Electron temperature of Titan's sunlit ionosphere
نویسندگان
چکیده
منابع مشابه
Unusual electron density profiles observed by Cassini radio occultations in Titans ionosphere: Effects of enhanced magnetospheric electron precipitation?
[1] The Cassini radio science facility provided 13 occultation electron density profiles of Titan during the period of 2006 and 2009. This paper presents the results of all of these occultation observations. It shows that ten of the observed electron density profiles are similar, but three are significantly different. The number of observations is relatively small for meaningful statistical con...
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Department of Physics, Imperial College, London SW7 2AZ, UK b Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721-0092, USA c School of Astronomy and Space Sciences, Nanjing University, Nanjing 210008, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China e Swedish Institute of Space Physics, Uppsala, Sweden Groupe de Spectrométrie Mol...
متن کاملEmpirical Modeling of the Total Electron Content of the Ionosphere
With the appearance of such satellite systems as GPS, GLONASS, Galileo, and others, the total electron content TEC measured by means of navigational satellites became a key parameter characterizing a state of the ionized space. In turn, functioning of navigational and telecommunication systems needs models of TEC for an estimation of accuracy of positioning, for the short-term and long-term pre...
متن کاملSunlit simulation chamber
Model-aided radiometric determination of photolysis frequencies in a sunlit atmosphere simulation chamber B. Bohn and H. Zilken Institut für Chemie und Dynamik der Geosphäre II: Troposphäre, Forschungszentrum Jülich, 52425 Jülich, Germany Zentralinstitut für Angewandte Mathematik, Forschungszentrum Jülich, 52425 Jülich, Germany Received: 3 September 2004 – Accepted: 15 October 2004 – Published:...
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-Results of electron spectrometer and cylindrical Langmuir probe measurements of ionospheric electron energy distribution in the range from about 0.2 eV to 4-0 eV are presented and discussed in this paper.
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ژورنال
عنوان ژورنال: Geophysical Research Letters
سال: 2006
ISSN: 0094-8276
DOI: 10.1029/2006gl027488