146 citations · 299 across the 6 of their papers we have counts for
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Highly depleted alkali metals in Jupiter's deep atmosphere
Ananyo Bhattacharya, Cheng Li, Sushil K. Atreya +12
Water and ammonia vapors are known to be the major sources of spectral absorption at pressure levels observed by the microwave radiometer (MWR) on Juno. However, the brightness tem…
Jupiter's Temperature Structure: A Reassessment of the Voyager Radio Occultation Measurements
Pranika Gupta, Sushil K. Atreya, Paul G. Steffes +12
The thermal structure of planetary atmospheres is an essential input for predicting and retrieving the distribution of gases and aerosols, as well as the bulk chemical abundances.…
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…
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…
Storms and the Depletion of Ammonia in Jupiter: II. Explaining the Juno Observations
Tristan Guillot, Cheng Li, Scott Bolton +8
Observations of Jupiter's deep atmosphere by the Juno spacecraft have revealed several puzzling facts: The concentration of ammonia is variable down to pressures of tens of bars, a…
The water abundance in Jupiter's equatorial zone
Cheng Li, Andrew Ingersoll, Scott Bolton +20
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 t…