EXCITATION TEMPERATURES DETERMINED FROM $H^{+}_{3}$ HOT BAND EMISSION IN THE JOVIAN IONOSPHERE

Loading...
Thumbnail Image

Date

1996

Journal Title

Journal ISSN

Volume Title

Publisher

Ohio State University

Research Projects

Organizational Units

Journal Issue

Abstract

Since our observation of the 3.544 $\mu$m $2v^{0}_{2}\rightarrow v_{2}$($J = 9 K=9\rightarrow J=8, G=9, U=1$) hot band transition of $H^{+}_{3}$ in the polar regions of $Jupitar,^{a}$ we have pursued the simultaneous detection of additional hot band transitions with fundamental band transitions in order to derive well determined $H^{+}_{3}$ excitation temperatures. We report 9 additional resolved $2v^{2}_{2}\rightarrow v_{2}$ and $v_{1} + v_{2}\rightarrow v_{1}$ hot band transitions observed in emission at 3.52, 3.63, 3.66, and 3.84 $\mu$m. The hot band transitions have thus far only been detected in the polar regions, with the occasional exception being the 3.544 $\mu$m $2v_{0}^{2}\rightarrow v_{2}$ transition around $45^{\prime}$ S latitude during the 1994 Comet Shoemaker Levy-9 encounter. Temporal and spatial variation of the excitation temperatures as well as their dependence on vibrational mode will be presented. Anomalous line intensities, e.g. $^{r}R(3,3)^{-b}$, will also be discussed. All observations were made with the CGS4 spectrometer at the United Kingdom Infrared Telescope on Mauna Kea, Hawaii.

Description

$^{a}$T. R. Geballe, M.-F. Jagod, and T. Oka, Astrophys, J. 408, L109-L112 (1993).$^{b}$J.-P. Maillard, P. Drossart, J. K. G. Watson, S. J. Kim, J. Caldwell, Astrophys. J. 363, L37-L41 (1990).
Author Institution: Department of Chemistry, Department of Astronomy and Astrophysics, and the Enrico Fermi Institute, The University of Chicago; Department of Chemistry, Department of Astronomy and Astrophysics, and the Enrico Fermi Institute, Joint Astronomy Centre

Keywords

Citation