Gamma ISP: Reference Manual


multi_SLC_WSS.c

ANSI-C program: multi_SLC_WSS.c

NAME
multi_SLC_WSS -  calculate multi-look intensity image (MLI) from a ASAR Wide-Swath SLC

SYNOPSIS
usage: multi_SLC_WSS <SLC> <SLC_par> <MLI> <MLI_par>

<SLC> (input) ASAR Wide-Swath SLC image
<SLC_par> (input) ASAR Wide-Swath SLC image parameter file
<MLI> (output) multi-look intensity image
<MLI_par> (output) MLI image parameter file

EXAMPLE
multi_SLC_WSS 20030921.VV.IS1.SLC 20030921.VV.IS1.SLC.par 20030921.VV.IS1.mli 20030921.VV.IS1.mli.par

DESCRIPTION
multi_SLC_WSS  reads the complex-valued input ASAR WSS SLC image and generates a real-valued multi-look intensity image (MLI). A new ISP parameter file  is generated that contains information on the image dimension. dimension. ASAR Wide-Swath SLC data consist of a series of burst images. Each of these bursts consists of 48 lines, spaced 80 meters in azimuth (along-track).  On average every point on the ground is imaged by 3 bursts. multi_SLC_WSS  detects each of these bursts and sums the intensity values from multiple bursts using the times given the SLC line headers. The program detects low-intensity lines at the edges of the SLC bursts and does not include these lines when summing the looks from each of the bursts. 

In the process of generating an interferogram from WSS data, MLI images must be produced from each of the SLCs. These MLI images are used for estimation of the offsets between the SLC images and for calculation of the interferometric coherence.  

SEE ALSO
WSS_intf


© Copyrights for Documentation, Users Guide and Reference Manual by Gamma Remote Sensing, 2005.
UW, CW, last change 21-Nov-2005.