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Summary:
The Visible Infrared Spin-Scan Radiometer (VISSR)
is an imaging device used for two-dimensional,
cloud cover pictures from a geosynchronous
altitude. This instrument provides for the both day
and night time observations of clouds and the
determination of temperatures, cloud heights and
wind fields. The VISSR instrument consists of a
scanning system, a telescope, and Infrared and
Visible sensors.
A VISSR instrument flies aboard the
Geostationary Operational Environmental Satellites
(GOES), the Geostationary Meteorological Satellite
(GMS) and the Meteorological Satellites (Meteosat).
In general, the instrumentation design and
operation are similar among all three
platforms.
Table of Contents:
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Visible Infrared Spin-Scan Radiometer,
VISSR
Visible Infrared Spin-Scan Radiometer
Atmospheric Sounder, VAS
Multispectral Radiometer, MSR (also
referred to as VISSR)
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The original GOES instrument was the VISSR.
The VISSR was first flown aboard the NOAA
Synchronous Meteorological Satellite (SMS-1
and SMS-2). GOES-1, GOES-2 and GOES-3 flew
the original VISSR instrument. The VISSR
was a dual-band (visible and infrared)
spin-scanning imaging device. This
instrument provided the capability for day
and night time observations of clouds and
the determination of cloud heights,
temperatures and wind fields. GOES-4
through GOES-8 were flown with a modified
instrument package called the VISSR
Atmospheric Sounder (VAS). The modified
instrument contained a set of infrared
sensors that provided an atmospheric
sounder capability. The VAS retained the
VISSR dual-band imaging function while
expanding to six infrared channels. The
additional channels allowed for the
determination of surface and cloud-top
temperatures as in VISSR plus
three-dimensional structure of the
atmospheric temperature and water-vapor
distribution.
Each GMS carried a VISSR and supporting
subsytems. The characteristics of the GMS
VISSR were essentially the same as the GOES
VISSR.
Each Meteosat has a payload of the
Mutispectral Radiometer, which is also
referred to as a VISSR. This radiometer
provided image generation in the infrared
region, in the water vapor absorption bands
and in the visible range.
In general, the instrumentation design
and operation were similar among all three
platforms.
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- The VISSR was designed to provide rapid
continuous viewing of local areas for
regional Earth and atmospheric
monitoring.
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- Radiant and solar-reflected energy.
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The VISSR is a multi-channel instrument
designed to sense radiant and
solar-reflected energy from sampled areas
of the Earth. The multi-element spectral
channels sweep east-west and west-east
along a north to south path by using a
two-axis mirror scan system. The instrument
uses a flexible scan system to produce
full-Earth disc images, sector images that
contain the edges of the Earth and area
scans of various sizes. Scan selection
allows for rapid continuous monitoring of
regional scale phenomena.
At the rotation rate of 100 rpm, the
full North to South view of the Earth is
accomplished in 18.21 minutes.
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The VISSR instrument consists of a scanning
system, a radiometer telescope and infrared
and visible sensors.
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For the GOES VISSR, the scanning system
consists of a mirror that mechanically
positioned to provide North to South
viewing while the 100 rpm rotation of the
satellite provides for West to East
scanning. Each step of the mirror changes
the scan angle by 192 microradians. A
sequence of 1,821 scans is performed in
order to obtain the full disk view of the
Earth.
The scanning mirror reflects the received
radiation into a sixteen inch diameter
telescope. The telescope is coupled with
the eight visible detectors via a
fiber-optics bundle. In addition, germanium
relay lenses are used to pass received
radiation to two HdCdTe infrared detectors.
The sensors are arranged in a linear
array oriented perpendicular to the scan
direction, and thus sweep out eight
parallel scan line paths as the satellite
rotates.
For GOES-1 through GOES-4, the sensors
have a field of view (FOV) of 21
microradians square. For GOES-5 through
GOES-8, the sensors have a field of view
(FOV) of 20 microradians (West-East
direction) and 25 microradians (North-South
direction). This FOV provides a ground
resolution of 0.9 km. The FOV of the IR
detectors is 192 microradians thus
providing equivalent coverage to the eight
visible sensors.
For the Meteosat platforms, the FOV is
18 degrees. The ground pixel size is 2.5 by
2.5 km for the visible and water vapor
bands and 5 by 5 km for the infrared
bands.
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- This information is not available at this
time.
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this time.
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Rao, P.K., S.J. Holmes, R.K. Anderson, J.S.
Winston, and P.E. Lehr, Weather Satellites:
Systems, Data, and Environmental
Applications, American Meteorological
Society, Boston, 1990.
Colwell, R.N. (Editor-in-Chief), Manual
of Remote Sensing: Second Edition, Volumes
I and II, American Society of
Photogrammetry, 1983.
Cornillon, P., A Guide to Environmental
Satellite Data, University of Rhode Island
Marine Technical Report 79, 1982.
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- See the
EOSDIS Glossary for a more general listing of
terms related to the Earth Observing System
project.
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See the
EOSDIS Acronyms for a more general listing
of terms related to the Earth Observing System
project.
- DAAC
Distributed Active Archive Center
- GMS
Geostationary Meteorological Satellite
- GOES
Geostationary Operational Environmental
Satellites
- IR Infrared
- GSFC Goddard
Space Flight Center
- Meteosat Meteorological
Satellite
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VISSR
Visible Infrared Spin-Scan Radiometer
- URL Uniform
Resource Locator
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- July 31, 1996
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- July 31, 1996
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- This information is not available at this
time.
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- Suraiya Ahmad
ahmad@daac.gsfc.nasa.gov
Change History
- Version 2.0
- Version baselined on addition to the GES
Controlled Documents List, July 31, 1996.
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