activity
20212026
most citedClaimed detection of PH in the clouds of Venus is consistent with mesospheric SO

57 citations · 153 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2026

Microwave Remote Sensing of Giant Planet Atmospheres: Considerations for Saturn and Uranus Orbiter Missions

Alex Akins, Mark Hofstadter

Microwave radiometer instruments are uniquely capable of studying volatile element abundances and heat/mass transport within the deep atmospheres of giant planets. The results of t…

astro-ph.EP2026

Can radio occultations constrain Uranus or Neptune's internal rotation periods?

Christopher R. Mankovich, Alex B. Akins, Dustin Buccino +2

The shapes of fluid planets bear the signatures of rotational flattening and atmospheric flows. Precise knowledge of their shapes and wind profiles may therefore reveal their inter…

astro-ph.EP2025

A multi-frequency global view of Callisto's thermal properties from ALMA

Maria Camarca, Katherine de Kleer, Bryan Butler +5

We present thermal observations of Callisto's leading and trailing hemispheres obtained using the Atacama Large Millimeter/submillimeter Array (ALMA) at 0.87 mm (343 GHz), 1.3 mm (…

astro-ph.EP2025★ 7 cited

Setting the Stage for Uranian Seismology from Rings and Radial Velocities

Christopher R. Mankovich, A. James Friedson, Marzia Parisi +6

A Uranus orbiter would be well positioned to detect the planet's free oscillation modes, whose frequencies can resolve questions about Uranus's weakly constrained interior. We calc…

astro-ph.EP2024

Subsurface Thermophysical Properties of Europa's Leading and Trailing Hemispheres as Revealed by ALM

A. E. Thelen, K. de Kleer, M. Camarca +4

We present best-fit values of porosity -- and the corresponding effective thermal inertiae -- determined from three different depths in Europa's near-subsurface (~1-20 cm). The por…

astro-ph.EP2023★ 19 cited

Planetary Radio Interferometry and Doppler Experiment (PRIDE) of the JUICE mission

Leonid I. Gurvits, Giuseppe Cimo, Dominic Dirkx +20

Planetary Radio Interferometry and Doppler Experiment (PRIDE) is a multi-purpose experimental technique aimed at enhancing the science return of planetary missions. The technique e…

astro-ph.EP2023★ 12 cited

Thermal properties of the leading hemisphere of Callisto inferred from ALMA observations

Maria Camarca, Katherine de Kleer, Bryan Butler +5

We present a thermal observation of Callisto's leading hemisphere obtained using the Atacama Large Millimeter/submillimeter Array (ALMA) at 0.87 mm (343 GHz). The angular resolutio…

astro-ph.EP2023★ 15 cited

Evidence of a Polar Cyclone on Uranus from VLA Observations

Alex Akins, Mark Hofstadter, Bryan Butler +4

We present observations of Uranus in northern spring with the VLA from 0.7 cm to 5 cm. These observations reveal details in thermal emission from Uranus' north pole at 10s of bars,…

astro-ph.EP2023

Approaches for Retrieving Sulfur Species Abundances from Dual X/Ka Band Radio Occultations of Venus with EnVision and VERITAS

Alex B. Akins, Tatiana M. Bocanegra-Bahamón, Kuo-Nung Wang +4

The EnVision and VERITAS missions to Venus will fly with X and Ka band telecommunications channels which can be used to conduct radio occultation studies of Venus' atmosphere. Whil…

astro-ph.EP2023★ 2 cited

Microwave Observations of Venus with CLASS

Sumit Dahal, Michael K. Brewer, Alex B. Akins +21

We report on the disk-averaged absolute brightness temperatures of Venus measured at four microwave frequency bands with the Cosmology Large Angular Scale Surveyor (CLASS). We meas…

astro-ph.EP2021★ 57 cited

Claimed detection of PH in the clouds of Venus is consistent with mesospheric SO

Andrew P. Lincowski, Victoria S. Meadows, David Crisp +7

The observation of a 266.94 GHz feature in the Venus spectrum has been attributed to PH in the Venus clouds, suggesting unexpected geological, chemical or even biological proce…

astro-ph.EP2021★ 41 cited

Complications in the ALMA Detection of Phosphine at Venus

Alex B. Akins, Andrew P. Lincowski, Victoria S. Meadows +1

Recently published ALMA observations suggest the presence of 20 ppb PH in the upper clouds of Venus. This is an unexpected result, as PH does not have a readily apparent so…