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The martian dust chronicle: Eight years of reconstructed climatology from spacecraft observations

机译:火星尘埃编年史:来自航天器观测的八年重建气候学

摘要

We have reconstructed the climatology of airborne dust from Martian years (MY) 24 to 31 using multiple datasetsudof retrieved or estimated column optical depth. The datasets are based on observations of the Martian atmosphereudfrom March 1999 to July 2013 by different orbiting instruments: the Thermal Emission Spectrometer (TES)udon board Mars Global Surveyor, the Thermal Emission Imaging System (THEMIS) on board Mars Odyssey,udand the Mars Climate Sounder (MCS) on board Mars Reconnaissance Orbiter (MRO). The procedure we haveudadopted consists in gridding the available retrievals of column dust optical depth (CDOD) from TES and THEMISudnadir observations, as well as the estimates of this quantity from MCS limb observations. Our gridding methodudcalculates weighted averages on a regular but likely incomplete spatial grid, using an iterative procedure withudweights in space, time, and retrieval uncertainty. The derived product consists of daily synoptic gridded maps ofudCDOD at a resolution of 6 degree longitude x 3 degree latitude for MY 24-26, and 6 degree longitude x 5 degreeudlatitude for MY 27-31.udWe have statistically analyzed the gridded maps to present an overview of the dust climatology on Marsudover eight years, specifically in relation to its intraseasonal and interannual variability.udFinally, we have produced complete daily maps of CDOD by spatially interpolating the available incompleteudgridded maps using a kriging method. These complete maps are used as dust scenarios in the Mars ClimateudDatabase (MCD) version 5, and should be useful for many other applications.udThe maps for the eight available Martian years are publicly available and distributed with open access, underudCreative Commons Attribution-ShareAlike 3.0 Unported License. The current version and future updatesudcan be downloaded from the MCD website at the Laboratoire de Meteorologie Dynamique: http://wwwmars.udlmd.jussieu.fr/mars/dust_climatology/
机译:我们使用多个数据集 udof检索到的或估计的柱光学深度,重建了从火星年(MY)24到31的气浮尘气候。这些数据集是基于1999年3月至2013年7月通过不同轨道仪器对火星大气的观测得出的:热发射光谱仪(TES)火星全球测量公司的乌冬面,火星奥德赛上的热成像系统( THEMIS), uds和Mars Reconnaissance Orbiter(MRO)上的Mars Climate Sounder(MCS)。我们已经采用的程序包括对来自TES和THEMIS udnadir观测值的柱尘光学深度(CDOD)的可用检索结果进行网格化,以及根据MCS肢体观测值对该量的估计。我们的网格化方法 ud使用空间,时间和检索不确定性 udweights的迭代过程,在规则但可能不完整的空间网格上计算加权平均值。派生产品由 udCDOD的每日概要网格图组成,对于MY 24-26,分辨率为6度经度x 3度纬度,对于MY 27-31,分辨率为6度经度x 5度纬度。 ud网格地图以概述火星 udover八年的沙尘气候学概况,特别是关于其季节内和年际变化的 ud。最后,我们通过使用克里金法对可用的不完整 udgrid的地图进行空间插值,制作了完整的CDOD日图方法。这些完整的地图在“火星气候” udDatabase(MCD)版本5中被用作尘埃场景,并且对许多其他应用程序也将很有用。 ud八月可用的火星年份的地图是公开可用的,并在 udCreative下公开开放Commons Attribution-ShareAlike 3.0无端口许可证。当前版本和将来的更新 ud可以从MCD网站上的实验室动力学实验室下载:http:// wwwmars。 udlmd.jussieu.fr/mars/dust_climatology/

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