@@ -16,15 +16,15 @@ fast but allows computing the anomaly of arbitrarily complex shapes.
16
16
Required Arguments (not all)
17
17
----------------------------
18
18
19
- - ** fname** : Optional positional argument with the name of a _ xyz..._ file that can be read by \myreflink{ gmtread} .
19
+ - ** fname** : Optional positional argument with the name of a _ xyz..._ file that can be read by gmtread.
20
20
The * xyz* file can have 3, 4, 5, 6 or 8 columns. In first case (3 columns) the magnetization (or density)
21
21
are assumed constant (controlled by ** density** or ** mag_params** ). Following cases are: 4 columns -> 4rth col
22
22
magnetization intensity; 5 columns: mag, mag dip; 6 columns: mag, mag dec, mag dip; 8 columns: field dec, field dip,
23
23
mag, mag dec, mag dip. When n columns > 3 the third argument of the ** mag_params** option is ignored.
24
24
25
- - ** arg1** : In alternative to ` fname ` pass in a Mx3 matrix or a \myreflink{ GMTdataset} with at least 3 columns.
26
- ` arg1 ` can also be a \myreflink{ GMTfv} type like those produced by the _ solids_ functions (\myreflink{ sphere} , etc)
27
- but it must be one made of triangles. That is, the output of \myreflink{ cube} wont work because the body is
25
+ - ** arg1** : In alternative to ` fname ` pass in a Mx3 matrix or a GMTdataset with at least 3 columns.
26
+ ` arg1 ` can also be a GMTfv type like those produced by the _ solids_ functions (sphere, etc)
27
+ but it must be one made of triangles. That is, the output of cube wont work because the body is
28
28
made out of quadrangles. Note, if the ** body** option is used neither this option nor ** fname** are used.
29
29
30
30
- ** C** or ** density** : -- * density=??* \
0 commit comments