TY - JOUR
T1 - Latitudinal Temperature Variations of Jovian H+3
AU - Ballester, Gilda E.
AU - Miller, Steven
AU - Tennyson, Jonathan
AU - Trafton, Laurence M.
AU - Geballe, Thomas R.
PY - 1994
Y1 - 1994
N2 - A spectral image of Jupiter centred on 3.45 μm, taken on the night of April 2, 1992, using cooled grating spectrometer CGS4 on the United Kingdom Infrared Telescope, shows that features due to the v2 ro-vibrational band of H+3 extend right across the planet. Analysis of these features indicates that the jovian disk may be divided into three regions-two mid-high latitude regions with temperatures around 800 K and a hotter, central region with a temperature around 1200 K. The central meridian longitude of the image in the jovian System III is 102°, coinciding with the region of the Lyman-α Bulge. The significance of new work on the bulge for understanding this image is discussed. The image also shows an interesting doublet centred on 3.52 μm. Candidates for this feature are discussed; none is found to be satisfactory.
AB - A spectral image of Jupiter centred on 3.45 μm, taken on the night of April 2, 1992, using cooled grating spectrometer CGS4 on the United Kingdom Infrared Telescope, shows that features due to the v2 ro-vibrational band of H+3 extend right across the planet. Analysis of these features indicates that the jovian disk may be divided into three regions-two mid-high latitude regions with temperatures around 800 K and a hotter, central region with a temperature around 1200 K. The central meridian longitude of the image in the jovian System III is 102°, coinciding with the region of the Lyman-α Bulge. The significance of new work on the bulge for understanding this image is discussed. The image also shows an interesting doublet centred on 3.52 μm. Candidates for this feature are discussed; none is found to be satisfactory.
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U2 - 10.1006/icar.1994.1015
DO - 10.1006/icar.1994.1015
M3 - Article
AN - SCOPUS:43949160996
SN - 0019-1035
VL - 107
SP - 189
EP - 194
JO - Icarus
JF - Icarus
IS - 1
ER -