Wuttke Sigrid, El Naggar Saad, Bluszcz Thaddäus, Schrems Otto
Alfred Wegener Institute for Polar and Marine Research, Am Handelshafen 12, 27570, Bremerhaven, Germany.
Photochem Photobiol Sci. 2007 Oct;6(10):1081-8. doi: 10.1039/b617602j. Epub 2007 Sep 3.
Ship-borne measurements of spectral as well as biologically effective UV irradiance have been performed on the German research vessel Polarstern during the Atlantic transect from Bremerhaven, Germany (53.5 degrees N, 8.5 degrees E), to Cape Town, South Africa (33.6 degrees S, 18.3 degrees E), from 13 October to 17 November 2005. Such measurements are required to study UV effects on marine organisms. They are also necessary to validate satellite-derived surface UV irradiance. Cloud free radiative transfer calculations support the investigation of this latitudinal dependence. Input parameters, such as total ozone column and aerosol optical depth have been measured on board as well. Using these measured parameters, the modelled cloudless noontime UVA irradiance (320-400 nm) shows the expected dependence on varying minimum solar zenith angles (SZA) at different latitudes. The modelled cloudless noontime UVB irradiance (290-320 nm) does not show this clear dependence on SZA due to the strong influence of ozone absorption in this spectral range. The maximum daily dose of erythemal irradiance of 5420 J m(-1) was observed on 14 November 2005, when the ship was in the tropical Atlantic south of the equator. The expected UV maximum should have been observed with the sun in the zenith during local noon (11 November). Stratiform clouds reduced the dose to 3835 J m(-1). In comparison, the daily erythemal doses in the mid-latitudinal Bay of Biscay only reached values between 410 and 980 J m(-1) depending on cloud conditions. The deviation in daily erythemal dose derived from different instruments is around 5%. The feasibility to perform ship-borne measurements of spectral UV irradiance is demonstrated.
2005年10月13日至11月17日期间,在德国研究船“极地号”从德国不来梅港(北纬53.5度,东经8.5度)至南非开普敦(南纬33.6度,东经18.3度)的大西洋断面航线上,进行了光谱以及生物有效紫外线辐照度的船载测量。进行此类测量对于研究紫外线对海洋生物的影响是必要的。它们对于验证卫星得出的地表紫外线辐照度也是必不可少的。无云辐射传输计算有助于对这种纬度依赖性进行研究。诸如总臭氧柱和气溶胶光学厚度等输入参数也在船上进行了测量。利用这些测量参数,模拟的无云正午UVA辐照度(320 - 400纳米)显示出在不同纬度对变化的最小太阳天顶角(SZA)的预期依赖性。由于该光谱范围内臭氧吸收的强烈影响,模拟的无云正午UVB辐照度(290 - 320纳米)并未显示出对SZA的这种明显依赖性。2005年11月14日,当船位于赤道以南的热带大西洋时,观测到了5420焦每平方米的最大每日红斑辐照度。预期的紫外线最大值本应在当地正午(11月11日)太阳位于天顶时观测到。层状云将剂量降低至3835焦每平方米。相比之下,取决于云况,中纬度的比斯开湾的每日红斑剂量仅达到410至980焦每平方米之间的值。不同仪器得出的每日红斑剂量偏差约为5%。证明了进行光谱紫外线辐照度船载测量的可行性。