Solar Irradiance from 165 to 400 nm in 2008 and UV Variations in Three Spectral Bands During Solar Cycle 24
Abstract Accurate measurements of the solar spectral irradiance (SSI) and its temporal variations are of primary interest to better understand solar mechanisms, and the links between solar variability and Earth’s atmosphere and climate. The SOLar SPECtrum (SOLSPEC) instrument of the Solar Monitoring...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Meftah, M. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media Dordrecht 2016 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Springer Netherlands, 1967, 291(2016), 12 vom: 18. Okt., Seite 3527-3547 |
|---|---|
| Übergeordnetes Werk: |
volume:291 ; year:2016 ; number:12 ; day:18 ; month:10 ; pages:3527-3547 |
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|---|
| DOI / URN: |
10.1007/s11207-016-0997-8 |
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OLC2033621693 |
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| 520 | |a Abstract Accurate measurements of the solar spectral irradiance (SSI) and its temporal variations are of primary interest to better understand solar mechanisms, and the links between solar variability and Earth’s atmosphere and climate. The SOLar SPECtrum (SOLSPEC) instrument of the Solar Monitoring Observatory (SOLAR) payload onboard the International Space Station (ISS) has been built to carry out SSI measurements from 165 to 3088 nm. We focus here on the ultraviolet (UV) part of the measured solar spectrum (wavelengths less than 400 nm) because the UV part is potentially important for understanding the solar forcing of Earth’s atmosphere and climate. We present here SOLAR/SOLSPEC UV data obtained since 2008, and their variations in three spectral bands during Solar Cycle 24. They are compared with previously reported UV measurements and model reconstructions, and differences are discussed. | ||
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10.1007/s11207-016-0997-8 doi (DE-627)OLC2033621693 (DE-He213)s11207-016-0997-8-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Meftah, M. verfasserin aut Solar Irradiance from 165 to 400 nm in 2008 and UV Variations in Three Spectral Bands During Solar Cycle 24 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2016 Abstract Accurate measurements of the solar spectral irradiance (SSI) and its temporal variations are of primary interest to better understand solar mechanisms, and the links between solar variability and Earth’s atmosphere and climate. The SOLar SPECtrum (SOLSPEC) instrument of the Solar Monitoring Observatory (SOLAR) payload onboard the International Space Station (ISS) has been built to carry out SSI measurements from 165 to 3088 nm. We focus here on the ultraviolet (UV) part of the measured solar spectrum (wavelengths less than 400 nm) because the UV part is potentially important for understanding the solar forcing of Earth’s atmosphere and climate. We present here SOLAR/SOLSPEC UV data obtained since 2008, and their variations in three spectral bands during Solar Cycle 24. They are compared with previously reported UV measurements and model reconstructions, and differences are discussed. Solar irradiance Solar cycle Instrumentation and data management Instrumental effects Bolsée, D. aut Damé, L. aut Hauchecorne, A. aut Pereira, N. aut Irbah, A. aut Bekki, S. aut Cessateur, G. aut Foujols, T. aut Thiéblemont, R. aut Enthalten in Solar physics Springer Netherlands, 1967 291(2016), 12 vom: 18. Okt., Seite 3527-3547 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:291 year:2016 number:12 day:18 month:10 pages:3527-3547 https://doi.org/10.1007/s11207-016-0997-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_70 AR 291 2016 12 18 10 3527-3547 |
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10.1007/s11207-016-0997-8 doi (DE-627)OLC2033621693 (DE-He213)s11207-016-0997-8-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Meftah, M. verfasserin aut Solar Irradiance from 165 to 400 nm in 2008 and UV Variations in Three Spectral Bands During Solar Cycle 24 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2016 Abstract Accurate measurements of the solar spectral irradiance (SSI) and its temporal variations are of primary interest to better understand solar mechanisms, and the links between solar variability and Earth’s atmosphere and climate. The SOLar SPECtrum (SOLSPEC) instrument of the Solar Monitoring Observatory (SOLAR) payload onboard the International Space Station (ISS) has been built to carry out SSI measurements from 165 to 3088 nm. We focus here on the ultraviolet (UV) part of the measured solar spectrum (wavelengths less than 400 nm) because the UV part is potentially important for understanding the solar forcing of Earth’s atmosphere and climate. We present here SOLAR/SOLSPEC UV data obtained since 2008, and their variations in three spectral bands during Solar Cycle 24. They are compared with previously reported UV measurements and model reconstructions, and differences are discussed. Solar irradiance Solar cycle Instrumentation and data management Instrumental effects Bolsée, D. aut Damé, L. aut Hauchecorne, A. aut Pereira, N. aut Irbah, A. aut Bekki, S. aut Cessateur, G. aut Foujols, T. aut Thiéblemont, R. aut Enthalten in Solar physics Springer Netherlands, 1967 291(2016), 12 vom: 18. Okt., Seite 3527-3547 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:291 year:2016 number:12 day:18 month:10 pages:3527-3547 https://doi.org/10.1007/s11207-016-0997-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_70 AR 291 2016 12 18 10 3527-3547 |
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10.1007/s11207-016-0997-8 doi (DE-627)OLC2033621693 (DE-He213)s11207-016-0997-8-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Meftah, M. verfasserin aut Solar Irradiance from 165 to 400 nm in 2008 and UV Variations in Three Spectral Bands During Solar Cycle 24 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2016 Abstract Accurate measurements of the solar spectral irradiance (SSI) and its temporal variations are of primary interest to better understand solar mechanisms, and the links between solar variability and Earth’s atmosphere and climate. The SOLar SPECtrum (SOLSPEC) instrument of the Solar Monitoring Observatory (SOLAR) payload onboard the International Space Station (ISS) has been built to carry out SSI measurements from 165 to 3088 nm. We focus here on the ultraviolet (UV) part of the measured solar spectrum (wavelengths less than 400 nm) because the UV part is potentially important for understanding the solar forcing of Earth’s atmosphere and climate. We present here SOLAR/SOLSPEC UV data obtained since 2008, and their variations in three spectral bands during Solar Cycle 24. They are compared with previously reported UV measurements and model reconstructions, and differences are discussed. Solar irradiance Solar cycle Instrumentation and data management Instrumental effects Bolsée, D. aut Damé, L. aut Hauchecorne, A. aut Pereira, N. aut Irbah, A. aut Bekki, S. aut Cessateur, G. aut Foujols, T. aut Thiéblemont, R. aut Enthalten in Solar physics Springer Netherlands, 1967 291(2016), 12 vom: 18. Okt., Seite 3527-3547 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:291 year:2016 number:12 day:18 month:10 pages:3527-3547 https://doi.org/10.1007/s11207-016-0997-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_70 AR 291 2016 12 18 10 3527-3547 |
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solar irradiance from 165 to 400 nm in 2008 and uv variations in three spectral bands during solar cycle 24 |
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Solar Irradiance from 165 to 400 nm in 2008 and UV Variations in Three Spectral Bands During Solar Cycle 24 |
| abstract |
Abstract Accurate measurements of the solar spectral irradiance (SSI) and its temporal variations are of primary interest to better understand solar mechanisms, and the links between solar variability and Earth’s atmosphere and climate. The SOLar SPECtrum (SOLSPEC) instrument of the Solar Monitoring Observatory (SOLAR) payload onboard the International Space Station (ISS) has been built to carry out SSI measurements from 165 to 3088 nm. We focus here on the ultraviolet (UV) part of the measured solar spectrum (wavelengths less than 400 nm) because the UV part is potentially important for understanding the solar forcing of Earth’s atmosphere and climate. We present here SOLAR/SOLSPEC UV data obtained since 2008, and their variations in three spectral bands during Solar Cycle 24. They are compared with previously reported UV measurements and model reconstructions, and differences are discussed. © Springer Science+Business Media Dordrecht 2016 |
| abstractGer |
Abstract Accurate measurements of the solar spectral irradiance (SSI) and its temporal variations are of primary interest to better understand solar mechanisms, and the links between solar variability and Earth’s atmosphere and climate. The SOLar SPECtrum (SOLSPEC) instrument of the Solar Monitoring Observatory (SOLAR) payload onboard the International Space Station (ISS) has been built to carry out SSI measurements from 165 to 3088 nm. We focus here on the ultraviolet (UV) part of the measured solar spectrum (wavelengths less than 400 nm) because the UV part is potentially important for understanding the solar forcing of Earth’s atmosphere and climate. We present here SOLAR/SOLSPEC UV data obtained since 2008, and their variations in three spectral bands during Solar Cycle 24. They are compared with previously reported UV measurements and model reconstructions, and differences are discussed. © Springer Science+Business Media Dordrecht 2016 |
| abstract_unstemmed |
Abstract Accurate measurements of the solar spectral irradiance (SSI) and its temporal variations are of primary interest to better understand solar mechanisms, and the links between solar variability and Earth’s atmosphere and climate. The SOLar SPECtrum (SOLSPEC) instrument of the Solar Monitoring Observatory (SOLAR) payload onboard the International Space Station (ISS) has been built to carry out SSI measurements from 165 to 3088 nm. We focus here on the ultraviolet (UV) part of the measured solar spectrum (wavelengths less than 400 nm) because the UV part is potentially important for understanding the solar forcing of Earth’s atmosphere and climate. We present here SOLAR/SOLSPEC UV data obtained since 2008, and their variations in three spectral bands during Solar Cycle 24. They are compared with previously reported UV measurements and model reconstructions, and differences are discussed. © Springer Science+Business Media Dordrecht 2016 |
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Solar Irradiance from 165 to 400 nm in 2008 and UV Variations in Three Spectral Bands During Solar Cycle 24 |
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