Three Dimensional Modeling of Hot Jupiter Atmospheric Flows

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

25 pages, 6 figures, minor revisions, ApJ accepted, version with hi-res figures: http://www.astro.columbia.edu/~kristen/Hire

Scientific paper

We present a three dimensional hot Jupiter model, extending from 200 bar to 1 mbar, using the Intermediate General Circulation Model from the University of Reading. Our horizontal spectral resolution is T31 (equivalent to a grid of 48x96), with 33 logarithmically spaced vertical levels. A simplified (Newtonian) scheme is employed for the radiative forcing. We adopt a physical set up nearly identical to the model of HD 209458b by Cooper & Showman (2005,2006) to facilitate a direct model inter-comparison. Our results are broadly consistent with theirs but significant differences also emerge. The atmospheric flow is characterized by a super-rotating equatorial jet, transonic wind speeds, and eastward advection of heat away from the dayside. We identify a dynamically-induced temperature inversion ("stratosphere") on the planetary dayside and find that temperatures at the planetary limb differ systematically from local radiative equilibrium values, a potential source of bias for transit spectroscopic interpretations. While our model atmosphere is quasi-identical to that of Cooper & Showman (2005,2006) and we solve the same meteorological equations, we use different algorithmic methods, spectral-implicit vs. grid-explicit, which are known to yield fully consistent results in the Earth modeling context. The model discrepancies identified here indicate that one or both numerical methods do not faithfully capture all of the atmospheric dynamics at work in the hot Jupiter context. We highlight the emergence of a shock-like feature in our model, much like that reported recently by Showman et al. (2009), and suggest that improved representations of energy conservation may be needed in hot Jupiter atmospheric models, as emphasized by Goodman (2009).

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Three Dimensional Modeling of Hot Jupiter Atmospheric Flows does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Three Dimensional Modeling of Hot Jupiter Atmospheric Flows, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three Dimensional Modeling of Hot Jupiter Atmospheric Flows will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-620693

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.