar flare line emission between 6 � and 25 �. Solar Physics, 31 (1). doi:10.1007/bf00156081*
	Kastner, S. O., Neupert, W. M., Swartz, M. (1975) Observation of possible Fe xvii 2p 53p(1S0)-2p 53s(1 P 1, 3 P 1) transitions in spectra of a solar active region and flare. Solar Physics, 43 (1). 111-115 doi:10.1007/bf00155148
	*Podgorny, I. M., Podgorny, A. I. (2018) Diagnostic of a Solar Flare via Analyses of Emission in Spectral Lines of Highly Ionized Iron. Astronomy Reports, 62. 696-704 doi:10.1134/s1063772918100074*
	*Bhatia, A. K., Kastner, S. O., Behring, W. E. (1982) The solar O III spectrum. I - Photoexcitation of EUV lines by He II Lyman-alpha. The Astrophysical Journal, 257. 887pp. doi:10.1086/160038*
	*Neupert, W. M., Gates, W., Swartz, M., Young, R. (1967) Observation of the Solar Flare X-Ray Emission-Line Spectrum of Iron from 1.3 to 20 Å. The Astrophysical Journal, 149. doi:10.1086/180061*
	Lippmann, S., Finkenthal, M., Huang, L. K., Moos, H. W., Stratton, B. C., Yu, T. L., Bhatia, A. K. (1987) Laboratory study of the spectrum of highly ionized calcium in the 100-250 A range applied to solar flare diagnostics. The Astrophysical Journal, 316. 819pp. doi:10.1086/165245
	*Neupert, Werner M. (1971) Satellite lines in the solar X-ray spectrum. Solar Physics, 18 (3). 474-488 doi:10.1007/bf00149069*
	*Kastner, S. O., Bhatia, A. K. (1984) On Bowen enhancement of the N III spectrum under solar and nebular conditions. The Astrophysical Journal, 287. 945pp. doi:10.1086/162751*

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Mason, H. E., Bhatia, A. K., Kastner, S. O., Neupert, W. M., Swartz, M. (1984) Diagnostic application of highly ionized iron lines in the XUV spectrum of a solar flare. Solar Physics, 92 (1). 199-216 doi:10.1007/bf00157246

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