
© P.H. Jeffries
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© J.F.P. Galvin
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The characteristic shape of these clouds can only be seen
as a whole when viewed from a distance (top photographs).
The tops of these massive clouds show a fibrous or striated
structure that frequently resembles an anvil (2nd row left),
plume or huge mass of hair (2nd row right). They may occur
as an isolated cloud or an extensive wall (3rd row left) and
squalls, hail and/or thunder often accompany them.
Underneath the base, which is often very dark, pannus clouds
CL7 frequently form and, in storms, these may
be only a few hundred feet above the earth's surface and
they can merge to form a continuous layer. There may be
rugged cumulus (3rd row right) or a dense horizontal roll
at the shower's edge. Mamma may form, especially on the
underside of the projecting anvil (bottom left) and may
appear particularly prominent when the sun is low in the
sky. Virga may often be seen (bottom right). A whole variety
of other clouds such as dense cirrus, altocumulus, altostratus,
stratocumulus, cumulus and stratus may also be present.
If the cumulonimbus passes nearly or directly overhead,
the characteristic top is lost to view. Consequently an
observer, seeing only the under surface, may confuse it
with nimbostratus, if a watch has not been kept on the sky.
By convention, the cloud is reported as cumulonimbus if
accompanied by lightning, thunder, hail or other precipitation
of a showery nature. CL9 is used when it is impossible
to differentiate between CL3 and CL9.
Cumulonimbus most frequently develops from large cumulus
CL2. They sometimes develop from altocumulus
castellanus CM8, when the base is unusually high
and can be embedded in altostratus or nimbostratus. Cumulonimbus
can disintegrate into dense cirrus CH3.
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