The spatial organization and time dependence of Jupiter's temperatures
near 25O-millibar pressure were measured through a jovian year by ima
ging thermal emission at 18 micrometers. The temperature field is infl
uenced by seasonal radiative forcing, and its banded organization is c
losely correlated with the visible cloud field. Evidence was found for
a quasi-periodic oscillation of temperatures in the Equatorial Zone,
a correlation between tropospheric and stratospheric waves in the Nort
h Equatorial Belt, and slowly moving thermal features in the North and
South Equatorial Belts. There appears to be no common relation betwee
n temporal changes of temperature and changes in the visual albedo of
the various axisymmetric bands.