Modelling the effects of solar variability on the middle atmosphere: A review
The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1994 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
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| Übergeordnetes Werk: |
in: Advances in Space Research - Amsterdam : Elsevier, 14(1994), 9, Seite 211-220 |
| Übergeordnetes Werk: |
volume:14 ; year:1994 ; number:9 ; pages:211-220 |
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| 520 | |a The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric forcing. Experiments with two types of numerical model used to examine the atmospheric response to changes in solar forcing are reviewed here. Firstly, mechanistic-model simultations of the solar-induced 27- and 13-day oscillations show that weak perturbations generated in the upper stratosphere can lead to detectable oscillations in the lower atmosphere. Secondly, a general circulation model shows that the modulation of the middle atmosphere dynamics by solar actity and the equatorial quasi-biennial oscillation is feasible. There are limitations to the studies. | ||
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(DE-627)NLEJ181659247 (DE-599)GBVNLZ181659247 DE-627 ger DE-627 rakwb eng Modelling the effects of solar variability on the middle atmosphere: A review 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric forcing. Experiments with two types of numerical model used to examine the atmospheric response to changes in solar forcing are reviewed here. Firstly, mechanistic-model simultations of the solar-induced 27- and 13-day oscillations show that weak perturbations generated in the upper stratosphere can lead to detectable oscillations in the lower atmosphere. Secondly, a general circulation model shows that the modulation of the middle atmosphere dynamics by solar actity and the equatorial quasi-biennial oscillation is feasible. There are limitations to the studies. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Dameris, M. oth Pawson, S. oth in Advances in Space Research Amsterdam : Elsevier 14(1994), 9, Seite 211-220 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:14 year:1994 number:9 pages:211-220 http://dx.doi.org/10.1016/0273-1177(94)90138-4 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1994 9 211-220 |
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(DE-627)NLEJ181659247 (DE-599)GBVNLZ181659247 DE-627 ger DE-627 rakwb eng Modelling the effects of solar variability on the middle atmosphere: A review 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric forcing. Experiments with two types of numerical model used to examine the atmospheric response to changes in solar forcing are reviewed here. Firstly, mechanistic-model simultations of the solar-induced 27- and 13-day oscillations show that weak perturbations generated in the upper stratosphere can lead to detectable oscillations in the lower atmosphere. Secondly, a general circulation model shows that the modulation of the middle atmosphere dynamics by solar actity and the equatorial quasi-biennial oscillation is feasible. There are limitations to the studies. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Dameris, M. oth Pawson, S. oth in Advances in Space Research Amsterdam : Elsevier 14(1994), 9, Seite 211-220 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:14 year:1994 number:9 pages:211-220 http://dx.doi.org/10.1016/0273-1177(94)90138-4 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1994 9 211-220 |
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(DE-627)NLEJ181659247 (DE-599)GBVNLZ181659247 DE-627 ger DE-627 rakwb eng Modelling the effects of solar variability on the middle atmosphere: A review 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric forcing. Experiments with two types of numerical model used to examine the atmospheric response to changes in solar forcing are reviewed here. Firstly, mechanistic-model simultations of the solar-induced 27- and 13-day oscillations show that weak perturbations generated in the upper stratosphere can lead to detectable oscillations in the lower atmosphere. Secondly, a general circulation model shows that the modulation of the middle atmosphere dynamics by solar actity and the equatorial quasi-biennial oscillation is feasible. There are limitations to the studies. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Dameris, M. oth Pawson, S. oth in Advances in Space Research Amsterdam : Elsevier 14(1994), 9, Seite 211-220 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:14 year:1994 number:9 pages:211-220 http://dx.doi.org/10.1016/0273-1177(94)90138-4 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1994 9 211-220 |
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(DE-627)NLEJ181659247 (DE-599)GBVNLZ181659247 DE-627 ger DE-627 rakwb eng Modelling the effects of solar variability on the middle atmosphere: A review 1994 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric forcing. Experiments with two types of numerical model used to examine the atmospheric response to changes in solar forcing are reviewed here. Firstly, mechanistic-model simultations of the solar-induced 27- and 13-day oscillations show that weak perturbations generated in the upper stratosphere can lead to detectable oscillations in the lower atmosphere. Secondly, a general circulation model shows that the modulation of the middle atmosphere dynamics by solar actity and the equatorial quasi-biennial oscillation is feasible. There are limitations to the studies. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Dameris, M. oth Pawson, S. oth in Advances in Space Research Amsterdam : Elsevier 14(1994), 9, Seite 211-220 (DE-627)NLEJ180340476 (DE-600)2023311-5 0273-1177 nnns volume:14 year:1994 number:9 pages:211-220 http://dx.doi.org/10.1016/0273-1177(94)90138-4 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1994 9 211-220 |
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modelling the effects of solar variability on the middle atmosphere: a review |
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Modelling the effects of solar variability on the middle atmosphere: A review |
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The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric forcing. Experiments with two types of numerical model used to examine the atmospheric response to changes in solar forcing are reviewed here. Firstly, mechanistic-model simultations of the solar-induced 27- and 13-day oscillations show that weak perturbations generated in the upper stratosphere can lead to detectable oscillations in the lower atmosphere. Secondly, a general circulation model shows that the modulation of the middle atmosphere dynamics by solar actity and the equatorial quasi-biennial oscillation is feasible. There are limitations to the studies. |
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The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric forcing. Experiments with two types of numerical model used to examine the atmospheric response to changes in solar forcing are reviewed here. Firstly, mechanistic-model simultations of the solar-induced 27- and 13-day oscillations show that weak perturbations generated in the upper stratosphere can lead to detectable oscillations in the lower atmosphere. Secondly, a general circulation model shows that the modulation of the middle atmosphere dynamics by solar actity and the equatorial quasi-biennial oscillation is feasible. There are limitations to the studies. |
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The effects of solar activity on the middle atmosphere are controversial since no clear physical mechanism exists to explain the interactions. Further, it is extremely difficult to isolate any solar-induced variability, since the dominant influence on the middle atmosphere appears to be tropospheric forcing. Experiments with two types of numerical model used to examine the atmospheric response to changes in solar forcing are reviewed here. Firstly, mechanistic-model simultations of the solar-induced 27- and 13-day oscillations show that weak perturbations generated in the upper stratosphere can lead to detectable oscillations in the lower atmosphere. Secondly, a general circulation model shows that the modulation of the middle atmosphere dynamics by solar actity and the equatorial quasi-biennial oscillation is feasible. There are limitations to the studies. |
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