On the instrumental and atmospheric stray-light for solar observations
Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrument...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Mattig, W. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1983 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Co 1983 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 87(1983), 1 vom: Aug., Seite 187-193 |
|---|---|
| Übergeordnetes Werk: |
volume:87 ; year:1983 ; number:1 ; month:08 ; pages:187-193 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00151169 |
|---|
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OLC203355421X |
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| 520 | |a Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. | ||
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10.1007/BF00151169 doi (DE-627)OLC203355421X (DE-He213)BF00151169-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mattig, W. verfasserin aut On the instrumental and atmospheric stray-light for solar observations 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1983 Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. Good Condition Wavelength Region Solar Disk Solar Radius Atmospheric Component Enthalten in Solar physics Kluwer Academic Publishers, 1967 87(1983), 1 vom: Aug., Seite 187-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:87 year:1983 number:1 month:08 pages:187-193 https://doi.org/10.1007/BF00151169 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4305 GBV_ILN_4306 AR 87 1983 1 08 187-193 |
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10.1007/BF00151169 doi (DE-627)OLC203355421X (DE-He213)BF00151169-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mattig, W. verfasserin aut On the instrumental and atmospheric stray-light for solar observations 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1983 Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. Good Condition Wavelength Region Solar Disk Solar Radius Atmospheric Component Enthalten in Solar physics Kluwer Academic Publishers, 1967 87(1983), 1 vom: Aug., Seite 187-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:87 year:1983 number:1 month:08 pages:187-193 https://doi.org/10.1007/BF00151169 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4305 GBV_ILN_4306 AR 87 1983 1 08 187-193 |
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10.1007/BF00151169 doi (DE-627)OLC203355421X (DE-He213)BF00151169-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mattig, W. verfasserin aut On the instrumental and atmospheric stray-light for solar observations 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1983 Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. Good Condition Wavelength Region Solar Disk Solar Radius Atmospheric Component Enthalten in Solar physics Kluwer Academic Publishers, 1967 87(1983), 1 vom: Aug., Seite 187-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:87 year:1983 number:1 month:08 pages:187-193 https://doi.org/10.1007/BF00151169 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4305 GBV_ILN_4306 AR 87 1983 1 08 187-193 |
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10.1007/BF00151169 doi (DE-627)OLC203355421X (DE-He213)BF00151169-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mattig, W. verfasserin aut On the instrumental and atmospheric stray-light for solar observations 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1983 Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. Good Condition Wavelength Region Solar Disk Solar Radius Atmospheric Component Enthalten in Solar physics Kluwer Academic Publishers, 1967 87(1983), 1 vom: Aug., Seite 187-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:87 year:1983 number:1 month:08 pages:187-193 https://doi.org/10.1007/BF00151169 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4305 GBV_ILN_4306 AR 87 1983 1 08 187-193 |
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10.1007/BF00151169 doi (DE-627)OLC203355421X (DE-He213)BF00151169-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mattig, W. verfasserin aut On the instrumental and atmospheric stray-light for solar observations 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co 1983 Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. Good Condition Wavelength Region Solar Disk Solar Radius Atmospheric Component Enthalten in Solar physics Kluwer Academic Publishers, 1967 87(1983), 1 vom: Aug., Seite 187-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:87 year:1983 number:1 month:08 pages:187-193 https://doi.org/10.1007/BF00151169 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4305 GBV_ILN_4306 AR 87 1983 1 08 187-193 |
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on the instrumental and atmospheric stray-light for solar observations |
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On the instrumental and atmospheric stray-light for solar observations |
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Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. © D. Reidel Publishing Co 1983 |
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Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. © D. Reidel Publishing Co 1983 |
| abstract_unstemmed |
Abstract From aureole measurements made with a 40 cm-Vacuum-Telescope at Izaña (Tenerife) in the wavelength region 417 nm < λ < 785 nm and from a comparison with other aureole measurements we conclude the following: (a) Within one solar radius from the limb, the aureole is mostly of instrumental origin, (b) Beyond that distance, the contribution of atmospheric stray-light becomes noticeable, (c) The atmospheric contribution to the aureole intensity is, under good conditions at mountain stations, a very slowly decreasing function, and amounts to some $ 10^{−5} $ of the solar disk intensity. A procedure is given to separate the variable atmospheric component of the stray-light from the constant instrumental one. © D. Reidel Publishing Co 1983 |
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On the instrumental and atmospheric stray-light for solar observations |
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