4.4.1. ASTER¶
ASTER¶
This tab allows for the conversion of ASTER L1T images to the physical measure of Top Of Atmosphere reflectance (TOA), or the application of a simple atmospheric correction using the DOS1 method (Dark Object Subtraction 1), which is an image-based technique (for more information about conversion to TOA and DOS1 correction, see Image conversion to reflectance).
Once the input is selected, available bands are listed in the metadata table.
4.4.1.1. ASTER conversion¶
Apply DOS1 atmospheric correction: if checked, the DOS1 Correction is applied to all the bands;
Use value as NoData
: if checked, pixels having NoDatavalue are not counted during conversion and the DOS1 calculation of DNmin; it is useful when image has a black border (usually pixel value = 0);
Create Band set and use Band set tools: if checked, bands are added to the active Band set after the conversion; also, the Band set is processed according to the tools checked in the Band set;
Add bands in a new Band set: if checked, bands are added to a new empty Band set after the conversion;
4.4.1.2. Metadata¶
All the bands found in the Select file ASTER L1T are listed in the table Metadata. For information about Metadata fields visit the ASTER page .
Earth sun distance
: Earth Sun distance in astronomical units (automatically calculated if Date is filled;UPPERLEFTM
: coordinates of the upper left corner of the image;LOWERRIGHTM
: coordinates of the lower right corner of the image;BATCH
: add this function to the Batch;RUN
: select an output directory and start the conversion process; only bands listed in the table Metadata are converted; converted bands are saved in the output directory with the prefix RT_and automatically loaded in QGIS;


