Vibrationally excited H2 in the outer planets thermosphere

Fluorescence in the Lyman and Werner bands

Tariq Majeed, John C. McConnell, Roger Yelle

Research output: Contribution to journalArticle

30 Citations (Scopus)

Abstract

We have considered the impact of fluorescence of ground state H2 on the distribution of the vibrational levels of Ha in the upper atmospheres of Jupiter and Saturn for non-auroral latitudes. For v ≥ 3, for the conditions studied, this is the most important source of vibrationally excited H2 compared with other sources, such as photoelectron induced fluorescence, dissociative recombination of H+3 ions, and direct vibrational excitation of H2 by photoelectron impact. Combining the Voyager limb observations of H2 band emissions on Saturn, theoretical calculations of the H2 fluoresence distribution, and column constraints of Jovian H2 airglow, we estimate that some of the higher vibrational levels may have effective temperatures > 3000 K on both Jupiter and Saturn. In turn, the vibrational population of v ≥ 4 levels are sufficiently increased by the fluorescence source that the chemical sink for the ionization is enhanced. As a result, ionospheric densities may be greatly affected. We also show that the vertical ion flows induced by horizontal neutral winds or dynamo electric fields must play some role in maintaining the plasma peaks at higher altitudes.

Original languageEnglish (US)
Pages (from-to)1591-1606
Number of pages16
JournalPlanetary and Space Science
Volume39
Issue number11
DOIs
StatePublished - 1991

Fingerprint

thermosphere
Saturn
planets
fluorescence
planet
Jupiter (planet)
Jupiter
photoelectrons
airglow
ion
upper atmosphere
high altitude
limbs
sinks
ionospherics
recombination
limb
electric field
ions
ionization

ASJC Scopus subject areas

  • Geophysics
  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Vibrationally excited H2 in the outer planets thermosphere : Fluorescence in the Lyman and Werner bands. / Majeed, Tariq; McConnell, John C.; Yelle, Roger.

In: Planetary and Space Science, Vol. 39, No. 11, 1991, p. 1591-1606.

Research output: Contribution to journalArticle

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N2 - We have considered the impact of fluorescence of ground state H2 on the distribution of the vibrational levels of Ha in the upper atmospheres of Jupiter and Saturn for non-auroral latitudes. For v ≥ 3, for the conditions studied, this is the most important source of vibrationally excited H2 compared with other sources, such as photoelectron induced fluorescence, dissociative recombination of H+3 ions, and direct vibrational excitation of H2 by photoelectron impact. Combining the Voyager limb observations of H2 band emissions on Saturn, theoretical calculations of the H2 fluoresence distribution, and column constraints of Jovian H2 airglow, we estimate that some of the higher vibrational levels may have effective temperatures > 3000 K on both Jupiter and Saturn. In turn, the vibrational population of v ≥ 4 levels are sufficiently increased by the fluorescence source that the chemical sink for the ionization is enhanced. As a result, ionospheric densities may be greatly affected. We also show that the vertical ion flows induced by horizontal neutral winds or dynamo electric fields must play some role in maintaining the plasma peaks at higher altitudes.

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