Titan's ionosphere: Model comparisons with Cassini Ta data

T. E. Cravens, I. P. Robertson, J. Clark, J. E. Wahlund, Jr H. Waite, S. A. Ledvina, H. B. Niemann, R. V. Yelle, W. T. Kasprzak, J. G. Luhmann, R. L. McNutt, W. H. Ip, V. De La Haye, I. Müller-Wodarg, D. T. Young, A. J. Coates

Research output: Contribution to journalArticle

60 Scopus citations

Abstract

On October 26, 2004, during its first encounter with Titan (Ta), the Cassini Orbiter moved from the dayside to the nightside with a closest approach altitude of 1174 km. In situ measurements of the main part of Titan's ionosphere were made by the Langmuir probe on the Cassini Radio and Plasma Wave Experiment (RPWS), while the Ion and Neutral Mass Spectrometer (INMS) measured the main constituents of the neutral atmosphere. The results of model calculations of Titan's ionosphere for Ta encounter conditions (e.g., near the terminator) are presented in this paper. The paper includes comparisons of calculated and measured electron densities along the spacecraft track. Ionization both by solar radiation and by incoming energetic electrons from Saturn's magnetosphere are needed to obtain good agreement between the measured and calculated electron densities.

Original languageEnglish (US)
Pages (from-to)1-5
Number of pages5
JournalGeophysical Research Letters
Volume32
Issue number12
DOIs
StatePublished - Jun 28 2005

ASJC Scopus subject areas

  • Geophysics
  • Earth and Planetary Sciences(all)

Fingerprint Dive into the research topics of 'Titan's ionosphere: Model comparisons with Cassini Ta data'. Together they form a unique fingerprint.

  • Cite this

    Cravens, T. E., Robertson, I. P., Clark, J., Wahlund, J. E., Waite, J. H., Ledvina, S. A., Niemann, H. B., Yelle, R. V., Kasprzak, W. T., Luhmann, J. G., McNutt, R. L., Ip, W. H., De La Haye, V., Müller-Wodarg, I., Young, D. T., & Coates, A. J. (2005). Titan's ionosphere: Model comparisons with Cassini Ta data. Geophysical Research Letters, 32(12), 1-5. https://doi.org/10.1029/2005GL023249