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Re-Analysis of the Cassini RPWS/LP Data in Titan's Ionosphere : 2. Statistics on 57 Flybys
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- Chatain, A. (author)
- Univ Paris Saclay, UVSQ, CNRS, LATMOS, Guyancourt, France.;Sorbonne Univ, LPP, CNRS, Ecole Polytech,Inst Polytech Paris, Palaiseau, France.
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- Wahlund, Jan-Erik (author)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
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- Shebanits, Oleg (author)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Imperial Coll London, London, England.
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- Univ Paris Saclay, UVSQ, CNRS, LATMOS, Guyancourt, France;Sorbonne Univ, LPP, CNRS, Ecole Polytech,Inst Polytech Paris, Palaiseau, France. Institutet för rymdfysik, Uppsalaavdelningen (creator_code:org_t)
- American Geophysical Union (AGU), 2021
- 2021
- English.
- In: Journal of Geophysical Research - Space Physics. - : American Geophysical Union (AGU). - 2169-9380 .- 2169-9402. ; 126:8
- Journal article (peer-reviewed)
Abstract
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- The ionosphere of Titan hosts a complex ion chemistry leading to the formation of organic dust below 1,200 km. Current models cannot fully explain the observed electron temperature in this dusty environment. To achieve new insight, we have re-analyzed the data taken in the ionosphere of Titan by the Cassini Langmuir probe (LP), part of the Radio and Plasma Wave Science package. A first paper (Chatain et al., 2021) introduces the new analysis method and discusses the identification of four electron populations produced by different ionization mechanisms. In this second paper, we present a statistical study of the whole LP dataset below 1,200 km which gives clues on the origin of the four populations. One small population is attributed to photo- or secondary electrons emitted from the surface of the probe boom. A second population is systematically observed, at a constant density (similar to 500 cm(-3)), and is attributed to background thermalized electrons from the ionization process of precipitating particles from the surrounding magnetosphere. The two last populations increase in density with pressure, solar illumination and Extreme ultraviolet flux. The third population is observed with varying densities at all altitudes and solar zenith angles (SZA) except on the far nightside (SZA > similar to 140 degrees), with a maximum density of 2,700 cm(-3). It is therefore certainly related to the photo-ionization of the atmospheric molecules. Finally, a fourth population detected only on the dayside and below 1,200 km reaching up to 2000 cm(-3) could be photo- or thermo-emitted from dust grains.
Subject headings
- NATURVETENSKAP -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- Titan ionosphere
- dusty plasma
- Langmuir probe
- electron population
- electron temperature
- electron density
Publication and Content Type
- ref (subject category)
- art (subject category)
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