Multiple‐wavelength sensing of Jupiter during the Juno mission's first perijove passage
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Shannon T. Brown | A. Ingersoll | G. Orton | M. Caplinger | C. Hansen | A. Adriani | S. Atreya | A. Mura | D. Grassi | M. Moriconi | S. Bolton | S. Levin | G. Sindoni | T. Momary | M. Janssen | J. Arballo | Chao Li
[1] G. Piccioni,et al. JIRAM, the Jovian Infrared Auroral Mapper , 2017 .
[2] Andrew P. Ingersoll,et al. Junocam: Juno’s Outreach Camera , 2017 .
[3] Shannon T. Brown,et al. The distribution of ammonia on Jupiter from a preliminary inversion of Juno microwave radiometer data , 2017 .
[4] A. Ingersoll,et al. Characterization of the white ovals on Jupiter's southern hemisphere using the first data by the Juno/JIRAM instrument , 2017 .
[5] A. Ingersoll,et al. Preliminary results on the composition of Jupiter's troposphere in hot spot regions from the JIRAM/Juno instrument , 2017 .
[6] R. Williamson,et al. MWR: Microwave Radiometer for the Juno Mission to Jupiter , 2017 .
[7] L. Fletcher,et al. Latitudinal variability in Jupiter's tropospheric disequilibrium species: GeH4, AsH3 and PH3 , 2016, 1610.09073.
[8] G. Orton,et al. Jupiter's Para-H2 Distribution from SOFIA/FORCAST and Voyager/IRIS 17-37 µm Spectroscopy , 2016, 1610.01304.
[9] T. Encrenaz,et al. Mid-infrared mapping of Jupiter’s temperatures, aerosol opacity and chemical distributions with IRTF/TEXES , 2016, 1606.05498.
[10] D. DeBoer,et al. Peering through Jupiter’s clouds with radio spectral imaging , 2016, Science.
[11] I. Pater,et al. JUPITER’S DEEP CLOUD STRUCTURE REVEALED USING KECK OBSERVATIONS OF SPECTRALLY RESOLVED LINE SHAPES , 2015, 1508.04795.
[12] R. West,et al. Stratospheric aerosols on Jupiter from Cassini observations , 2013 .
[13] H. Hammel,et al. Keck adaptive optics images of Jupiter’s north polar cap and Northern Red Oval , 2011 .
[14] Michael H. Wong,et al. Persistent rings in and around Jupiter's anticyclones - Observations and theory , 2010 .
[15] G. Piccioni,et al. Jupiter’s hot spots: Quantitative assessment of the retrieval capabilities of future IR spectro-imagers , 2010 .
[16] Bryan M. Karpowicz,et al. A new model of the hydrogen and helium-broadened microwave opacity of ammonia based on extensive laboratory measurements , 2008 .
[17] T. Owen,et al. Updated Galileo probe mass spectrometer measurements of carbon, oxygen, nitrogen, and sulfur on Jupiter , 2004 .
[18] J. Burns,et al. Cassini Imaging of Jupiter's Atmosphere, Satellites, and Rings , 2003, Science.
[19] John T. Rayner,et al. SpeX: A Medium‐Resolution 0.8–5.5 Micron Spectrograph and Imager for the NASA Infrared Telescope Facility , 2003 .
[20] R. Carlson,et al. The Origin of Belt/Zone Contrasts in the Atmosphere of Jupiter and Their Correlation with 5-μm Opacity , 2001 .
[21] W. Folkner,et al. Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signal , 1998 .
[22] Jelena Tesic,et al. Characteristics of the Galileo Probe Entry Site From Earth-Based Remote Sensing Observations , 1998 .
[23] G. Orton,et al. Evolution and persistence of 5‐μm hot spots at the Galileo probe entry latitude , 1998 .
[24] C. Sobeck,et al. Galileo Probe: In Situ Observations of Jupiter's Atmosphere , 1996, Science.
[25] P. Drossart,et al. Earth-Based Observations of the Galileo Probe Entry Site , 1996, Science.
[26] P. Gierasch,et al. Global variation of the para hydrogen fraction in Jupiter's atmosphere and implications for dynamics on the outer planets , 1984 .
[27] R. Terrile,et al. Colors on Jupiter , 1981 .
[28] JOHN S. Lewis,et al. Chemical structure of the deep atmosphere of Jupiter , 1978 .
[29] J. Westphal,et al. The vertical cloud structure of Jupiter from 5 μm measurements , 1977 .
[30] F. O. Rice. Colors on Jupiter , 1956 .