activity
20082026
most citedOptimal Estimation Retrievals of the Atmospheric Structure and Composition of HD 189733b from Secondary Eclipse Spectroscopy

181 citations · 3.6k across the 98 of their papers we have counts for

collaborators
Showing 2017Show all

7 papers · 1 filter

astro-ph.EP2017★ 122 cited

Hydrogen dimers in giant-planet infrared spectra

L. N. Fletcher, M. Gustafsson, G. S. Orton

Despite being one of the weakest dimers in nature, low-spectral-resolution Voyager/IRIS observations revealed the presence of (H) dimers on Jupiter and Saturn in the 1980s.…

astro-ph.EP2017★ 13 cited

Ammonia in Jupiter's troposphere from high-resolution 5-\textmu m spectroscopy

Rohini S. Giles, Leigh N. Fletcher, Patrick G. J. Irwin +2

Jupiter's tropospheric ammonia (NH\textsubscript{3}) abundance is studied using spatially-resolved 5-\textmu m observations from CRIRES, a high resolution spectrometer at the Europ…

astro-ph.EP2017★ 28 cited

Cycles of Activity in the Jovian Atmosphere

L. N. Fletcher

Jupiter's banded appearance may appear unchanging to the casual observer, but closer inspection reveals a dynamic, ever-changing system of belts and zones with distinct cycles of a…

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…

astro-ph.EP2017★ 100 cited

Scientific rationale for Uranus and Neptune in situ explorations

O. Mousis, D. H. Atkinson, T. Cavalié +53

The ice giants Uranus and Neptune are the least understood class of planets in our solar system but the most frequently observed type of exoplanets. Presumed to have a small rocky…

astro-ph.EP2017★ 56 cited

Moist Convection and the 2010-2011 Revival of Jupiter's South Equatorial Belt

Leigh N. Fletcher, G. S. Orton, J. H. Rogers +4

The transformation of Jupiter's South Equatorial Belt (SEB) from its faded, whitened state in 2009-2010 to its normal brown appearance is documented via comparisons of thermal-infr…

astro-ph.EP2017★ 47 cited

Jovian Temperature and Cloud Variability during the 2009-2010 Fade of the South Equatorial Belt

Leigh N. Fletcher, G. S. Orton, J. H. Rogers +7

Mid-infrared 7-20 m imaging of Jupiter demonstrates that the increased albedo of Jupiter's South Equatorial Belt (SEB) during the `fade' (whitening) event of 2009-2010 was corre…