On pressure measurement and seasonal pressure variations during the Phoenix mission

被引:31
|
作者
Taylor, Peter A. [1 ]
Kahanpaa, Henrik [4 ]
Weng, Wensong [1 ]
Akingunola, Ayodeji [2 ]
Cook, Clive [1 ]
Daly, Mike [3 ]
Dickinson, Cameron [1 ]
Harri, Ari-Matti [4 ]
Hill, Darren [3 ]
Hipkin, Victoria [2 ]
Polkko, Jouni [4 ]
Whiteway, Jim [1 ]
机构
[1] York Univ, Ctr Res Earth & Space Sci, N York, ON M3J 1P3, Canada
[2] Canadian Space Agcy, St Hubert, PQ J3Y 8Y9, Canada
[3] MDA, Brampton, ON L6S 4J3, Canada
[4] Finnish Meteorol Inst, FI-00101 Helsinki, Finland
关键词
MARTIAN ATMOSPHERE; DUST STORMS; CYCLE;
D O I
10.1029/2009JE003422
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
In situ surface pressures measured at 2 s intervals during the 150 sol Phoenix mission are presented and seasonal variations discussed. The lightweight Barocap (R)/Thermocap (R) pressure sensor system performed moderately well. However, the original data processing routine had problems because the thermal environment of the sensor was subject to more rapid variations than had been expected. Hence, the data processing routine was updated after Phoenix landed. Further evaluation and the development of a correction are needed since the temperature dependences of the Barocap sensor heads have drifted after the calibration of the sensor. The inaccuracy caused by this appears when the temperature of the unit rises above 0 degrees C. This frequently affects data in the afternoons and precludes a full study of diurnal pressure variations at this time. Short-term fluctuations, on time scales of order 20 s are unaffected and are reported in a separate paper in this issue. Seasonal variations are not significantly affected by this problem and show general agreement with previous measurements from Mars. During the 151 sol mission the surface pressure dropped from around 860 Pa to a minimum (daily average) of 724 Pa on sol 140 (Ls 143). This local minimum occurred several sols earlier than expected based on GCM studies and Viking data. Since battery power was lost on sol 151 we are not sure if the timing of the minimum that we saw could have been advanced by a low-pressure meteorological event. On sol 95 (Ls 122), we also saw a relatively low pressure feature. This was accompanied by a large number of vertical vortex events, characterized by short, localized (in time), low-pressure perturbations.
引用
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页数:11
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