These, however, are superimposed on the much more sluggish circulation driven by
horizontal differences in temperature and salinity — namely, the thermohaline circulation.
Not exact matches
Because of
differences in vertical or
horizontal distribution of forcings, some changes can have a more than proportional effect on
temperatures.
Because of
differences in vertical or
horizontal distribution of forcings, some changes can have a more than proportional effect on
temperatures.
That means saturation will not have occured; the OLR brightness
temperature will be larger than the skin
temperature, though the
difference will be smaller for intensities
in nearly
horizontal directions — not just because the skin layer is colder but because some portion of the atmosphere below that is colder (the
temperature will gradually approach the skin
temperature going upward from the «photosphere» (effective emitting level) as you would call it
in analogy with the sun).
The graph has
horizontal lines drawn every 0.2 K, but the
difference in temperature rise between these two data sets isn't clearly visible on the plot.