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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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Reference TypeJournal (article/letter/editorial)
TitleDiagnostic application of highly ionized iron lines in the XUV spectrum of a solar flare
JournalSolar Physics
AuthorsMason, H. E.Author
Bhatia, A. K.Author
Kastner, S. O.Author
Neupert, W. M.Author
Swartz, M.Author
Year1984 (May)Volume92
Issue1
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/bf00157246Search in ResearchGate
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Mindat Ref. ID8917787Long-form Identifiermindat:1:5:8917787:9
GUID0
Full ReferenceMason, 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 TextMason, 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

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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 Ã…. 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 Ã…. 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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