Publications.
2022
[38] Ganymede's UV reflectance from Juno-UVS data (Molyneux et al., 2022)
[37] Three-dimensional structure of thermal waves in Venus' mesosphere from ground-based observations (Giles et al., 2022) [arXiv]
[36] A comprehensive set of Juno in situ and remote sensing observations of the Ganymede auroral footprint (Hue et al., 2022)
2021
[35] Local time dependence of Jupiter's polar auroral emissions observed by Juno UVS (Greathouse et al., 2021)
[34] Updated radiometric and wavelength calibration of the Juno Ultraviolet Spectrograph (UVS) (Hue et al., 2021)
[33] Meridional variations of C2H2 in Jupiter's stratosphere from Juno UVS observations (Giles et al., 2021) [arXiv]
[32] Mapping the zonal winds of Jupiter's stratospheric equatorial oscillation (Benmahi et al., 2021)
[31] Variability and hemispheric symmetry of the Pedersen conductance in the Jovian aurora (Gérard et al., 2021)
[30] Detection and characterization of circular expanding UV-emissions observed in Jupiter's polar auroral regions (Hue et al., 2021)
[29] Are Dawn Storms Jupiter's auroral substorms? (Bonfond et al., 2021)
[28] Detection of a bolide in Jupiter's atmosphere with Juno UVS (Giles et al., 2021) [arXiv]
[27] Morphology of Jupiter's polar auroral bright spot emissions via Juno-UVS observations (Haewsantati et al., 2021)
2020
[26] Spatial variations in the altitude of the CH4 homopause at Jupiter's mid-to-high latitudes, as constrained from IRTF-TEXES spectra (Sinclair et al., 2020b)
[25] Ground calibration results of the JUICE ultraviolet spectrograph (Davis et al., 2020)
[24] The effects of waves on the meridional thermal structure of Jupiter’s stratosphere (Cosentino et al., 2020)
[23] Possible Transient Luminous Events observed in Jupiter's upper atmosphere. (Giles et al., 2020b) [arXiv]
[22] A stringent upper limit of the PH3 abundance at the cloud top of Venus (Encrenaz et al., 2020b)
[21] HDO and SO2 thermal mapping on Venus. V. Evidence for a long-term anti-correlation (Encrenaz et al., 2020a)
[20] Vertically-resolved observations of Jupiter's quasi-quadrennial oscillation from 2012 to 2019 (Giles et al., 2020a) [arXiv]
[19] Spatial structure in Neptune's 7.90-μm stratospheric CH4 emission, as measured by VLT-VISIR (Sinclair et al., 2020a)
[18] Alfvénic acceleration sustains Ganymede's footprint tail aurora (Szalay et al., 2020)
[17] Long-term tracking of circumpolar cyclones on Jupiter from polar observations with JunoCam (Tabataba-Vakili et al., 2020)
2019
[16] Jupiter's atmospheric variability from longterm ground-based observations at 5 microns (Antuñano et al., 2019)
[15] A brightening of Jupiter's auroral 7.8-μm CH4 emission during a solar-wind compression (Sinclair et al., 2019)
[14] Wave activity in Jupiter’s North Equatorial Belt from near-infrared reflectivity observations (Giles et al., 2019)
[13] HDO and SO2 thermal mapping of Venus. IV. Statistical analysis of the SO2 plumes (Encrenaz et al., 2019)
2018
[12] Assessing the long-term variability of acetylene and ethane in the stratosphere of Jupiter (Melin et al., 2018)
2017
[11] Ammonia in Jupiter’s troposphere from high-resolution 5-μm spectroscopy (Giles et al., 2017b) [arXiv]
[10] Independent evolution of stratospheric temperatures in Jupiter’s northern and southern auroral regions from 2014 to 2016 (Sinclair et al., 2017)
[9] Latitudinal variability in Jupiter’s tropospheric disequilibrium species: GeH4, AsH3 and PH3 (Giles et al., 2017a) [arXiv]
[8] Moist convection and the 2010-2011 revival of Jupiter’s South Equatorial Belt (Fletcher et al., 2017b)
[7] Jupiter’s North Equatorial Belt expansion and thermal wave activity ahead of Juno’s arrival (Fletcher et al., 2017a)
2016
[6] Detection of H3+ auroral emission in Jupiter’s 5-micron window auroral emission in Jupiter’s 5-micron window (Giles et al., 2016) [arXiv]
[5] Mid-infrared mapping of Jupiter’s temperatures, aerosol opacity and chemical distributions with IRTF/TEXES (Fletcher et al., 2016)
[4] Probing Saturn’s tropospheric cloud with Cassini/VIMS (Barstow et al., 2016)
2015
[3] Cloud structure and composition of Jupiter’s troposphere from 5-μm Cassini VIMS spectroscopy (Giles et al., 2015) [arXiv]
[2] Seasonal evolution of Saturn’s polar temperatures and composition (Fletcher et al., 2015)
2014
[1] The origin of nitrogen on Jupiter and Saturn from the 15N/14N ratio (Fletcher et al., 2014)
[38] Ganymede's UV reflectance from Juno-UVS data (Molyneux et al., 2022)
[37] Three-dimensional structure of thermal waves in Venus' mesosphere from ground-based observations (Giles et al., 2022) [arXiv]
[36] A comprehensive set of Juno in situ and remote sensing observations of the Ganymede auroral footprint (Hue et al., 2022)
2021
[35] Local time dependence of Jupiter's polar auroral emissions observed by Juno UVS (Greathouse et al., 2021)
[34] Updated radiometric and wavelength calibration of the Juno Ultraviolet Spectrograph (UVS) (Hue et al., 2021)
[33] Meridional variations of C2H2 in Jupiter's stratosphere from Juno UVS observations (Giles et al., 2021) [arXiv]
[32] Mapping the zonal winds of Jupiter's stratospheric equatorial oscillation (Benmahi et al., 2021)
[31] Variability and hemispheric symmetry of the Pedersen conductance in the Jovian aurora (Gérard et al., 2021)
[30] Detection and characterization of circular expanding UV-emissions observed in Jupiter's polar auroral regions (Hue et al., 2021)
[29] Are Dawn Storms Jupiter's auroral substorms? (Bonfond et al., 2021)
[28] Detection of a bolide in Jupiter's atmosphere with Juno UVS (Giles et al., 2021) [arXiv]
[27] Morphology of Jupiter's polar auroral bright spot emissions via Juno-UVS observations (Haewsantati et al., 2021)
2020
[26] Spatial variations in the altitude of the CH4 homopause at Jupiter's mid-to-high latitudes, as constrained from IRTF-TEXES spectra (Sinclair et al., 2020b)
[25] Ground calibration results of the JUICE ultraviolet spectrograph (Davis et al., 2020)
[24] The effects of waves on the meridional thermal structure of Jupiter’s stratosphere (Cosentino et al., 2020)
[23] Possible Transient Luminous Events observed in Jupiter's upper atmosphere. (Giles et al., 2020b) [arXiv]
[22] A stringent upper limit of the PH3 abundance at the cloud top of Venus (Encrenaz et al., 2020b)
[21] HDO and SO2 thermal mapping on Venus. V. Evidence for a long-term anti-correlation (Encrenaz et al., 2020a)
[20] Vertically-resolved observations of Jupiter's quasi-quadrennial oscillation from 2012 to 2019 (Giles et al., 2020a) [arXiv]
[19] Spatial structure in Neptune's 7.90-μm stratospheric CH4 emission, as measured by VLT-VISIR (Sinclair et al., 2020a)
[18] Alfvénic acceleration sustains Ganymede's footprint tail aurora (Szalay et al., 2020)
[17] Long-term tracking of circumpolar cyclones on Jupiter from polar observations with JunoCam (Tabataba-Vakili et al., 2020)
2019
[16] Jupiter's atmospheric variability from longterm ground-based observations at 5 microns (Antuñano et al., 2019)
[15] A brightening of Jupiter's auroral 7.8-μm CH4 emission during a solar-wind compression (Sinclair et al., 2019)
[14] Wave activity in Jupiter’s North Equatorial Belt from near-infrared reflectivity observations (Giles et al., 2019)
[13] HDO and SO2 thermal mapping of Venus. IV. Statistical analysis of the SO2 plumes (Encrenaz et al., 2019)
2018
[12] Assessing the long-term variability of acetylene and ethane in the stratosphere of Jupiter (Melin et al., 2018)
2017
[11] Ammonia in Jupiter’s troposphere from high-resolution 5-μm spectroscopy (Giles et al., 2017b) [arXiv]
[10] Independent evolution of stratospheric temperatures in Jupiter’s northern and southern auroral regions from 2014 to 2016 (Sinclair et al., 2017)
[9] Latitudinal variability in Jupiter’s tropospheric disequilibrium species: GeH4, AsH3 and PH3 (Giles et al., 2017a) [arXiv]
[8] Moist convection and the 2010-2011 revival of Jupiter’s South Equatorial Belt (Fletcher et al., 2017b)
[7] Jupiter’s North Equatorial Belt expansion and thermal wave activity ahead of Juno’s arrival (Fletcher et al., 2017a)
2016
[6] Detection of H3+ auroral emission in Jupiter’s 5-micron window auroral emission in Jupiter’s 5-micron window (Giles et al., 2016) [arXiv]
[5] Mid-infrared mapping of Jupiter’s temperatures, aerosol opacity and chemical distributions with IRTF/TEXES (Fletcher et al., 2016)
[4] Probing Saturn’s tropospheric cloud with Cassini/VIMS (Barstow et al., 2016)
2015
[3] Cloud structure and composition of Jupiter’s troposphere from 5-μm Cassini VIMS spectroscopy (Giles et al., 2015) [arXiv]
[2] Seasonal evolution of Saturn’s polar temperatures and composition (Fletcher et al., 2015)
2014
[1] The origin of nitrogen on Jupiter and Saturn from the 15N/14N ratio (Fletcher et al., 2014)
