activity
20172024
most citedFirst ALMA Millimeter Wavelength Maps of Jupiter, with a Multi-Wavelength Study of Convection

44 citations · 227 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2024★ 30 cited

Infrared Characterisation of Jupiter's Equatorial Disturbance Cycle

Arrate Antuñano, Leigh N. Fletcher, Glenn S. Orton +6

We use an infrared dataset captured between 1984 and 2017 using several instruments and observatories to report five rare equatorial disturbances that completely altered the appear…

astro-ph.EP2024★ 1 cited

Investigating Thermal Contrasts Between Jupiter's Belts, Zones, and Polar Vortices with VLT/VISIR

Deborah Bardet, Padraig T. Donnelly, Leigh N. Fletcher +8

Using images at multiple mid-infrared wavelengths, acquired in May 2018 using the VISIR instrument on ESO's Very Large Telescope (VLT), we study Jupiter's pole-to-pole thermal, che…

astro-ph.EP2022★ 21 cited

Unexpected Long-Term Variability in Jupiter's Tropospheric Temperatures

Glenn S. Orton, Arrate Antunano, Leigh N. Fletcher +9

An essential component of planetary climatology is knowledge of the tropospheric temperature field and its variability. Previous studies of Jupiter hinted at periodic behavior that…

astro-ph.EP2021★ 3 cited

Refining Saturn's deuterium-hydrogen ratio via IRTF/TEXES spectroscopy

James S. D. Blake, Leigh N. Fletcher, Thomas K. Greathouse +7

The abundance of deuterium in giant planet atmospheres provides constraints on the reservoirs of ices incorporated into these worlds during their formation and evolution. Motivated…

astro-ph.EP2019★ 44 cited

First ALMA Millimeter Wavelength Maps of Jupiter, with a Multi-Wavelength Study of Convection

Imke de Pater, R. J. Sault, Chris Moeckel +15

We obtained the first maps of Jupiter at 1-3 mm wavelength with the Atacama Large Millimeter/Submillimeter Array (ALMA) on 3-5 January 2017, just days after an energetic eruption a…

astro-ph.EP2019★ 23 cited

Jupiter's Atmospheric Variability from Long-Term Ground-based Observations at 5 microns

Arrate Antuñano, Leigh N. Fletcher, Glenn S. Orton +7

Jupiter's banded structure undergoes strong temporal variations, changing the visible and infrared appearance of the belts and zones in a complex and turbulent way due to physical…

astro-ph.EP2018★ 19 cited

Jupiter's Mesoscale Waves Observed at 5 m by Ground-Based Observations and Juno JIRAM

L. N. Fletcher, H. Melin, A. Adriani +12

We characterise the origin and evolution of a mesoscale wave pattern in Jupiter's North Equatorial Belt (NEB), detected for the first time at 5 m using a 2016-17 campaign of `lu…

astro-ph.EP2018★ 33 cited

Assessing the long-term variability of acetylene and ethane in the stratosphere of Jupiter

Henrik Melin, L. N. Fletcher, P. T. Donnelly +6

Acetylene (CH) and ethane (CH) are both produced in the stratosphere of Jupiter via photolysis of methane (CH). Despite this common source, the latitudinal dist…

astro-ph.EP2017★ 18 cited

The quest for H at Neptune: deep burn observations with NASA IRTF iSHELL

H. Melin, L. N. Fletcher, T. S. Stallard +4

Emission from the molecular ion H is a powerful diagnostic of the upper atmosphere of Jupiter, Saturn, and Uranus, but it remains undetected at Neptune. In search of this emi…

astro-ph.EP2017★ 35 cited

Jupiter's North Equatorial Belt expansion and thermal wave activity ahead of Juno's arrival

L. N. Fletcher, G. S. Orton, J. A. Sinclair +13

The dark colors of Jupiter's North Equatorial Belt (NEB, N) appeared to expand northward into the neighboring zone in 2015, consistent with a 3-5 year cycle of activity…