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首页> 外文期刊>Icarus: International Journal of Solar System Studies >Meteorological pressure at Gale crater from a comparison of REMS/MSL data and MCD modelling: Effect of dust storms
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Meteorological pressure at Gale crater from a comparison of REMS/MSL data and MCD modelling: Effect of dust storms

机译:VELS / MSL数据和MCD模型的比较,大牙陨石坑的气象压力:尘暴的影响

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We examine the record of atmospheric pressure in Gale crater measured in-situ by the Rover Environmental Monitoring Station (REMS) instrument (Gomez-Elvira et al., 2012) on the Mars Science Laboratory (MSL) rover over two Martian years. We compare the data with pressure predictions from the Mars Climate Database (MCD) (Forget et al., 1999; Millour et al., 2015) version 5.2, which is a climatological database derived from numerical simulations of the Martian atmosphere produced by a General Circulation Model run over several Martian years. Seasonal and daily trends in pressure data from REMS are well reproduced by the standard climatology of the MCD using its high resolution mode. This high-resolution mode extrapolates pressure values from the nominal model into the altitude of each location using a high-resolution topography model and a fine tuning of the vertical scale height that was chosen to mimic effects of slope winds not directly accounted for in the General Circulation Model on which the MCD is based. Differences between the synthetic MCD pressure data and the REMS measurements are produced by meteorological features that are identified on particular groups of sols and quantified in intensity. We show that regional dust storms outside Gale crater and dust abundance at the crater are important factors in the behaviour of the pressure exciting larger amplitudes on the daily pressure variations and causing most of the largest REMS-MCD differences. We compare the pressure signals with published data of the dust optical depth obtained by the REMS ultraviolet photodiodes and the Mastcam instrument on MSL, and with orbital images of the planet acquired by the MARCI instrument on the Mars Reconnaissance Orbiter (MRO). We show that in some cases regional dust storms induce a characteristic signature in the surface pressure measured by REMS several sols before the dust arrives to Gale crater. We explore the capability of daily pressure measurements to serve as a fast
机译:我们在火车环境监测站(REMS)仪器(REMS)仪器(Gomez-Elvira等,2012)在Mars Science实验室(MSL)虎在两个火星岁月上,研究了大气压力的记录。我们将数据与火星气候数据库(MCD)的压力预测进行比较(忘记等,1999; Millour et al。,2015)版本5.2,这是一种从一般产生的火星大气层的数值模拟导出的气候数据库流通模式在几个火星岁月内运行。通过高分辨率模式,通过MCD的标准气候学,REMS的季节性和日常趋势来自MCD的标准气候。这种高分辨率模式使用高分辨率形貌模型将来自标称模型的压力值推断到每个位置的高度,并选择垂直刻度高度的微调,选择用于斜坡风的效果而不是一般占用基于MCD的循环模型。合成MCD压力数据与REMS测量之间的差异是通过在特定溶胶组上鉴定的气象特征和强度定量的气象特征产生。我们表明,火山口外部大风陨石坑和粉尘丰富的区域尘暴是在日常压力变化上激发较大幅度的压力的行为的重要因素,并导致大多数最大的REMS-MCD差异。我们将压力信号与MSL上的MSL上获得的灰尘光学深度和MASTCAM仪器上的粉尘光学深度的发布数据进行比较,以及由MARCI仪器在火星侦察轨道器(MRO)上获取的行星轨道图像。我们表明,在某些情况下,区域沙尘暴在灰尘到达大孔陨石坑之前通过REMS几个溶胶测量​​的表面压力诱导特征签名。我们探索日常压力测量的能力作为快速

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