Calculation of 5250.216 Å line profiles in sunspots
Abstract The assumptions of pure absorption and local thermodynamic equilibrium are sometimes used to calculate approximate spectral line profiles in cases where a rigorous treatment is impractical or impossible. In certain conditions, the profile is not completely defined under these assumptions.
Autor*in: |
Dunn, A. R. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
1972 |
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Schlagwörter: |
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Anmerkung: |
© D. Reidel Publishing Company 1972 |
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Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 26(1972), 1 vom: Sept., Seite 83-86 |
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Übergeordnetes Werk: |
volume:26 ; year:1972 ; number:1 ; month:09 ; pages:83-86 |
Links: |
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DOI / URN: |
10.1007/BF00155107 |
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Katalog-ID: |
OLC203352910X |
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10.1007/BF00155107 doi (DE-627)OLC203352910X (DE-He213)BF00155107-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Dunn, A. R. verfasserin aut Calculation of 5250.216 Å line profiles in sunspots 1972 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1972 Abstract The assumptions of pure absorption and local thermodynamic equilibrium are sometimes used to calculate approximate spectral line profiles in cases where a rigorous treatment is impractical or impossible. In certain conditions, the profile is not completely defined under these assumptions. Spectral Line Thermodynamic Equilibrium Line Profile Local Thermodynamic Equilibrium Rigorous Treatment Enthalten in Solar physics Kluwer Academic Publishers, 1967 26(1972), 1 vom: Sept., Seite 83-86 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:26 year:1972 number:1 month:09 pages:83-86 https://doi.org/10.1007/BF00155107 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4305 GBV_ILN_4306 AR 26 1972 1 09 83-86 |
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10.1007/BF00155107 doi (DE-627)OLC203352910X (DE-He213)BF00155107-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Dunn, A. R. verfasserin aut Calculation of 5250.216 Å line profiles in sunspots 1972 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1972 Abstract The assumptions of pure absorption and local thermodynamic equilibrium are sometimes used to calculate approximate spectral line profiles in cases where a rigorous treatment is impractical or impossible. In certain conditions, the profile is not completely defined under these assumptions. Spectral Line Thermodynamic Equilibrium Line Profile Local Thermodynamic Equilibrium Rigorous Treatment Enthalten in Solar physics Kluwer Academic Publishers, 1967 26(1972), 1 vom: Sept., Seite 83-86 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:26 year:1972 number:1 month:09 pages:83-86 https://doi.org/10.1007/BF00155107 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4305 GBV_ILN_4306 AR 26 1972 1 09 83-86 |
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Abstract The assumptions of pure absorption and local thermodynamic equilibrium are sometimes used to calculate approximate spectral line profiles in cases where a rigorous treatment is impractical or impossible. In certain conditions, the profile is not completely defined under these assumptions. © D. Reidel Publishing Company 1972 |
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Abstract The assumptions of pure absorption and local thermodynamic equilibrium are sometimes used to calculate approximate spectral line profiles in cases where a rigorous treatment is impractical or impossible. In certain conditions, the profile is not completely defined under these assumptions. © D. Reidel Publishing Company 1972 |
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Abstract The assumptions of pure absorption and local thermodynamic equilibrium are sometimes used to calculate approximate spectral line profiles in cases where a rigorous treatment is impractical or impossible. In certain conditions, the profile is not completely defined under these assumptions. © D. Reidel Publishing Company 1972 |
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R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Calculation of 5250.216 Å line profiles in sunspots</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1972</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© D. 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