PLOTS FOR ZONAL MEAN GROUP

MARS GRANADA WORKSHOP, JANUARY 2003

Last updated: 1/8/2003
Alison F.C. Bridger


All plots are based on 30 sol-averaged fields, unless otherwise stated. As much as possible, all like-runs have the same attributes. For example, the low dust runs ideally all have the same visible opacity with temporally- and spatially-fixed dust having the same vertical decay profiles etc.

As of noon on Jan 8, it's beginning to look unlikely that I'll have time to get streamfunction plots created and loaded :-(


GROUP CLEAR LOW DUST HIGH DUST "REAL" DUST

Ames

tau=0 temperatures, winds
tau=0.3 temperatures, winds

tau=1.0 temperatures, winds
tau=MGS temperatures, winds

Comparisons

. temperature comparisons at Ls 90 (postscript)
temperature comparisons at Ls 180 (postscript)
temperature comparisons at Ls 270 (postscript)
temperature comparisons at Ls 360 (postscript)
. TES temperatures
(postscript)

France

tau=0 temperatures, winds
tau=0.2 temperatures, winds

tau=2.0 temperatures, winds
tau=MGS temperatures, winds

GFDL


(5 sol-averages)
tau=0 temperatures, winds
tau=0.3 temperatures, winds

tau=1.0 temperatures, winds
pending

Japan

tau=0 temperatures, winds
tau=0.3 temperatures, winds

pending pending

Oxford

tau=0 temperatures, winds
tau=0.2 temperatures, winds

tau=1.0 temperatures, winds
tau=MGS temperatures, winds