Scatterometer Climate Record Pathfinder
NSCAT Enhanced Resolution Image Product Users Notes
This page is designed as a dynamic
repository of relevant information to aid users of NSCAT enhanced
resolution image products.
Enhanced resolution images made from NSCAT data use the
Scatterometer Image Reconstruction with Filtering (SIRF)
algorithm. This version of the algorithm incoporates a median
filter and a simplified spatial response function in which the
spatial response is assumed to be 1 over the footprint and 0
elsewhere. In the processing, a linear model relating sigma-0 and
incidence angle is assumed, i.e. sigma-0(db) = A + B (theta - 40)
where A is the "incidence angle normalized sigma-0" at 40
deg incidence in dB, B is the effective incidence slope of sigma-0
versus incidence angle in dB/deg, and theta is the incidence angle
of the observation. The SIR algorithm makes images of A and B on an
4.5 km pixel grid. The effective resolution varies depending on
region and sampling conditions but is estimated to be 8-10 km in
most areas. Multiple passes of the spacecraft are combined to
produce a higher spatial resolution (at a cost of reduced temporal
resolution) and fill in coverage gaps between the individual
measurement footprints. NSCAT measurement footprints are not
contiguous and have six-sided shapes with a nominal 25 km
resolution.
NSCAT was operated continuously in double-sided mode, collecting
measurements over two 600 km wide swaths at both V and H pol. Since
only two of the antennas were operated in dual-pol mode, there are
significantly fewer H pol measurements than V pol and, in contrast
to the V pol measurements, tend to be aligned with each other and
thereby reducing the effective resolution enhancement. NSCAT
operated at 13.995 GHz. In combining the multiple passes, sigma-0 is
assumed to be independent of azimuth angle. While true for most
areas, some azimuth dependence in sigma-0 has been observed in
Antarctic firn, presumably due to sastrugi or snow dunes.
NSCAT data was obtained from the NSCAT L1.5 dataset archived at the PO.DAAC.
No recalibration has been applied.
Images are produced in the BYU .SIR file
format, using the standard naming
scheme. The files are gzipped to minimize storage and transfer
requirements. The standard images are designed for land and ice
observation and so are landmasked. However, .SIR format land mask
files (containing 0 for ocean and 1 for land) are available for each
standard region. .SIR format images containing "images" of the
latitude and longitude of each pixel for each region are also
available.
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