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首页> 外文期刊>Planetary and space science >Exploiting night-time averaged spectra from PFS/MEX shortwave channel. Part 2: Near-surface CO retrievals
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Exploiting night-time averaged spectra from PFS/MEX shortwave channel. Part 2: Near-surface CO retrievals

机译:利用PFS / MEX短波通道的夜间平均光谱。第2部分:近地面CO检索

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Because of its important role in the Martian carbon cycle, carbon monoxide (CO) has been the subject of many measurements from ground and from space. Daytime measurements have been mostly exploited to measure the CO abundance because of their good signal-to-noise ratio, but night-time observations have not been documented yet. We demonstrate here the possibility of using PFS (Planetary Fourier Spectrometer) night-time observations to measure the Martian CO abundance. More particularly in this paper, we show that measuring CO during night with PFS can be achieved by averaging a large number of spectra to reach sufficient signal-to-noise. Furthermore, we show that the number of averaged spectra is not the only driving parameter for the detection of CO. High surface temperatures and high thermal contrast (negative in our case) are the two other conditions required for the measurement of the night-time CO abundance. Because of this, the retrievals are especially successful in the Southern Hemisphere during spring and summer when and where these two conditions are met. For night-time spectra with a positive detection, CO vertical profiles are successfully retrieved using the Optimal Estimation method and are characterized in terms of vertical sensitivity. Successful retrievals imply the use of accurate temperature profiles, and in particular an appropriate representation of the thermal inversion in the lower atmosphere. The temperature was obtained by using the relevant information from the CO2 nu(3) band (Bauduin et al., 2020, this issue). A complete error budget of the retrieved CO profiles is also performed and includes different sources of uncertainty. Although the retrieved profiles are not resolved vertically, we show in particular that night-time PFS observations carry information mostly on the CO abundance for the 0-10 km altitude region, and thus provide a stronger constraint on the near-surface CO abundance compared to daytime observations.
机译:由于其在火星碳循环中的重要作用,一氧化碳(CO)一直是从地面和空间进行许多测量的主题。由于其良好的信噪比,日间测量主要被利用来测量CO丰富,但尚未记录夜间观察。我们展示了使用PFS(行星傅里叶谱仪)夜间观察来测量火星Co丰富的可能性。更具体地,在本文中,我们示出了通过平均大量光谱来达到足够的信噪比,可以实现在夜间用PFS期间的测量CO。此外,我们表明平均光谱的数量不是用于检测CO的唯一驱动参数。高表面温度和高热对比(在我们的情况下负)是夜间CO测量所需的两个其他条件丰富。因此,在春季和夏季何时何地满足这两个条件时,检索在南半球尤其成功。对于具有阳性检测的夜间光谱,使用最佳估计方法成功检索CO垂直轮廓,并以垂直灵敏度为特征。成功的检索意味着使用精确的温度曲线,特别是在低层大气中的热反转的适当表示。通过使用来自CO2 NU(3)频段的相关信息(Bauduin等,2020,这个问题)获得的温度。还执行了检索到的CO配置文件的完整错误预算,并包括不同的不确定性源。虽然检索的概况垂直解,但特别说明,夜间PFS观察主要在0-10公里高度区域的CO丰富上携带信息,从而为近表面共同提供了更强的限制白天观察。

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