| Environments | PYTHON :: EASI :: MODELER |
| Batch Mode | Yes |
| Quick links | Description :: Parameters :: Parameter descriptions :: Details :: References :: Related |
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| Name | Type | Length | Value range |
|---|---|---|---|
| Input MERIS File Name * | String | 1 - | |
| Output: Output file name * | Raster port | 1 - | |
| OutputOrbit: Output satellite orbital ephemeris layer * | ORB port | 1 - 1 | |
| CD Input Layer(s) List * | Integer | 1 - 16 | |
| File Description | String | 0 - 1 | |
| Report | String | 0 - 192 | See parameter description |
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Input MERIS File Name
Specifies the full path and file name of the MERIS-format file to be processed. The input file has an .N1 extension.
Output: Output file name
Specifies the name of the output file that will receive the processed data. The output file is created automatically and must not already exist.
OutputOrbit: Output satellite orbital ephemeris layer
Specifies the output satellite orbital ephemeris layer that will receive the orbital information.
CD Input Layer(s) List
Specifies the list of channels or layers to read from the CD. Up to 9 channels may be specified.
For each channel, a corresponding channel is created in the output PCIDSK file. Duplicate channels are not allowed.
If this parameter is not specified, all channels will be read from the file.
File Description
Optionally specifies a line of text that describes the file. Typically, this contains information that identifies the location of the data and the CD reference number.
If TEX1 (File Description) is not specified, the File Header fields in the generated output PCIDSK image database hold the following information:
Report
Specifies where to direct the generated report.
Available options are:
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CDMERIS is part of the satellite orthorectification component. It reads the MERIS format CD when satellite orthorectification is required. CDMERIS automatically creates a PCIDSK file, reads all the requested image channels from CD, and saves the satellite path information in a segment.
CDMERIS extracts from the CD the geographic coordinates of the scene center and the four corner points. The values are stored in the output orbit segment. These points can be used as ground control point (GCP) input for an approximate correction, which is useful when GCPs are unavailable for an area. Note, however, that using geographic coordinates may not produce very accurate results. To ensure an accurate calculation, a sufficient number of GCPs must be used for each scene or block of scenes.
The output file is automatically created with the dimensions required to hold all of the requested data. Ensure that sufficient disk space is available before running CDMERIS.
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Toutin, Th. "Analyse mathématique des possibilités cartographiques du système SPOT". Thèse de Docteur-Ingénieur en Sciences Géodésiques, ENSG, Paris, France, 1985. pp1 -163.
Toutin, Th. and Carbonneau Y. "La multi-stéréoscopie pour les corrections d'images SPOT-HRV", Canadian Journal of Remote Sensing, Vol. 15, No. 2 (September 1989) p110. (Also available in English from the Canada Centre for Remote Sensing.)
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