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首页> 外文期刊>Atmospheric chemistry and physics >Aerosol optical depth measurements by airborne sun photometer in SOLVE II: Comparisons to SAGE III, POAM III and airborne spectrometer measurements
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Aerosol optical depth measurements by airborne sun photometer in SOLVE II: Comparisons to SAGE III, POAM III and airborne spectrometer measurements

机译:SOLVE II中通过机载太阳光度计进行气溶胶光学深度测量:与SAGE III,POAM III和机载光谱仪测量结果的比较

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The 14-channel NASA Ames Airborne Tracking Sunphotometer (AATS-14) measured solar-beam transmission on the NASA DC-8 during the second SAGE III Ozone Loss and ValidationExperiment (SOLVE II). This paper presents AATS-14 results for multiwavelength aerosoloptical depth (AOD), including comparisons to results from two satellite sensors and anotherDC-8 instrument, namely the Stratospheric Aerosol and Gas Experiment III (SAGE III), thePolar Ozone and Aerosol Measurement III (POAM III) and the Direct-beam Irradiance AirborneSpectrometer (DIAS). AATS-14 provides aerosol results at 13 wavelengths λ spanning therange of SAGE III and POAM III aerosol wavelengths. Because most AATS measurements weremade at solar zenith angles (SZA) near 90°, retrieved AODs are strongly affected byuncertainties in the relative optical airmass of the aerosols and other constituents along the lineof sight (LOS) between instrument and sun. To reduce dependence of the AATS-satellitecomparisons on airmass, we perform the comparisons in LOS transmission and LOS opticalthickness (OT) as well as in vertical OT (i.e., optical depth, OD). We also use a new airmassalgorithm that validates the algorithm we previously used to within 2% for SZA<90°, and inaddition provides results for SZA≥90°.

For 6 DC-8 flights, 19 January-2 February 2003, AATS and DIAS results for LOS aerosol OT atλ=400nm agree to ≤12%of the AATS value. Mean and root-mean-square (RMS) differences,(DIAS-AATS)/AATS, are -2.3% and 7.7%, respectively.For DC-8 altitudes, AATS-satellite comparisons are possible only for λ>440nm, because ofsignal depletion for shorter λ on the satellite full-limb LOS. For the 4 AATS-SAGE and4 AATS-POAM near-coincidences conducted 19-31 January 2003, AATS-satellite AODdifferences were ≤0.0041 for all λ>440nm. RMS differences were ≤0.0022 for SAGE-AATSand ≤0.0026 for POAM-AATS. RMS relative differences in AOD ([SAGE-AATS]/AATS) were≤33% for λ<~755nm, but grew to 59% for 1020nm and 66% at 1545nm. For λ>~755nm,AATS-POAM differences were less than AATS-SAGE differences, and RMS relativedifferences in AOD ([AATS-POAM]/AATS) were ≤31% for all λ between 440 and 1020nm.Unexplained differences that remain are associated with transmission differences, rather thandifferences in gas subtraction or conversion from LOS to vertical quantities. The very smallstratospheric AOD values that occurred during SOLVE II added to the challenge of thecomparisons, but do not explain all the differences.

机译:14通道的NASA艾姆斯机载跟踪日光计(AATS-14)在第二次SAGE III臭氧损失和验证实验(SOLVE II)期间测量了NASA DC-8上的太阳光束透射率。本文介绍了多波长气溶胶深度( AOD )的AATS-14结果,包括与两个卫星传感器和另一台DC-8仪器(平流层气溶胶和气体实验III(SAGE III),Polar)的结果进行比较臭氧和气溶胶测量III(POAM III)和直接束辐照机载光谱仪(DIAS)。 AATS-14在跨越SAGE III和POAM III气溶胶波长范围的13个波长λ处提供气溶胶结果。由于大多数ATS的测量都是在接近90°的太阳天顶角( SZA )上进行的,因此,所获得的 AOD 受到沿途气溶胶和其他成分的相对光学气质不确定性的强烈影响。仪器和太阳之间的视线(LOS)。为了减少AATS卫星比较对气团的依赖性,我们在LOS传输和LOS光学厚度(OT)以及垂直OT(即光学深度, OD )中进行比较。我们还使用了一种新的空气质量算法,该算法验证了先前用于 SZA <90°的算法在2%以内的算法,此外还提供了 SZA ≥90°的结果。 =“ line-height:20px;”>对于2003年1月19日至2月2日的6架DC-8航班,LOS气溶胶OT在λ= 400nm处的AATS和DIAS结果符合≤AATS值的12%。 (DIAS-AATS)/ AATS的均值和均方根(RMS)差分别为-2.3%和7.7%。对于DC-8高度,由于信号的缘故,仅在λ> 440nm时才可以进行ATS-卫星比较卫星全边视距上的较短λ的损耗。对于2003年1月19日至31日进行的4次AATS-SAGE和4次AATS-POAM近符合,所有λ> 440nm的AATS-卫星 AOD 差均≤0.0041。 SAGE-AATS的RMS差异≤0.0022,POAM-AATS的RMS差异≤0.0026。 AOD ([SAGE-AATS] / AATS)的RMS相对差异在λ<〜755nm时≤33%,但在1020nm时为59%,在1545nm时为66%。对于λ>〜755nm,AATS-POAM差异小于AATS-SAGE差异,并且 AOD ([AATS-POAM] / AATS)的RMS相对差异≤440%至1020nm之间的所有λ剩余的无法解释的差异与传输差异有关,而不是与气体减法差异或从LOS转换为垂直量的差异有关。 SOLVE II期间发生的非常小的平流层 AOD 值增加了比较的挑战,但并不能解释所有差异。

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