ATSR-1
AVAILABILITY
http://www.atsr.rl.ac.uk/ The ATSR channels are at wavelengths of 1.6um (swir) and three thermal bands at 3.7um, 11um, and 12um. Data products - http://www.atsr.rl.ac.uk/dataproducts/index.shtml
REQUEST PROCEDURE
SST product - http://www.atsr.rl.ac.uk/ssts/index.shtml If you have any problems, please email support@www.atsr.rl.ac.uk. for other data- http://earth.esa.int/dataproducts/
Satellite Instruments
The ATSR (Along Track Scanning Radiometer) instruments produce infrared images of the Earth at a spatial resolution of one kilometre. The data from these instruments is useful for scientific studies of the land surface, atmosphere, clouds, oceans, and the cryosphere. The first ATSR instrument, ATSR-1, was launched on board the European Space Agency's (ESA) European Remote Sensing Satellite (ERS-1) in July 1991, as part of their Earth Observation Programme. ATSR stands for Along Track Scanning Radiometer. They are imaging radiometers that provide images of the Earth's surface from space. Each ATSR instrument has been designed for exceptional sensitivity and stability of calibration, which are achieved through the incorporation of several innovative features in the instrument design. This design has, among other things, enabled the accurate measurement of sea surface temperature to an accuracy of +/- 0.3K! Satellite measurements of the temperature of the surface of the Earth are inevitably affected by the passage of the radiation through the atmosphere. The dual view design of ATSR makes it possible to estimate and correct for these atmospheric effects. The two views result from the instrument's conical scanning mechanism. Each scan takes readings from the nadir position and then sweeps round to take measurements from a point about 900Km along the satellite's track. A few minutes after acquiring the forward view, the satellite passes over the same spot and takes readings for the nadir view. As the two views of the same scene are taken through different atmospheric path lengths, it is possible to calculate a correction for the effect of atmospheric absorption. Rather than relying on pre launch calibration, the ATSR instrument has two on-board black bodies at known temperatures. Radiation from these is measured during each scan and used to provide a continuous re-calibration of the instrument. This makes it possible to determine single channel equivalent temperatures correct to +/- 0.05K.
CONTACT
C.T. Mutlow
Rutherford Appleton Laboratory
ATSR Science Group Space Science and Technology Department Chilton Didcot Oxfordshire England OX11 0QX
+44 (0)1235 446525
C.T.Mutlow@rl.ac.uk
http://www.atsr.rl.ac.uk/contacts/staff/cmutlow/index.shtml
SPECIFICATIONS
Measurment TypeVisible/IR-imager
Platform TypeERS-1
OrbitSun synchronous
Spectral Coverage
Active/PassivePassive
Scan PatternConical
Variables
Altitude
Inclination
Repeat Time
Wavelength1.6 to 12um
Number of Bands1.6um, 3.7um, 11um, and 12um
Start DateJul 1991
Temporal Coverage
Swath Widthnarrow
REFERENCES
http://www.atsr.rl.ac.uk/index.shtml
UPDATED ON
30 Sep 2009 08:17