On pressure measurement and seasonal pressure variations during the Phoenix mission

[1] In situ surface pressures measured at 2 s intervals during the 150 sol Phoenix mission are presented and seasonal variations discussed. The lightweight Barocap®/Thermocap® 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°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.

[1]  David C. Catling,et al.  Temperature, pressure, and wind instrumentation in the Phoenix meteorological package , 2008 .

[2]  Larry W. Esposito,et al.  Meteorological observations on Martian surface: met-packages of Mars-96 Small Stations and Penetrators , 1998 .

[3]  Paul S. Smith,et al.  Winds at the Phoenix landing site , 2010 .

[4]  J. McConnell,et al.  A new model for multiscale modeling of the Martian atmosphere, GM3 , 2005 .

[5]  S. Larsen,et al.  The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment. , 1997, Science.

[6]  R. M. Henry,et al.  Frontal systems during passage of the Martian north polar hood over the Viking Lander 2 site prior to the first 1977 dust storm , 1979 .

[7]  Kevin Hamilton,et al.  Comprehensive Model Simulation of Thermal Tides in the Martian Atmosphere , 1996 .

[8]  S. Larsen,et al.  Telltale wind indicator for the Mars Phoenix lander , 2008 .

[9]  M. D. Ellehoj,et al.  Phoenix Mars Lander: Vortices and Dust Devils at the Landing Site , 2008 .

[10]  J. Tillman Mars global atmospheric oscillations - Annually synchronized, transient normal-mode oscillations and the triggering of global dust storms , 1988 .

[11]  P. Taylor,et al.  Initial analysis of air temperature and related data from the Phoenix MET station and their use in estimating turbulent heat fluxes , 2010 .

[12]  M. Richardson,et al.  The Martian Atmosphere During the Viking Mission, I Infrared Measurements of Atmospheric Temperatures Revisited , 2000 .

[13]  A. Harri,et al.  Aspects of atmospheric science and instrumentation for martian missions , 1995 .

[14]  Peter Guttorp,et al.  The Martian annual atmospheric pressure cycle: Years without great dust storms , 1993 .

[15]  R. M. Henry,et al.  The annual cycle of pressure on Mars measured by Viking landers 1 and 2 , 1980 .