ahmilb@houu64$bhp3dnmo
BHP3DNMO - NMO for multiple lines, using user-specified arbitrary velocity
functions
bhp3dnmo is a multi-line adaptation of the SU sunmo program.
bhp3dnmo <stdin >stdout [optional parameters]
Optional Parameters:
veltype=par3d Velocity file type. Use veltype=su for velocities
from seismic traces. It is assumed that velocity
traces are in correct line,cdp order, and that each
trace has the same sampling interval and trace length
as the seismic data being corrected. Within a line,
velocity traces will be linearly interpolated for
missing CDPs.
velfile=vels.su Velocity traces if veltype=su.
pardir=3dvels Directory containing par file for each line, where
files are named line_'num'.par3d. 'num' corresponds
to 3D line number, which is matched against
lhdr value in trace data. Not used if veltype=su.
lhdr=ep Header used to locate par3d file containing correct
vnmo,tnmo,anis1,anis2, and cdp parameters. If
veltype=su, velocity trace header to use for line.
tnmo=0 NMO times corresponding to velocities in vnmo
vnmo= NMO velocities corresponding to times in tnmo
anis1=0 two anisotropy coefficients making up quartic term
anis2=0 in traveltime curve, corresponding to times in tnmo
cdp= CDPs for which vnmo & tnmo are specified (see Notes)
smute=1.5 samples with NMO stretch exceeding smute are zeroed
lmute=25 length (in samples) of linear ramp for stretch mute
sscale=1 =1 to divide output samples by NMO stretch factor
invert=0 =1 to perform (approximate) inverse NMO
ixoffset=0 do not consider cross-line offset
=1 read cross-line offset from trace header
Notes:
For constant-velocity NMO, specify only one vnmo=constant and omit tnmo.
The anisotropy coefficients anis1, anis2 permit non-hyperbolicity due
to layering, mode conversion, or anisotropy. Default is isotropic NMO.
For NMO with a velocity function of time only, specify the arrays
vnmo=v1,v2,... tnmo=t1,t2,...
where v1 is the velocity at time t1, v2 is the velocity at time t2, ...
The times specified in the tnmo array must be monotonically increasing.
Linear interpolation and constant extrapolation of the specified velocities
is used to compute the velocities at times not specified.
The same holds for the anisotropy coefficients as a function of time only.
For NMO with a velocity function of time and CDP, specify the array
cdp=cdp1,cdp2,...
and, for each CDP specified, specify the vnmo and tnmo arrays as described
above. The first (vnmo,tnmo) pair corresponds to the first cdp, and so on.
Linear interpolation and constant extrapolation of 1/velocity^2 is used
to compute velocities at CDPs not specified.
The same holds for the anisotropy coefficients as a function of time and
CDP.
Moveout is defined by
1 anis1
--- x^2 + ------------- x^4.
v^2 1 + anis2 x^2
Note: In general, the user should set the cdp parameter. The default is
to use tr.cdp from the first trace and assume only one cdp.
Caveat:
Nmo cannot handle negative moveout as in triplication caused by
anisotropy. But negative moveout happens necessarily for negative anis1 at
sufficiently large offsets. Then the error-negative moveout- is printed.
Check anis1. An error (anis2 too small) is also printed if the
denominator of the quartic term becomes negative. Check anis2. These errors
are prompted even if they occur in traces which would not survive the
NMO-stretch threshold. Chop off enough far-offset traces (e.g. with suwind)
if anis1, anis2 are fine for near-offset traces.
NMO interpolation error is less than 1% for frequencies less than 60% of
the Nyquist frequency.
Exact inverse NMO is impossible, particularly for early times at large
offsets and for frequencies near Nyquist with large interpolation errors.