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UV climatology at Palmer Station, Antarctica, based on Version 2 NSF network data

机译:基于版本2 NSF网络数据的南极帕尔默站的紫外线气候

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Spectral ultraviolet (UV) and visible irradiance has been measured at Palmer Station, Antarctica, between 1988 and 2004 with a SUV-100 spectroradiometer. The instrument is part of the U.S. National Science Foundation's UV Monitoring Network. Here we present a UV climatology for Palmer Station based on the recently produced "Version 2" data edition. This data set will supersede the original release "Version 0". Corrections applied to the new version increased biologically effective UV dose rates by 0-9%. Values of UV-A irradiance changed by -8% to +10%. A comparison with results of a radiative transfer model confirmed that measurements of different years are consistent to within ±5%. Total ozone column was calculated from UV spectra and was found to agree with measurements of NASA's Total Ozone Mapping Spectrometer (TOMS) installed on the Nimbus-7 satellite to within 1%. TOMS measurements on the Earth Probe satellite are 3% lower than SUV-100 data. Effective surface albedo was estimated from clear sky spectra. Between August and November, albedo typically ranges between 0.6 and 0.95. After melting of snow and sea ice, albedo varies between 0.3 and 0.5. Biologically effective UV radiation is largest in November and December when low total ozone amounts coincide with relatively small solar zenith angles (SZA). During these months, the noon-time UV Index typically varies between 4 and 7, but UV indices as high as 14.8 have been observed. The largest erythemal daily dose of 8.8 kJ/m~2 was measured on 11/10/97 and 12/7/98. Linear regression analyses did not indicate statistically significant trends in UV or visible radiation, with the exception of February when small downward trends with statistical significance were observed. On average, clouds reduce UV irradiance at 345 nm between 28% (October and November) and 42% (February) compared to clear sky levels. In extreme cases, reductions by clouds can be as high as 90%. Between September and November, the variability introduced by ozone is similar to that caused by clouds.
机译:1988年至2004年之间,使用SUV-100分光光度计在南极帕尔默站测量了光谱紫外线(UV)和可见光辐照度。该仪器是美国国家科学基金会紫外线监测网络的一部分。在这里,我们根据最近制作的“版本2”数据版本介绍Palmer Station的紫外线气候。该数据集将取代原始发行版“版本0”。应用于新版本的修正使生物有效的紫外线剂量率增加了0-9%。 UV-A辐照度值从-8%更改为+ 10%。与辐射传输模型结果的比较证实,不同年份的测量值一致在±5%以内。总臭氧柱是根据紫外线光谱计算得出的,与安装在Nimbus-7卫星上的NASA总臭氧测图光谱仪(TOMS)的测量值相差1%以内。 Earth Probe卫星上的TOMS测量值比SUV-100数据低3%。有效表面反照率是根据晴朗的天空光谱估计的。在8月到11月之间,反照率通常在0.6到0.95之间。雪和海冰融化后,反照率在0.3到0.5之间变化。当臭氧总量较低且太阳天顶角(SZA)相对较小时,生物有效的紫外线辐射在11月和12月最大。在这几个月中,中午时紫外线指数通常在4到7之间变化,但观察到的紫外线指数高达14.8。在11/10/97和12/7/98测得的最大红斑日剂量为8.8 kJ / m〜2。线性回归分析未显示紫外线或可见辐射的统计学显着趋势,但2月份除外,当时观察到具有统计意义的小幅下降趋势。与晴朗的天空水平相比,平均而言,云在345 nm处的紫外线辐射降低了28%(十月和十一月)至42%(二月)。在极端情况下,云的减少可能高达90%。在9月和11月之间,臭氧引起的变异性类似于云造成的变异性。

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