UV radiation in the southern seas in early spring 1993
Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Wendler, G. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1996 |
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| Schlagwörter: |
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| Systematik: |
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| Anmerkung: |
© Springer-Verlag 1996 |
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| Übergeordnetes Werk: |
Enthalten in: Theoretical and applied climatology - Springer-Verlag, 1986, 53(1996), 4 vom: Dez., Seite 221-230 |
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| Übergeordnetes Werk: |
volume:53 ; year:1996 ; number:4 ; month:12 ; pages:221-230 |
| Links: |
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| DOI / URN: |
10.1007/BF00871738 |
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| Katalog-ID: |
OLC2048433979 |
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| 520 | |a Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. | ||
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10.1007/BF00871738 doi (DE-627)OLC2048433979 (DE-He213)BF00871738-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Wendler, G. verfasserin aut UV radiation in the southern seas in early spring 1993 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1996 Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. Ozone Ozone Concentration Radiation Level Global Radiation Ozone Level Quakenbush, T. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 53(1996), 4 vom: Dez., Seite 221-230 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:53 year:1996 number:4 month:12 pages:221-230 https://doi.org/10.1007/BF00871738 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4311 GBV_ILN_4313 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 53 1996 4 12 221-230 |
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10.1007/BF00871738 doi (DE-627)OLC2048433979 (DE-He213)BF00871738-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Wendler, G. verfasserin aut UV radiation in the southern seas in early spring 1993 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1996 Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. Ozone Ozone Concentration Radiation Level Global Radiation Ozone Level Quakenbush, T. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 53(1996), 4 vom: Dez., Seite 221-230 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:53 year:1996 number:4 month:12 pages:221-230 https://doi.org/10.1007/BF00871738 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4311 GBV_ILN_4313 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 53 1996 4 12 221-230 |
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10.1007/BF00871738 doi (DE-627)OLC2048433979 (DE-He213)BF00871738-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Wendler, G. verfasserin aut UV radiation in the southern seas in early spring 1993 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1996 Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. Ozone Ozone Concentration Radiation Level Global Radiation Ozone Level Quakenbush, T. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 53(1996), 4 vom: Dez., Seite 221-230 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:53 year:1996 number:4 month:12 pages:221-230 https://doi.org/10.1007/BF00871738 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4311 GBV_ILN_4313 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 53 1996 4 12 221-230 |
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10.1007/BF00871738 doi (DE-627)OLC2048433979 (DE-He213)BF00871738-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Wendler, G. verfasserin aut UV radiation in the southern seas in early spring 1993 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1996 Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. Ozone Ozone Concentration Radiation Level Global Radiation Ozone Level Quakenbush, T. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 53(1996), 4 vom: Dez., Seite 221-230 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:53 year:1996 number:4 month:12 pages:221-230 https://doi.org/10.1007/BF00871738 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4311 GBV_ILN_4313 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 53 1996 4 12 221-230 |
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10.1007/BF00871738 doi (DE-627)OLC2048433979 (DE-He213)BF00871738-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Wendler, G. verfasserin aut UV radiation in the southern seas in early spring 1993 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1996 Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. Ozone Ozone Concentration Radiation Level Global Radiation Ozone Level Quakenbush, T. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 53(1996), 4 vom: Dez., Seite 221-230 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:53 year:1996 number:4 month:12 pages:221-230 https://doi.org/10.1007/BF00871738 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4311 GBV_ILN_4313 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 53 1996 4 12 221-230 |
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uv radiation in the southern seas in early spring 1993 |
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UV radiation in the southern seas in early spring 1993 |
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Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. © Springer-Verlag 1996 |
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Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. © Springer-Verlag 1996 |
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Summary Radiation measurements were carried out during a research cruise of theN. Palmer in August and September 1993, from the tip of South America to Antarctica. As the measurements were carried out on a moving platform their validity had to be confirmed. This was undertaken for hourly data. Some of the main results are as follows:The radiation levels changed substantially during the cruise, as both latitude and season changed. Daily values of global, UV-A and UV-B radiation are presented.The mean value of the clearness indexKt (total transmissivity) was found to be 0.44. This is rather a low value, however, the cloudiness was high (mean value 78%). The clearness index increased with decreasing cloudiness from 0.41 for overcast conditions to 0.62 for clear sky conditions. Individual daily values varied even more, but always ranged between 0.2 and 0.8.The UV-A and UV-B radiation levels were related to the global radiation. However, correlation coefficients improved substantially when the analysis was carried out for different cloudiness classes. Clouds produced the largest reduction in global radiation and reduced UV-A and then UV-B to a lesser extent.As can be deduced from the previous bullet point therelative intensity of the UV radiation increased with cloudiness. This was more pronounced for UV-B than for UV-A.Ozone concentrations during the trip varied between 160 to 290 DU (Dobson Units). We passed under the “Antarctic ozone hole” several times during the cruise.UV-B radiation levels were affected by ozone levels and cloudiness. A 3-dimensional presentation is presented for UV-B versus ozone and cloudiness.UV-B radiation levels were, on average, more than double the average whilst under the “Antarctic ozone hole”, whereas UV-A radiation levels were hardly affected. © Springer-Verlag 1996 |
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