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Автор Trafton, L. M.
Дата выпуска 1993
dc.description On February 15, 1992, from 0638 to 1023 UT, a single emission feature at 2.104 μm was observed over a wide area on Jupiter, covering much of the southern hemisphere. The emission was observed from the south limb to the equator along the central meridian at longitudes from 72° to 207° but appeared to be absent in the northern hemisphere. The emission was widespread in longitude, in that it was also visible at both the east and west limbs on a latitudinal chord 6 arc sec from the southern limb when the central meridian longitude was 189°–207°. The emission was not detected during the following two nights of the run. The wavelength is consistent with the l = 3 to l = 0 transition of the quasibound H<sub>2</sub> dimer double transition Q<sub>1</sub>(1) + S<sub>0</sub>(1). No other emission features were detected.
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Копирайт Copyright 1993 by the American Geophysical Union.
Тема Variable Phenomena in Jovian Planetary Systems
Тема ATMOSPHERIC COMPOSITION AND STRUCTURE
Тема Airglow and aurora
Тема IONOSPHERE
Тема Auroral ionosphere
Тема MAGNETOSPHERIC PHYSICS
Тема Auroral phenomena
Тема PLANETARY SCIENCES: FLUID PLANETS
Тема Planetology: Fluid Planets: Atmospheric composition and chemistry
Тема Planetology: Fluid Planets: Ionospheres
Название A new global‐scale emission event for Jupiter: tentative H<sub>2</sub> dimer emission at 2.104 μm on February 15, 1992
Тип article
DOI 10.1029/93JE01272
Electronic ISSN 2156-2202
Print ISSN 0148-0227
Журнал Journal of Geophysical Research: Planets
Том 98
Первая страница 18831
Последняя страница 18836
Выпуск E10
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