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researcher

C. Watkins

4 papers hereh-index 588 citations11 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP4
same name
  • C. Watkins — 43 papers, h 8
  • C. Watkins — 13 papers, h 3
  • C. Watkins — 2 papers, h 3
  • C. Watkins — 1 paper, h 1
  • C. Watkins — 1 paper, h 7
  • C. Watkins — 1 paper, h 5

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20102015
most citedIntercomparison of General Circulation Models for Hot Extrasolar Planets

66 citations · 153 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2015★ 34 cited

The EChO science case

Giovanna Tinetti, Pierre Drossart, Paul Eccleston +347

The discovery of almost 2000 exoplanets has revealed an unexpectedly diverse planet population. Observations to date have shown that our Solar System is certainly not representativ…

astro-ph.EP2013★ 66 cited

Intercomparison of General Circulation Models for Hot Extrasolar Planets

Inna Polichtchouk, James Y-K. Cho, Chris Watkins +3

We compare five general circulation models (GCMs) which have been recently used to study hot extrasolar planet atmospheres (BOB, CAM, IGCM, MITgcm, and PEQMOD), under three test ca…

astro-ph.EP2013★ 8 cited

The vertical structure of Jupiter's equatorial zonal wind above the cloud deck, derived using mesoscale gravity waves

C. Watkins, J. Y-K. Cho

Data from the Galileo Probe, collected during its descent into Jupiter's atmosphere, is used to obtain a vertical profile of the zonal wind from ∼0.5 bar (upper trop…

astro-ph.EP2010★ 45 cited

Gravity Waves on Hot Extrasolar Planets: I. Propagation and Interaction with the Background

Chris Watkins, James Y-K. Cho

We study the effects of gravity waves, or g-modes, on hot extrasolar planets. These planets are expected to possess stably-stratified atmospheres, which support gravity waves. In t…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.