High‐resolution absorption spectroscopy of the circumgalactic medium of the Milky Way

In this article we discuss the importance of high‐resolution absorption spectroscopy for our understanding of the distribution and physical nature of the gaseous circumgalactic medium (CGM) that surrounds the Milky Way. Observational and theoretical studies indicate a high complexity of the gas kinematics and an extreme multi‐phase nature of the CGM in low‐redshift galaxies. High‐precision absorption‐line measurements of the Milky Way's gas environment thus are essential to explore fundamental parameters of circumgalactic gas in the local Universe, such as mass, chemical composition, and spatial distribution. We shortly review important characteristics of the Milky Way's CGM and discuss recent results from our multi‐wavelength observations of the Magellanic Stream. Finally, we discuss the potential of studying the warm‐hot phase of the Milky Way's CGM by searching for extremely weak [Fe X] λ 6374.5 Å and [Fe XIV] λ 5302.9 Å absorption in optical QSO spectra. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

卫星反演太阳紫外辐射数据产品在东疆黑戈壁区域的适用性验证

论文利用2017年东疆哈密地区红柳河黑戈壁地面高精度紫外辐射实测数据与美国NASA Langely研究中心大气科学数据中心提供的CERES_SYN1 deg_Ed4A产品数据,对卫星反演的紫外辐射A、B波段(UVA和UVB)数据在该地区的适用性进行了对比验证。结果表明：① 在日尺度上,该地区地面实测紫外辐射UVA和UVB与卫星反演数据之间的相关系数达0.9以上,其中在全天空情况下UVA平均偏差为1.15 W·m ^-2、UVB 平均偏差为0.03 W·m ^-2,晴天条件下UVA和UVB的平均偏差分别为0.93 W·m ^-2和0.03 W·m ^-2;② 在季节尺度上,实测和卫星反演UVA和UVB的偏差夏季最大,分别为2.04 W·m ^-2和0.05 W·m ^-2,春冬两季次之,秋季最小;③ 红柳河地区在春夏两季受到气溶胶光学厚度(AOD)影响较大,呈现显著负相关;④ 云量越大,紫外辐射削弱程度越大,在多云条件下地面实测与卫星反演UVA与UVB偏差最大,分别为1.73 W·m ^-2和0.05 W·m ^-2。     

石油类污染水体吸收特性分析

石油类污染物主要以漂浮油、分散油、乳化油和分解油等形式存在于水体中,影响着水体的表观和固有光学特性。利用2008年5月在辽宁省盘锦市辽河油田境内双台子河和绕阳河所测定的水色三要素吸收系数以及对应的水体组分数据,分析了研究区域内Ⅱ类水体水色三要素的吸收光谱特性;探讨了水体中由于石油类污染物的存在,黄色物质和色素吸收光谱的变化特征;采用差值法确定了水体中石油类污染物的吸收系数。研究结果表明:(1)研究区域内,无论是石油类污染水体还是非石油类污染水体,非色素颗粒物和黄色物质的吸收光谱都遵循e指数衰减规律,色素吸收光谱在440nm和675nm处有以叶绿素为主的典型的色素吸收峰,在490nm处有类胡萝卜素的吸收峰;(2)对于石油类污染水体,在测定黄色物质和色素吸收系数时,由于包含了石油类污染物的作用,会增大黄色物质和色素的吸收系数;(3)石油类物质的吸收光谱曲线和非色素颗粒物、黄色物质一样遵循e指数衰减规律,但三者的指数函数斜率有明显的差别,这为将三者区分开来提供了可行性。     

成象光谱图象光谱吸收鉴别模型与矿物填图研究

本文提出了一种光谱吸收鉴别模型，拟通过矿物光谱吸收特征的鉴别，在成象光谱上实现矿物直接识别与填图。该模型的核心是光谱吸收指数技术（ＳＡＩ）。从理论上探讨了ＳＡＩ的本质，应用Ｈａｐｋｅ光谱模型讨论了ＳＡＩ与光谱吸收系数（ｄ）以及单散射反照率（ｗ）之间的函数关系，并从成象光谱图象辐射信息传递过程分析了图象ＳＡＩ与光谱吸收深度的关系，而光谱吸收深度与岩石矿物成分含量之间具有定量关系，这显示了ＳＡＩ提取矿物定量遥感信息能力。ＳＡＩ已经成功地应用于ＦＩＭＳ、ＭＡＩＳ和ＧＥＲＩＳ图象处理与矿物填图，本文通过哈图、塔里木、以及澳大利亚松谷的实例研究，表明ＳＡＩ是一种有效的提取矿物类型与丰度信息的方法。     

水合铁离子及铁络合物吸收系数光谱(400-900 nm)测量

测量铁化合物溶解物的吸收光谱曲线是水中铁离子含量遥感反演的关键。采用自主设计的水体透射光测量装置,利用ASD光谱仪测量相同厚度不同浓度铁离子溶液的透射光辐亮度,然后运用比值法计算出水中3种铁化合物(硫酸铁、氯化铁和铁氰化钾)的消光系数和吸收系数,最终得到400—900 nm波长范围内3种铁离子吸收系数光谱。该方法可以较好地消除实验装置和水中悬浮物的影响。结果表明,水中3种铁离子均在紫蓝光波段吸收作用较大,绿光次之,逐渐减少至红光波段后,吸收系数变化很小呈平缓直线。测量结果可作为水体铁离子浓度遥感反演模型所需的基础参数。     

激光掩星探测大气UTLS温度和水汽的方法及仿真

以高精度和高垂直分辨率探测大气区间对流层顶—平流层底UTLS (Upper Troposphere/Lower Stratosphere,5—35 km)的温度和水汽廓线是提高大气条件变化监测水平的关键,而利用激光掩星方法同时探测温度和水汽则是对现有探测技术的重要补充。本文研究了激光掩星协同探测和反演温度和水汽分子数密度的方法,其中重点研究了双吸收波长近红外激光反演温度的方法,具体为从近红外波段氧气吸收光谱中,选择2个不同跃迁能级对应的特征吸收峰,在每个吸收峰附近各选出1个吸收线,利用2个吸收线对应的双吸收波长激光以及参考线对应波长激光进行掩星探测,进而由探测数据反演出温度。整个温度和水汽协同反演步骤是先反演温度廓线,然后由温度廓线以及5 km参考高度处的压强先验值计算得到压强廓线,最后在温度和压强廓线基础上,结合水汽单吸收波长和参考波长激光掩星数据,反演得到水汽分子数密度廓线。此外,本文对探测和反演过程进行了模拟仿真,通过在近红外波段选择合适的氧气吸收波长和水汽吸收波长,模拟得到掩星透过率数据,以此反演得到温度和水汽分子数密度廓线。并通过对整个过程的分析,明确了反演过程中的误差项及其...     

The NO2 absorption spectrum. I: Absorption cross-sections at ambient temperature in the 300–500 nm region

New laboratory measurements of NO₂ absorption cross-sections have been performed between 300 and 500 nm at ambient temperature with improved experimental conditions: low gas pressures, long absorption paths, suitable absorbance values, narrow spectral bandwidths. The data, stored at 0.01 nm intervals, have been compared to those of the more recent studies and some reasons of disagreement are discussed.In the photolysis region below 400 nm, our absorption cross-sections are larger than those previously published, suggesting that the photodissociation coefficient calculated from the current data sets is underestimated. In the structured region of the spectrum above 400 nm, improvement of the resolution gives more precise values useful for optical measurements in atmosphere.Unité de Recherche Associée au CNRS.     

Analysis of UVB values in the centre of the Iberian Peninsula

Records of UV data started in Madrid at the beginning of the 90's decade. After some quality control on the data a seven year period from 1996 to 2002 was selected to perform an analysis of daily and seasonal variability of solar ultraviolet B (UVB) values at the centre of the Iberian Peninsula. Instruments used are a Brewer MKIV spectrophotometer and a YES UVB-1 broadband pyranometer. Both instruments provided integrated daily values according with the Diffey spectrum although they have different measurement procedures. Data statistics from each instrument for the same period and statistical relationships between daily values from both instruments are shown. As broadband YES provided a record with fewer time gaps, analysis of UVI extreme values is performed using that instrument. The relationship between UVB values with ozone, cloudiness and visible radiation has been described in several papers for different places in the world. In this paper, those relationships are shown for Madrid. A discussion about specific problems found when trying to isolate every effective factor is also included. Some of those relationships could be helpful to retrieve UVB values from other ancillary data as visible radiation and cloudiness. Finally, a detailed study for 10 days in June 1997 when the maximum record of daily values from the present time series was obtained, highlight the close correlation between total ozone content and the daily variability of UVB for similar amounts of incoming radiation.     

冠层内动量和物质吸收特征的数值研究

本文设计了一冠层(CL)和大气边界层(ABL)之间物质和动量交换的耦合模式,并对CL内风速、物质随高度分布和日变化作了数值模拟.结果表明,由大尺度扩散引起冠层低层的第二个风速极大和多极值的浓度分布,CL内湍流通量和物质浓度随高度减小而迅速降低,以及CL动量减小对浓度分布的重要影响,模式都能很好地描述,模拟结果与观测事实有好的一致性.利用浓度和温度廓线相似假设,导出了质量汇的经验关系.     

哈尔滨市地下水污染特征与水质净化作用研究

松花江哈尔滨江段水质污染较重,是否可能通过入渗补给影响哈尔滨市区地下水的水质?为此,分别对松花江哈尔滨江段和哈尔滨市地下含水层的污染特征与各自的净化能力进行了分析研究.结果表明,两者的净化能力均很强,并可不断地得以自然恢复。净化作用主要表现为稀释、吸附、过滤等.保持这种自然净化能力,对保护哈尔滨市地下含水层的优良水质有十分重要的作用。