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ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

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100 CHAPTER 13. DATA CALIBRATION<br />

13.2 Calibrating the PDS<br />

So you have your PDS created and want to calibrate it. There is a core set of CIA calibration<br />

routines that perform corrections which are required for all CAM data regardless of AOT, e.g.<br />

dark correction, deglitching, stabilization, flat-fielding. These routines are described in the<br />

Section 13.2.1. Further sections describe routines that perform AOT dedicated processing, e.g.<br />

raster MOSAIC creation. So to do a complete calibration of your data first read Section 13.2.1<br />

followed by one of Sections 13.2.2, 13.2.4 or 13.2.5 depending on the flavour of your PDS.<br />

13.2.1 Core calibration<br />

The first three core calibration routines that we will meet are corr dark, deglitch and stabilize.<br />

These routines perform the following core corrections: (i) dark correction, (ii) deglitching,<br />

(iii) stabilization. All have a choice of different methods, though for simplicity we will just use<br />

the default here. Though we use a raster PDS in our example below, these routines accept any<br />

flavour of PDS as input.<br />

1. Following from Section 13.1.2 we will restore our previously saved raster PDS and perform<br />

the first calibration steps on the IMAGEs in lw6 raster.cube.<br />

CIA> restore, ’lw6_raster.dat’, /verb<br />

CIA> corr_dark, lw6_raster<br />

CIA> deglitch, lw6_raster<br />

CIA> stabilize, lw6_raster<br />

2. We can look at the results of our processing so far by viewing the the corrected IMAGEs<br />

in lw6 raster.cube with x3d.<br />

CIA> x3d, lw6_raster<br />

Clicking on the button mask indicates the pixels that have been masked as unstable. By<br />

looking at the temporal history of the pixels you can immediately see if good stabilisation<br />

and deglitching have been achieved. A vertical profile of some background pixels will tell<br />

you if a good dark correction has been applied.<br />

3. Now can proceed with flat-fielding. Firstly, all the IMAGEs per CAM pointing /SCD must<br />

be averaged to EXPOSUREs – the routine reduce does just that. Then the flat-fielding<br />

is performed on each EXPOSURE with corr flat.<br />

CIA> reduce, lw6_raster<br />

CIA> corr_flat, lw6_raster<br />

Now we have completed the final processing step with the core calibration routines.

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