AISTAIST > AM Expert System > calmas GSJGSJ
to Top Menu Program "calmas"
Calculate theoretical magnetic anomaly distribution on the specified observation surface, caused by symple source model.
Working Dir.        
LOG Filename    
Calc.Altitude grid Filename        
Model anom. Outfile   (new)
How to specify Source Pos.  
Ambient field Direction   (Inclination and Declination) (in deg.)  
Model parameter definition     Model           Northing,   Easting (km)       Depth (km)     Effective       Magnetization
  Type           (Median Size)   (Median Size)   (Top Bottom)   Vol.etc.     (A/m)       (Inc., Dec.)
(6 individual models at most)  
If models less than 6,  
select the value of   "No"  
at the top of excess field.