Objective: To learn how to apply the specular interferometric imaging condition (i.e., migration with semi-natural Green's functions) to VSP data to obtain ghost migration images.
Skill Learned: Compile and run a Fortran program for ghost migration with specular interferometry; Analyze the migration results; QC data.
Procedure:
ximage < file_crgmutedirect/crg/crg1 n1=12000 d1=0.00025 label1='Time (s)' perc=99 title='crg1 ' & ximage < file_crgmutedirect/crg/crg45 n1=12000 d1=0.00025 label1='Time (s)' perc=99 title='crg45' & ximage < file_crgmutedirect/crg/crg91 n1=12000 d1=0.00025 label1='Time (s)' perc=99 title='crg91' & ximage < time_s/ts/ts1 n1=521 d1=2.5 d2=2.5 label1='Depth (m)' label2='Dist (m)' title='ts1 ' & ximage < time_s/ts/ts46 n1=521 d1=2.5 d2=2.5 label1='Depth (m)' label2='Dist (m)' title='ts46' & ximage < time_s/ts/ts92 n1=521 d1=2.5 d2=2.5 label1='Depth (m)' label2='Dist (m)' title='ts92' &
ximage < SI.mig/image/image_file1 n1=521 d1=2.5 d2=2.5 label1='Depth (m)' label2='Dist (m)' title='image_file1' & ximage < SI.mig/image/image_file45 n1=521 d1=2.5 d2=2.5 label1='Depth (m)' label2='Dist (m)' title='image_file45' & ximage < SI.mig/image/image_file91 n1=521 d1=2.5 d2=2.5 label1='Depth (m)' label2='Dist (m)' title='image_file91' &
Something to think about:
open(unit=5, file=filename2,form='unformatted', + access='direct', recl=nz*4) do ix=1,nx write(5,rec=ix) ( image(ix,iz),iz=1,nz ) enddo close(5)