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1 to 10 of 13 Results
May 12, 2021
Glenn Orton, 2021, "Longitudinal Variations in the Stratosphere of Uranus from the Spitzer Infrared Spectrometer", https://doi.org/10.48577/jpl.QLS7MP, Icarus, JPL Open Repository
NASA’s Spitzer Infrared Spectrometer (IRS) acquired mid-infrared (5-37 m) disc-averaged spectra of Uranus very near to its equinox in December 2007. A mean spectrum was constructed from observations of multiple central meridian longitudes, spaced equally around the planet, which...
May 3, 2021
Glenn Orton, 2021, "Fluctuations in the reversal of Jupiter’s stratospheric jet streams", https://doi.org/10.48577/jpl.AFZ3AF, Nature Astronomy, JPL Open Repository
Solar System planetary atmospheres, from the terrestrial planets to the giants, display a banded structure of winds and temperatures over a wide range of altitudes. The equatorial stratospheres of the Earth, Jupiter, and Saturn all exhibit a remarkable periodic oscillation of the...
Mar 15, 2021
Glenn Orton, 2021, "Ice Giant Circulation Patterns: Implications for Atmospheric Probes", https://doi.org/10.48577/jpl.I9NWVT, Space Science Reviews, JPL Open Repository
Atmospheric circulation patterns derived from multi-spectral remote sensing can serve as a guide for choosing a suitable entry location for a future in situ probe mission to the Ice Giants. Since the Voyager-2 flybys in the 1980s, three decades of observations from ground- and sp...
Mar 15, 2021
Glenn Orton, 2021, "On the clouds and ammonia in Jupiter’s upper troposphere from Juno JIRAM reflectivity observations", https://doi.org/10.48577/jpl.VAGMDC, Monthly Notices of the Royal Astronomical Society, JPL Open Repository
We analyse spectra measured by the Jovian Infrared Auroral Mapper (JIRAM, a payload element of the NASA Juno mission) in the 3150-4910 cm-1 (2.0-3.2 μm) range during the perijiove passage of August 2016. Despite modelling uncertainties, the quality and the relative uniformity of...
Mar 15, 2021
Glenn Orton, 2021, "The water abundance in Jupiter’s equatorial zone", https://doi.org/10.48577/jpl.GANDGA, Nature Astronomy, JPL Open Repository
Oxygen is the most common element after hydrogen and helium in Jupiter’s atmosphere, and may have been the primary condensable (as water ice) in the protoplanetary disk. Prior to the Juno mission, in situ measurements of Jupiter’s water abundance were obtained from the Galileo pr...
Mar 15, 2021
Glenn Orton, 2021, "Jupiter’s Great Red Spot: Strong interactions with incoming anticyclones in 2019", https://doi.org/10.48577/jpl.PFAQZH, Journal of Geophysical Research: Planets, JPL Open Repository
Jupiter’s Great Red Spot (GRS), a giant anticyclone, is the largest and longest-lived of all the vortices observed in planetary atmospheres. During its history, the GRS has shrunk to half its size since 1879, and encountered many smaller anticyclones and other dynamical features...
Mar 11, 2021
Glenn Orton, 2021, "Constraints on Neptune’s haze structure and formation from VLT observations in the H-band", https://doi.org/10.48577/jpl.DPF0PT, Icarus, JPL Open Repository
A 1-dimensional microphysics model has been used to constrain the structure and formation of haze in Neptune’s atmosphere. These simulations were coupled to a radiative-transfer and retrieval code (NEMESIS) to model spectral observations of Neptune in the H-band performed by the...
Mar 11, 2021
Glenn Orton, 2021, "Turbulence Power Spectra in Regions Surrounding Jupiter's South Polar Cyclones From Juno/JIRAM", https://doi.org/10.48577/jpl.MHJISV, Journal of Geophysical Research: Planets, JPL Open Repository
We present a power spectral analysis of two narrow annular regions near Jupiter's South Pole derived from data acquired by the Jovian Infrared Auroral Mapper instrument onboard NASA's Juno mission. In particular, our analysis focuses on the data set acquired by the Jovian Infrare...
Mar 11, 2021
Glenn Orton, 2021, "Jupiter's Equatorial Plumes and Hot Spots: Spectral 2 Mapping from Gemini/TEXES and Juno/MWR", https://doi.org/10.48577/jpl.DTUSQW, Journal of Geophysical Research: Planets, JPL Open Repository
We present multi-wavelength measurements of the thermal, chemical, and cloud contrasts associated with the visibly dark formations (also known as 5-m hot spots) and intervening bright plumes on the boundary between Jupiter's Equatorial Zone (EZ) and North Equatorial Belt (NEB)....
Mar 11, 2021
Glenn Orton, 2021, "Vertically-resolved observations of Jupiter’s quasi-quadrennial oscillation from 2012 to 2019", https://doi.org/10.48577/jpl.F4AGDI, Icarus, JPL Open Repository
Over the last eight years, a rich dataset of mid-infrared CH4 observations from the TEXES instrument at IRTF has been used to characterize the thermal evolution of Jupiter’s stratosphere. These data were used to produce vertically-resolved temperature maps between latitudes of 50...
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