2010
DOI: 10.1016/j.icarus.2010.03.024
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High-resolution 3-μm spectra of Jupiter: Latitudinal spectral variations influenced by molecules, clouds, and haze

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Cited by 10 publications
(4 citation statements)
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References 48 publications
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“…Comparisons between our results and a representative set of observations for the depthdependent mixing ratios, for the species CH 4 , C 2 H 2 , C 2 H 4 , C 2 H 6 ,and C 4 H 2 , are shown in Figure 12. The observations for CH 4 are taken from Drossart et al (1999) and Yelle et al (1996), C 2 H 2 observations are from Fouchet et al (2000), Moses et al (2005), and Kim et al (2010), C 2 H 4 observations are from Romani et al (2008) and Moses et al (2005), C 2 H 6 observations are from Fouchet et al 2000, Moses et al (2005), Yelle et al (2001) and Kim et al (2010), and the C 4 H 2 observations are from Fouchet et al (2000) and Moses et al (2005). We also incorporate observations for C 2 H 2 , C 2 H 4 ,and C 2 H 6 from Gladstone et al (1996) and references therein.…”
Section: Jupitermentioning
confidence: 99%
“…Comparisons between our results and a representative set of observations for the depthdependent mixing ratios, for the species CH 4 , C 2 H 2 , C 2 H 4 , C 2 H 6 ,and C 4 H 2 , are shown in Figure 12. The observations for CH 4 are taken from Drossart et al (1999) and Yelle et al (1996), C 2 H 2 observations are from Fouchet et al (2000), Moses et al (2005), and Kim et al (2010), C 2 H 4 observations are from Romani et al (2008) and Moses et al (2005), C 2 H 6 observations are from Fouchet et al 2000, Moses et al (2005), Yelle et al (2001) and Kim et al (2010), and the C 4 H 2 observations are from Fouchet et al (2000) and Moses et al (2005). We also incorporate observations for C 2 H 2 , C 2 H 4 ,and C 2 H 6 from Gladstone et al (1996) and references therein.…”
Section: Jupitermentioning
confidence: 99%
“…The absolute intensities presented in Figure 1abcd were obtained from the observed fluxes of the standard stars as well as by cross-checking the previous absolute calibrations of the 3.3-m continuum levels of the non-auroral regions observed by UKIRT/CGS4 (Kim et al 2010), ISO (Kim et al 2014), and Gemini North/GNIRS (Kim et al 2015). A discussion of the uncertainties in the intensities is given below.…”
Section: ) Observations and Data Reductionmentioning
confidence: 99%
“…We derive temperatures from the rotational lines of the CH 4 bands using the following considerations. Radiative transfer programs that simulate the fluorescent emission of the 3-lm bands of CH 4 have been developed for analysis of jovian spectra (Drossart et al, 1999;Kim et al, 2009Kim et al, , 2010Kim et al, , 2014. For the CH 4 molecular line list, we adopt the HITRAN2012 database (Rothman et al, 2009).…”
Section: Observations and Data Reductionmentioning
confidence: 99%