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Examples

The following OASR input file dacol-rhs.dat produces the plot of the reflection coefficient shown in Fig. 3 of Ref. [16], and generates the file dacol-rhs.rhs with the boundary operators used subsequently by OASS to compute the scattering kernels.

dacol-rhs.dat:

Dacol and Berman. l= 7.07. 
N s
3
0 1500 0 0 0 1 0
0 1500 0 0 0 1 0
0 5000 2000 0.00 0.00 3.0 -1. 7.07 
100 100 1 1
0.01 89.99 91 0
90 0 12 15                         # Grazing angle axes
0. 10 12 1                         # Loss axes

The input file used subsequently by OASS to generate the plots in Figs. 4 and 5 of Ref.[16], is

dacol-sca.dat:

Dacol and Berman. l= 7.07.
P N I S                             # Plane geometry
100
3
0 1500 0 0 0 1 0
0 1500 0 0 0 1 0
0 5000 2000 0.00 0.00 3.0 -1. 7.07
2121.32 3                           # cph=2121 ~ 45 deg.
2                                   # two depths
-60 0 0 1 0
-10 0 0 1 0

1000 -1000                          # pos+neg spectrum
1024 1 1024

The following OAST input file arsrp-mean.dat produces the contour plot of the mean field for the ARSRP scenari, shown in Fig.1 of Ref. [15]:

arsrp-mean.dat:

ARSRP J218. 6 deg. Basalt.      # >>> Block I: Title
N J C I T L P G s               # >>> Block II: Options
250 250 1 0                     # >>> Block III: Frequency sampling
16                              # >>> Block IV: Environment
0 0 0 0 0 0 0
0 1544 -1524 0 0 1 0
175.0 1524. -1521 0 0 1 0
350   1521. -1510 0 0 1 0
650 1510 -1497 0 0 1 0
950 1497 -1495 0 0 1 0
1250 1495 -1497 0 0 1 0
1500 1497 -1498 0 0 1 0
1750 1498 -1500 0 0 1 0
2125 1500 -1504 0 0 1 0
2500 1504 -1510 0 0 1 0
2875 1510 -1516 0 0 1 0
3250 1516 -1523 0 0 1 0
3625 1523 -1530 0 0 1 0
3990 1530 0 0 0 1 0             # Note iso layer at rough bottom!
4000 5200 2500 .2 .5 2.4 -2 6   # 2 m RMS, L=6 m


175 10 3.66 6.0 1 4000          # Block V: Source array
1 4000 41 40                    # Block VI:Receiver depths

1520 1545                       # Block VII: Phase velocities
-1 1 1                          #            Auto sampling

0 40 20 10                      # Block VIII: Range axis
0 80 12 10                      # Block IX: TL axes.
0 4000 12 500                   # Block X: Depth axis
40 70 3                         # Block XI: Contour intervals

1450 1550 15 25                 # Block XII: Velocity axis
0 4000 15 1000                  #            Depth axis

To create the expectation of the scattered field intensity in Fig.2b of Ref.[15], use the following input file with OASS.

arsrp.dat:

ARSRP J218. 6 deg. Basalt. L=6m # Block I: Title
P D G                           # Block II: Options
250 0                           # Block III: Frequency
16                              # Block IV: Environment            
0 0 0 0 0 0 0
0 1544 -1524 0 0 1 0
175.0 1524. -1521 0 0 1 0
350   1521. -1510 0 0 1 0
650 1510 -1497 0 0 1 0
950 1497 -1495 0 0 1 0
1250 1495 -1497 0 0 1 0
1500 1497 -1498 0 0 1 0
1750 1498 -1500 0 0 1 0
2125 1500 -1504 0 0 1 0
2500 1504 -1510 0 0 1 0
2875 1510 -1516 0 0 1 0
3250 1516 -1523 0 0 1 0
3625 1523 -1530 0 0 1 0
3990 1530 0 0 0 1 0             # Note iso layer at rough bottom!
4000 5200 2500 .2 .5 2.4 -2 6   # 2 m RMS, L=6 m

1500 16                         # Block V: dummy, Interface #.

21                              # Block VI: 4 km long VLA
1 0 0 1 0
200 0 0 1 0
400 0 0 1 0
600 0 0 1 0
800 0 0 1 0
1000 0 0 1 0
1200 0 0 1 0
1400 0 0 1 0
1600 0 0 1 0
1800 0 0 1 0
2000 0 0 1 0
2200 0 0 1 0
2400 0 0 1 0
2600 0 0 1 0
2800 0 0 1 0
3000 0 0 1 0
3200 0 0 1 0
3400 0 0 1 0
3600 0 0 1 0
3800 0 0 1 0
3999 0 0 1 0

1450 -1450                      # Block VII: CMIN, CMAX
2048 1 2048			#            dummy

0 40 101                        # Block VIII: 101 ranges, 0<r<40 km



henrik schmidt
1999-08-25