The interpretation of absorption-line shifts in the solar spectrum
Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV a...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Kostik, R. I. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| 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 42-51 |
|---|---|
| Übergeordnetes Werk: |
volume:26 ; year:1972 ; number:1 ; month:09 ; pages:42-51 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00155104 |
|---|
| Katalog-ID: |
OLC2033529134 |
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| 520 | |a Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. | ||
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| 650 | 4 | |a Homogeneous Medium | |
| 650 | 4 | |a Solar Disk | |
| 650 | 4 | |a Solar Spectrum | |
| 700 | 1 | |a Orlova, T. V. |4 aut | |
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10.1007/BF00155104 doi (DE-627)OLC2033529134 (DE-He213)BF00155104-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kostik, R. I. verfasserin aut The interpretation of absorption-line shifts in the solar spectrum 1972 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1972 Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. Chemical Element Sound Wave Homogeneous Medium Solar Disk Solar Spectrum Orlova, T. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 26(1972), 1 vom: Sept., Seite 42-51 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:26 year:1972 number:1 month:09 pages:42-51 https://doi.org/10.1007/BF00155104 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-PHA SSG-OLC-DE-84 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 42-51 |
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10.1007/BF00155104 doi (DE-627)OLC2033529134 (DE-He213)BF00155104-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kostik, R. I. verfasserin aut The interpretation of absorption-line shifts in the solar spectrum 1972 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1972 Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. Chemical Element Sound Wave Homogeneous Medium Solar Disk Solar Spectrum Orlova, T. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 26(1972), 1 vom: Sept., Seite 42-51 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:26 year:1972 number:1 month:09 pages:42-51 https://doi.org/10.1007/BF00155104 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-PHA SSG-OLC-DE-84 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 42-51 |
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10.1007/BF00155104 doi (DE-627)OLC2033529134 (DE-He213)BF00155104-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kostik, R. I. verfasserin aut The interpretation of absorption-line shifts in the solar spectrum 1972 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1972 Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. Chemical Element Sound Wave Homogeneous Medium Solar Disk Solar Spectrum Orlova, T. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 26(1972), 1 vom: Sept., Seite 42-51 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:26 year:1972 number:1 month:09 pages:42-51 https://doi.org/10.1007/BF00155104 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-PHA SSG-OLC-DE-84 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 42-51 |
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10.1007/BF00155104 doi (DE-627)OLC2033529134 (DE-He213)BF00155104-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kostik, R. I. verfasserin aut The interpretation of absorption-line shifts in the solar spectrum 1972 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1972 Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. Chemical Element Sound Wave Homogeneous Medium Solar Disk Solar Spectrum Orlova, T. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 26(1972), 1 vom: Sept., Seite 42-51 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:26 year:1972 number:1 month:09 pages:42-51 https://doi.org/10.1007/BF00155104 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-PHA SSG-OLC-DE-84 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 42-51 |
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10.1007/BF00155104 doi (DE-627)OLC2033529134 (DE-He213)BF00155104-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kostik, R. I. verfasserin aut The interpretation of absorption-line shifts in the solar spectrum 1972 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1972 Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. Chemical Element Sound Wave Homogeneous Medium Solar Disk Solar Spectrum Orlova, T. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 26(1972), 1 vom: Sept., Seite 42-51 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:26 year:1972 number:1 month:09 pages:42-51 https://doi.org/10.1007/BF00155104 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OLC-PHA SSG-OLC-DE-84 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 42-51 |
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the interpretation of absorption-line shifts in the solar spectrum |
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The interpretation of absorption-line shifts in the solar spectrum |
| abstract |
Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. © D. Reidel Publishing Company 1972 |
| abstractGer |
Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. © D. Reidel Publishing Company 1972 |
| abstract_unstemmed |
Abstract The shifts of Fraunhofer lines of different chemical elements in a homogeneous medium with a plane monochromatic progressive adiabatic sound waves are derived. The calculations indicate that lines of neutral elements (6 ⩽ $ χ_{0} $ ⩽ 14) with lower excitation potentials $ χ_{0} $i= 0–2 eV are red shifted, those with excitation potential $ χ_{0} $i= 4–12 eV are blue shifted, and with $ χ_{0} $i= 3 eV are both blue and red shifted. The lines of ions are shifted toward the blue. The shifts of Fraunhofer lines are found to decrease from the centre of the solar disk to the limb. These results agree qualitatively and quantitatively with observations. © D. Reidel Publishing Company 1972 |
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The interpretation of absorption-line shifts in the solar spectrum |
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