35 citations · 89 across the 4 of their papers we have counts for
7 papers
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…
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…
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…
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…
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…
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…