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A revised calibration function and results for the Phoenix mission TECP relative humidity sensor

机译:凤凰城任务TECP相对湿度传感器的校准功能和结果的修订

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abstract_textpA new calibration function for the humidity sensor in the Thermal and Electrical Conductivity Probe (TECP) on the Phoenix (PHX) Mars mission has been developed. Two changes are incorporated: (1) it is now cast in terms of frost point (T-f) rather than relative humidity (RH), and (2) flight data, taken when the atmosphere is independently known to be saturated, are included in the calibration data set. Daytime (6: 00 h-19: 00 h) frost points ranged from 194 K to 209 K; the nighttime frost point ranged from 179 K to 206 K. The response of the sensor was smooth and continuous throughout. Daytime humidity exhibited large, high-frequency variance driven by turbulence, whereas nighttime humidity varied smoothly with the temperature of the atmosphere. Nighttime saturation of the atmosphere begins at L-s 101 degrees, (Martian solar day (sol) 55), which is earlier than reported by either Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) or solid-state imager (SSI). Early mornings are the most humid part of the sol after L-s 113 degrees (sol 80), due to sublimation of surface ice that precipitates overnight. H2O is removed from the atmosphere into the regolith, mostly during the late afternoon, although this continues into the evening. The ground ice exposed by Phoenix operations masks the naturally occurring process in the early evening and may cause the atmosphere immediately around the lander to saturate somewhat earlier in the evening than it otherwise would have. The average H2O vapor density is close to the summertime value expected for equilibrium with ground ice. A discrepancy between the H2O column calculated from TECP data and the column measured by CRISM and SSI is likely due to comparable timescales between turbulent mixing through the planetary boundary layer and adsorptive drawdown of H2O. We find that RH is mostly 5 (daytime) or 95 (nighttime), and the transition between the two extremes is extremely rapid./p/abstract_text
机译:凤凰号(PHX)火星任务中的热导率和电导率探头(TECP)中的湿度传感器的新校准功能已经开发出来。包含两个变化:(1)它现在是根据霜点(T-f)而不是相对湿度(RH)来铸造的,以及(2)当独立已知大气饱和时获取的飞行数据包含在校准数据集中。白天(6:00 h-19:00 h)霜点范围为194 K至209 K;夜间霜点在179 K至206 K之间。传感器的响应自始至终都是平稳和连续的。湍流驱动的白天湿度表现出较大的高频变化,而夜间湿度随大气温度的变化而平滑变化。大气的夜间饱和度从L-s 101度开始,(火星太阳日(sol)55),这比火星紧凑型侦察成像光谱仪(CRISM)或固态成像仪(SSI)报告的要早。清晨是 L-s 113 度(sol 80)之后最潮湿的部分,这是由于地表冰在一夜之间降水。H2O从大气中进入风化层,主要是在下午晚些时候,尽管这种情况一直持续到晚上。凤凰号作业暴露的地面冰掩盖了傍晚自然发生的过程,并可能导致着陆器周围的大气在傍晚比原本更早饱和。平均H2O蒸气密度接近与地面冰平衡的夏季预期值。根据TECP数据计算出的H2O色谱柱与CRISM和SSI测得的色谱柱之间存在差异,这可能是由于通过行星边界层的湍流混合与H2O的吸附下降之间的时间尺度相当。我们发现相对湿度大多95%(夜间),两个极端之间的转换非常迅速。

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