Dr. Paquita Zuidema
NOAA Environmental Technology Laboratory
The radiative impacts of cloud spatial inhomogeneity are not
realistically accounted for both in climate models and in the interpretation of
satellite shortwave radiance measurements. The radiative effects can vary
widely in importance depending on the underlying cloud structure. Studies employing
high-resolution cloud observations are appealing, as such studies can
realistically quantify the magnitude of a particular effect.
In this talk I will give an overview of ways in which two
instruments contribute to understanding the radiative impacts of cloud spatial
inhomogeneity. One instrument is a cloud radar, which can delineate and profile
clouds at a high spatial resolution. The top-of-cloud two-dimensional shortwave
radiation fields of marine stratocumulus clouds and tropical fair-weather
cumuli are examined. The high-quality cloud depiction allows for a thorough
evaluation of the independent pixel approximation (IPA), a popular radiative
transfer approximation in which only horizontal variations in optical depth are
taken into account. This works well at large scales (>~ 6km), e.g. for
marine stratocumulus clouds, but not at smaller scales. The IPA performs
spectacularly poorly for the tropical fair-weather cumuli. A major improvement to
IPA for broken clouds is the Tilted Independent Pixel Approximation (TIPA),
which takes the first-order contribution from the cloud sides into account.
A drawback of the cloud radar data is that it is two-dimensional, a limitation that becomes more important for broken clouds. The Multi-angle Imaging SpectroRadiometer (MISR), aboard the Terra satellite, allows the three-dimensional reconstruction of a cloud. MISR has the unique capability of measuring nine independent radiances for the same cloud scene.