Cloud Streets in Satellite
Imagery
Dr. Brad Muller
Cloud streets are lines
of
relatively low-level
cumulus
or towering cumulus clouds that tend to line up with the
wind direction
or with the wind shear vector. According to Conway
(1997), they
line up with the wind direction during their early stages of
formation;
farther down wind they are aligned more with the wind shear,
rather
than the wind direction itself (see Figs. 7.1-7.5).
They are an example of horizontal roll convection, that is,
buoyantly rising air organizing into parallel, horizontal
rolling motions in the atmosphere:
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They typically form under two different weather regimes that
produce
low-level convection:
(1) during the cold season when cold air moves over
relatively warmer
water, destabilizing the lower air layers and producing
lines of
convective clouds that usually are limited in vertical
extent by a
temperature inversion. Because they do not have high,
cold tops,
they do not appear bright on IR imagery.
They often can be seen off the east coast of the U.S. after
a frontal
passage during a cold air outbreak with northwesterly
offshore
flow. They also often can be seen over the Gulf of
Mexico after a
strong cold frontal passage, and over the Great Lakes during
synoptic
weather patterns that produce "lake
effect" snow
.
(2) During the warm season, cloud streets often can be seen
over land
surfaces as the sun heats up the ground producing cumulus
clouds that
more or less line up with the wind direction.
They are frequently seen during the warmer months over
Florida, Texas, and much of the southeastern U.S. They
are common
almost any time of year over the Yucatan Peninsula.
A related phenomenon can often be seen in weather radar
"clear air echoes" of horizontal convective rolls:
From Wilson et al., 1994:
https://doi.org/10.1175/1520-0426(1994)011%3C1184:BLCARE%3E2.0.CO;2