The 3 $\mu$m region of ethane, propane and propene contains a number of vibrational modes dominated by various C-H stretches. Transmission spectra for these hydrocarbons have been obtained at high resolution (0.005 \wn) and at elevated temperatures (up to 773 K). The integrated absorption cross sections over the isolated 3 $\mu$m region are calibrated to those from the Pacific Northwest National Laboratory (PNNL) in order to obtain an effective pressure for the sample. With the Jovian Infrared Auroral Mapper (JIRAM on Juno) due to arrive at Jupiter in July 2016, these cross sections will find use in the study of hot emission from hydrocarbons in the auroral regions of Jupiter. They are also appropriate for modeling atmospheres of hot Jupit...
In this paper we report the mapping of H3+, C2H2, and CH4 as derived by an unexploited Galileo/Near-...
Auroral processes are evident in Jupiter's polar atmosphere over a large range in wavelength (X-ray ...
The hydrocarbon photochemistry in the upper atmosphere of Jupiter is investigated using a one-dimens...
The 3 $\mu$m region of ethane, propane and propene contains a number of vibrational modes dominated ...
Propane is one of several hydrocarbons present in the atmospheres of the Giant Planets, Jupiter and ...
Absorption cross sections for a range of small hydrocarbons, from C2-C4, in the far and mid IR spec...
High-resolution infrared absorption cross sections are presented for the $nu_{9}$ band of ethane (C$...
Hydrocarbons are of considerable importance in studies of planetary atmospheres such as Titan and Gi...
Hydrocarbons are of considerable importance in studies of planetary atmospheres such as Titan and Gi...
We compute models of the transmission spectra of planets HD 209458b, HD 189733b, and generic hot Jup...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
International audienceWe report on spectro-imaging infrared observations of Jupiter's auroral zones,...
Spectral observations of Jupiter's far-ultraviolet (FUV) auroral emissions are commonly used to dete...
We have constructed a model of the Jovian ionosphere that includes direct photoionization of hydroca...
9 pages, 12 figuresInternational audienceUV absorption cross sections are an essential ingredient of...
In this paper we report the mapping of H3+, C2H2, and CH4 as derived by an unexploited Galileo/Near-...
Auroral processes are evident in Jupiter's polar atmosphere over a large range in wavelength (X-ray ...
The hydrocarbon photochemistry in the upper atmosphere of Jupiter is investigated using a one-dimens...
The 3 $\mu$m region of ethane, propane and propene contains a number of vibrational modes dominated ...
Propane is one of several hydrocarbons present in the atmospheres of the Giant Planets, Jupiter and ...
Absorption cross sections for a range of small hydrocarbons, from C2-C4, in the far and mid IR spec...
High-resolution infrared absorption cross sections are presented for the $nu_{9}$ band of ethane (C$...
Hydrocarbons are of considerable importance in studies of planetary atmospheres such as Titan and Gi...
Hydrocarbons are of considerable importance in studies of planetary atmospheres such as Titan and Gi...
We compute models of the transmission spectra of planets HD 209458b, HD 189733b, and generic hot Jup...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
International audienceWe report on spectro-imaging infrared observations of Jupiter's auroral zones,...
Spectral observations of Jupiter's far-ultraviolet (FUV) auroral emissions are commonly used to dete...
We have constructed a model of the Jovian ionosphere that includes direct photoionization of hydroca...
9 pages, 12 figuresInternational audienceUV absorption cross sections are an essential ingredient of...
In this paper we report the mapping of H3+, C2H2, and CH4 as derived by an unexploited Galileo/Near-...
Auroral processes are evident in Jupiter's polar atmosphere over a large range in wavelength (X-ray ...
The hydrocarbon photochemistry in the upper atmosphere of Jupiter is investigated using a one-dimens...