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Results:
1-9
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Results: 9
Authors:
Kastner, SO
Bhatia, AK
Citation: So. Kastner et Ak. Bhatia, Optically thin and thick Fe xv spectrum: Effect of self-absorption on the 284.16 angstrom resonance line, ASTROPHYS J, 553(1), 2001, pp. 421-428
Authors:
Bhatia, AK
Kastner, SO
Citation: Ak. Bhatia et So. Kastner, Global and local Doppler-profile escape factors for plane-parallel geometry, J QUAN SPEC, 67(1), 2000, pp. 55-63
Authors:
Kastner, SO
Citation: So. Kastner, Rao coefficients for the solution of convolution integral equations, COMP PHYS C, 127(2-3), 2000, pp. 286-289
Authors:
Kastner, SO
Citation: So. Kastner, Re-analysis of published linewidths to obtain improved Voigt a-parameters and optical thicknesses in the inductively coupled plasma, SPECT ACT B, 54(11), 1999, pp. 1547-1555
Authors:
Kastner, SO
Citation: So. Kastner, An accuracy check for relative oscillator strengths using an intensity/linewidth method applied to precise data, PHYS LETT A, 254(5), 1999, pp. 279-286
Authors:
Kastner, SO
Citation: So. Kastner, Reliable resonance line opacity values by an intensity/linewidth method applied to precise data, PHYS SCR, 60(4), 1999, pp. 381-386
Authors:
Kastner, SO
Bhatia, AK
Citation: So. Kastner et Ak. Bhatia, A correction factor for Gaussian deconvolution of optically thick linewidths in homogeneous sources, M NOT R AST, 310(3), 1999, pp. 693-702
Authors:
Bhatia, AK
Kastner, SO
Citation: Ak. Bhatia et So. Kastner, The optically thick Fe XVII spectrum: X-ray, extreme-ultraviolet and forbidden line ratios, ASTROPHYS J, 516(1), 1999, pp. 482-489
Authors:
Kastner, SO
Citation: So. Kastner, Clarification and interpretation of the Friedjung-Muratorio self absorption curve method, ASTRON ASTR, 351(3), 1999, pp. 1016-1020
Risultati:
1-9
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