The structure and time variability of the ring atmosphere and ionosphere

Wei-Ling Tseng, W. H. Ip, R. E. Johnson, T. A. Cassidy, M. K. Elrod

Research output: Contribution to journalArticle

35 Citations (Scopus)

Abstract

The saturnian system is subject to constant bombardment by interplanetary meteoroids and irradiation by solar UV photons. Both effects release neutral molecules from the icy ring particles either in the form of impact water vapor or gas emission in the form of H2O, O2 and H2. The observations of the Cassini spacecraft during its orbit insertion have shown the existence of molecular and atomic oxygen ions. Subsequent modeling efforts have led to the picture that an exospheric population of neutral oxygen molecules is probably maintained in the vicinity of the rings via photolytic-decomposition of ice and surface reactions. At the same time, ionized products O+ and O2+ ions move along the magnetic field lines and, depending on the optical local thickness rings, can thread through the ring plane or impact a ring particle, the ion principal sink. In addition, collisional interactions between the ions and neutrals will change the scale height of the ions and produce a scattered component of O2 molecules and O atoms which can be injected into Saturn's upper atmosphere or the inner magnetosphere. The ring atmosphere, therefore, serves as a source of O2+ ions throughout Saturn's magnetosphere. If photolysis of ice is the dominant source of O2, then the complex structure of the ring atmosphere/ionosphere and the injection rate of neutral O2 will be subject to modulation by the seasonal variation of Saturn along its orbit. In this work, we show how the physical properties of the ring oxygen atmosphere, the scattered component, and the magnetospheric O2+ ion source rate vary as the ring system goes through the cycle of solar insolation. In particular, it is shown that the magnetopheric O2+ ions should be nearly depleted at Saturn's equinox if O2 is produced mainly by photolysis of the ring material.

Original languageEnglish
Pages (from-to)382-389
Number of pages8
JournalIcarus
Volume206
Issue number2
DOIs
Publication statusPublished - 2010 Apr 1

Fingerprint

ionospheres
ionosphere
atmospheres
ion
atmosphere
rings
Saturn
photolysis
ions
oxygen
magnetosphere
magnetospheres
ice
orbit insertion
upper atmosphere
molecules
insolation
scale height
threads
meteoroids

Keywords

  • Atmosphere
  • Magnetosphere
  • Rings
  • Saturn

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Tseng, W-L., Ip, W. H., Johnson, R. E., Cassidy, T. A., & Elrod, M. K. (2010). The structure and time variability of the ring atmosphere and ionosphere. Icarus, 206(2), 382-389. https://doi.org/10.1016/j.icarus.2009.05.019

The structure and time variability of the ring atmosphere and ionosphere. / Tseng, Wei-Ling; Ip, W. H.; Johnson, R. E.; Cassidy, T. A.; Elrod, M. K.

In: Icarus, Vol. 206, No. 2, 01.04.2010, p. 382-389.

Research output: Contribution to journalArticle

Tseng, W-L, Ip, WH, Johnson, RE, Cassidy, TA & Elrod, MK 2010, 'The structure and time variability of the ring atmosphere and ionosphere', Icarus, vol. 206, no. 2, pp. 382-389. https://doi.org/10.1016/j.icarus.2009.05.019
Tseng, Wei-Ling ; Ip, W. H. ; Johnson, R. E. ; Cassidy, T. A. ; Elrod, M. K. / The structure and time variability of the ring atmosphere and ionosphere. In: Icarus. 2010 ; Vol. 206, No. 2. pp. 382-389.
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