Chandra, Suresh (1982) Intensity of lines from low-lying levels in C ii, N iii, O iv, Ne vi, Mg viii, Si x, and Si ii. Solar Physics, 75 (1). 133-137 doi:10.1007/bf00153466

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Reference Type	Journal (article/letter/editorial)
Title	Intensity of lines from low-lying levels in C ii, N iii, O iv, Ne vi, Mg viii, Si x, and Si ii
Journal	Solar Physics
Authors	Chandra, Suresh		Author
Year	1982 (January)	Volume	75
Issue	1
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/bf00153466Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	8917152	Long-form Identifier	mindat:1:5:8917152:9
GUID	0
Full Reference	Chandra, Suresh (1982) Intensity of lines from low-lying levels in C ii, N iii, O iv, Ne vi, Mg viii, Si x, and Si ii. Solar Physics, 75 (1). 133-137 doi:10.1007/bf00153466
Plain Text	Chandra, Suresh (1982) Intensity of lines from low-lying levels in C ii, N iii, O iv, Ne vi, Mg viii, Si x, and Si ii. Solar Physics, 75 (1). 133-137 doi:10.1007/bf00153466
In	(1982, January) Solar Physics Vol. 75 (1) Springer Science and Business Media LLC

	Nahar, Sultana N. (1995) Electron-Ion Recombination Rate Coefficients for SI i, SI ii, S ii, S iii, C ii, and C-like Ions C i, N ii, O iii, F iv, NE v, NA vi, MG vii, AL viii, SI ix, and S XI. The Astrophysical Journal Supplement Series, 101. 423 doi:10.1086/192248
	Nahar, Sultana N. (1996) Electron-Ion Recombination Rate Coefficients for SI i, SI ii, S ii, S iii, C ii, and C-like Ions C i, N ii, O iii, F iv, NE v, NA vi, MG vii, AL viii, SI ix, and S xi: Erratum. The Astrophysical Journal Supplement Series, 106. 213 doi:10.1086/192336
	*Dwivedi, B. N., Mohan, Anita (1995) Diagnostics of solar ions: Ne VI, Mg VI, Si VIII and Mg VIII observed by SERTS. Solar Physics, 156 (1). 81-94 doi:10.1007/bf00669577*
	Heroux, L., Cohen, M., Malinovsky, Monique (1972) The interpretation of XUV rocket measurements of intensity ratios of solar spectral lines of the lithiumlike ions O vi, Ne viii, and Mg x. Solar Physics, 23 (2). 369-393 doi:10.1007/bf00148101
	*Chandra, Suresh (1978) Excitation equilibrium for low lying levels in Cii, Niii, Oiv, Nevi, Mgviii, Six, and Siii. Solar Physics, 58 (2). 291-297 doi:10.1007/bf00157274*
	Simon, T., Kelch, W. L., Linsky, J. L. (1980) Outer atmospheres of cool stars. VI - Models for Epsilon Eridani based on IUE spectra of C II, MG II, SI II, and SI III. The Astrophysical Journal, 237. 72pp. doi:10.1086/157845
	Westhaus, Paul, Sinanoglu, Oktay (1969) Nontransferable Correlation Effects and Multiplet Oscillator Strengths for Electric Dipole Transitions in Atoms with Results on C ii, N i, N ii, N III, O ii, O III, O iv, F ii, and NE II. The Astrophysical Journal, 157. 997pp. doi:10.1086/150130
	*Münch, G., Neugebauer, G., McCammon, D. (1967) Infrared Coronal Lines. II. Observation of [SI x] λ 1.43 μ and [Mg VIII] λ 3.03μ. The Astrophysical Journal, 149. 681pp. doi:10.1086/149297*
	*Dwivedi, B. N. (1991) Forbidden line ratios from Si viii and S x coronal ions. Solar Physics, 131 (1). 49-52 doi:10.1007/bf00151743*
	Ayres, Thomas, De Pontieu, Bart, Testa, Paola (2021) In the Trenches of the Solar-stellar Connection. IV. Solar Full-disk Scans of C ii, Si iv, and Mg ii by the Interface Region Imaging Spectrograph. The Astrophysical Journal, 916 (1) 36pp. doi:10.3847/1538-4357/abfa92
	*Roussel-Dupr�, D., Shine, R. A. (1982) Evidence of redshifts in the average solar line profiles of C iv and Si iv from OSO-8 observations. Solar Physics, 77 (1). 329-340 doi:10.1007/bf00156115*

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Chandra, Suresh (1982) Intensity of lines from low-lying levels in C ii, N iii, O iv, Ne vi, Mg viii, Si x, and Si ii. Solar Physics, 75 (1). 133-137 doi:10.1007/bf00153466

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