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A new approach for estimating Titan's electron conductivity based on data from relaxation probe sensors on the Huygens experiment

机译:基于惠更斯实验中松弛探针传感器数据估算泰坦电子传导率的新方法

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摘要

The Huygens Probe measured the electrical conductivity of Titan atmosphere from about 140 km down to the surface, employing relaxation and mutual impedance techniques. Previous analyses have shown some differences on the conductivity measurements obtained with two independent sensors-relaxation probe (RP) and mutual impedance probe (MIP). A 20-fold maximum discrepancy occurred around the conductivity peak at 60-70 km. To understand the nature of such discrepancy, we reassess the RP data by taking into account a geometrical factor related to the electrode finite size and the Debye length of the ionized medium. The present analysis implies replacing the standard Laplace field distribution by a more elaborated model considering the Poisson equation and the resistance between the RP electrodes and the medium. Although a complete understanding of the conductivity profile is still missing, this work brings RP and MIP data to a much better agreement. The conductivity maximum difference derived from the two sensors is now lower a factor of 2. This reassessment is also useful for future instruments and missions.
机译:惠更斯探针采用松弛和互阻抗技术,测量了大约140公里至地面的泰坦大气的电导率。先前的分析表明,使用两个独立的传感器-松弛探头(RP)和互阻抗探头(MIP)获得的电导率测量值存在一些差异。在60-70 km处的电导率峰值周围出现20倍的最大差异。为了理解这种差异的性质,我们通过考虑与电极有限尺寸和电离介质的德拜长度有关的几何因素来重新评估RP数据。目前的分析意味着考虑泊松方程以及RP电极与介质之间的电阻,用更精细的模型代替标准的Laplace场分布。尽管仍然缺少对电导率分布图的完整理解,但这项工作使RP和MIP数据达到了更好的一致性。从两个传感器得出的最大电导率差现在降低了2倍。这种重新评估对于将来的仪器和任务也很有用。

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  • 来源
    《Planetary and space science 》 |2010年第15期| p.1945-1952| 共8页
  • 作者单位

    Depto. Fisica, Facultad de Quimica, Campus Espinardo, Murcia, E30100, Spain,Instituto de Astrofisica de Andaluia CSIC, P.O. Box 3004, 18080 Granada, Spain;

    Department of Mathematics and Computer Science, Royal Military College of Canada, Kingston (On.), Canada K7K 7B4;

    Instituto de Astrofisica de Andaluia CSIC, P.O. Box 3004, 18080 Granada, Spain;

    Universite Versailles St Quentin CNRS/INSU LATMOS-1PSL, UPMC, 4, place Jusssieu, Paris, France;

    RSSD, ESA-ESTEC, European Space Agency, Kepleriaan 1, 2200 AC Noordwijk, The Netherlands;

    Universite Versailles St Quentin CNRS/INSU LATMOS-1PSL, UPMC, 4, place Jusssieu, Paris, France,Depto. Fisica, Facultad de Quimica, Campus Espinardo, Murcia, E30100, Spain;

    Space Research Institute, OEAW, Schmiedlstrasse 6, 8042 Graz, Austria;

    Instituto de Astrofisica de Andaluia CSIC, P.O. Box 3004, 18080 Granada, Spain;

    RSSD, ESA-ESTEC, European Space Agency, Kepleriaan 1, 2200 AC Noordwijk, The Netherlands;

    C/SAS, C. Colombo, Universita di Padova, Via Venezia 15, 35131 Padova, Italy;

    Space Research Institute, OEAW, Schmiedlstrasse 6, 8042 Graz, Austria;

    Instituto de Astrofisica de Andaluia CSIC, P.O. Box 3004, 18080 Granada, Spain;

    Instituto de Astrofisica de Andaluia CSIC, P.O. Box 3004, 18080 Granada, Spain;

    RSSD, ESA-ESTEC, European Space Agency, Kepleriaan 1, 2200 AC Noordwijk, The Netherlands;

    Depto. Fisica, Facultad de Quimica, Campus Espinardo, Murcia, E30100, Spain;

    Institute for Aerospace Studies, University of Toronto, 4925 Dufferin Street, Toronto, Canada M3H 5T6;

    Institute for Aerospace Studies, University of Toronto, 4925 Dufferin Street, Toronto, Canada M3H 5T6;

    Depto. Fisica, Facultad de Quimica, Campus Espinardo, Murcia, E30100, Spain;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    titan; relaxation probe; atmospheric electron conductivity; space instrumentation;

    机译:泰坦松弛探针大气电子传导率太空仪器;

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