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📄 gslib help sgsim.htm

📁 地质统计学代码。适合所有地质和地球科学人员使用。内有帮助文档。在linux和windows下均可使用.
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<HTML><HEAD><TITLE>GSLIB Help: SGSIM</TITLE>
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<H2>GSLIB Help Page: SGSIM</H2></CENTER>
<DL>
  <DT><IMG height=14 alt=o src="GSLIB Help SGSIM.files/ball.red.gif" width=14> 
  <STRONG>Description:</STRONG> 
  <UL>
    <LI>Sequential Gaussian simulation program </LI></UL>
  <DT><IMG height=14 alt=o src="GSLIB Help SGSIM.files/ball.red.gif" width=14> 
  <STRONG>Parameters:</STRONG> 
  <UL>
    <LI><B>datafl:</B> the input data in a simplified Geo-EAS formatted file. If 
    this file does not exist then an unconditional simulation will be generated. 

    <LI><B>icolx, icoly, icolvr, icolwt</B> and <B>icolsec:</B> the column 
    numbers for the <I>x,y</I> and <I>z</I> coordinates, the variable to be 
    simulated, the declustering weight, and the secondary variable (e.g., for 
    external drift if used). One or two of the coordinate column numbers can be 
    set to zero which indicates that the simulation is 2-D or 1-D. For equal 
    weighting, set <B>icolwt</B> to zero. 
    <LI><B>tmin</B> and <B>tmax:</B> all values strictly less than <B>tmin</B> 
    and strictly greater than <B>tmax</B> are ignored. 
    <LI><B>itrans:</B> if set to 0 then no transformation will be performed; the 
    variable is assumed already standard normal (the simulation results will 
    also be left unchanged). If <B>itrans=1</B>, transformations are performed. 
    <LI><B>transfl:</B> output file for the transformation table if 
    transformation is required (<B>igauss</B>=0). 
    <LI><B>ismooth:</B> if set to 0, then the data histogram, possibly with 
    declustering weights is used for transformation, if set to 1, then the data 
    are transformed according to the values in another file (perhaps from 
    histogram smoothing). 
    <LI><B>smthfl:</B> file with the values to use for transformation to normal 
    scores (if <B>ismooth</B> is set to 0). 
    <LI><B>icolvr</B> and <B>icolwt:</B> columns in <B>smthfl</B> for the 
    variable and the declustering weight (set to 1 and 2 if <B>smthfl</B> is the 
    output from <TT>histsmth</TT>). 
    <LI><B>zmin</B> and <B>zmax</B> the minimum and maximum allowable data 
    values. These are used in the back transformation procedure. 
    <LI><B>ltail</B> and <B>ltpar</B> specify the back transformation 
    implementation in the lower tail of the distribution: <B>ltail</B>=1 
    implements linear interpolation to the lower limit <B>zmin</B>, and 
    <B>ltail</B>=2 implements power model interpolation, with <B>w=ltpar</B>, to 
    the lower limit <B>zmin</B>. 
    <LI>The middle class interpolation is linear. 
    <LI><B>utail</B> and <B>utpar</B> specify the back transformation 
    implementation in the upper tail of the distribution: <B>utail</B>=1 
    implements linear interpolation to the upper limit <B>zmax</B>, 
    <B>utail</B>=2 implements power model interpolation, with <B>w=utpar</B>, to 
    the upper limit <B>zmax</B>, and <B>utail</B>=4 implements hyperbolic model 
    extrapolation with <B>w=utpar</B>. The hyperbolic tail extrapolation is 
    limited by <B>zmax</B>. 
    <LI><B>idbg:</B> an integer debugging level between 0 and 3. The larger the 
    debugging level the more information written out. 
    <LI><B>dbgfl:</B> the file for the debugging output. 
    <LI><B>outfl:</B> the output grid is written to this file. The output file 
    will contain the results, cycling fastest on <I>x</I> then <I>y</I> then 
    <I>z</I> then simulation by simulation. 
    <LI><B>nsim:</B> the number of simulations to generate. 
    <LI><B>nx, xmn, xsiz:</B> definition of the grid system (<I>x</I> axis). 
    <LI><B>ny, ymn, ysiz:</B> definition of the grid system (<I>y</I> axis). 
    <LI><B>nz, zmn, zsiz:</B> definition of the grid system (<I>z</I> axis). 
    <LI><B>seed:</B> random number seed (a large odd integer). 
    <LI><B>ndmin</B> and <B>ndmax:</B> the minimum and maximum number of 
    original data that should be used to simulate a grid node. If there are 
    fewer than <B>ndmin</B> data points the node is not simulated. 
    <LI><B>ncnode:</B> the maximum number of previously simulated nodes to use 
    for the simulation of another node. 
    <LI><B>sstrat:</B> if set to 0, the data and previously simulated grid nodes 
    are searched separately: the data are searched with a super block search and 
    the previously simulated nodes are searched with a spiral search (see 
    section II.4). If set to 1, the data are relocated to grid nodes and a 
    spiral search is used and the parameters <B>ndmin</B> and <B>ndmax</B> are 
    not considered. 
    <LI><B>multgrid:</B> a multiple grid simulation will be performed if this is 
    set to 1 (otherwise a standard spiral search for previously simulated nodes 
    is considered). 
    <LI><B>nmult:</B> the number of multiple grid refinements to consider (used 
    only if <B>multgrid</B> is set to 1). 
    <LI><B>noct:</B> the number of original data to use per octant. If this 
    parameter is set less than or equal to 0, then it is not used; otherwise, it 
    overrides the <B>ndmax</B> parameter and the data is partitioned into 
    octants and the closest <B>noct</B> data in each octant is retained for the 
    simulation of a grid node. 
    <LI><B>radius_hmax</B>, <B>radius_hmin</B> and <B>radius_vert</B>: the 
    search radii in the maximum horizontal direction, minimum horizontal 
    direction, and vertical direction (see angles below). 
    <LI><B>sang1, sang2</B> and <B>sang3:</B> the angle parameters that describe 
    the orientation of the search ellipsoid. See the discussion on anisotropy 
    specification associated with Figure II.4. 
    <LI><B>ktype:</B> the kriging type (0 = simple kriging, 1 = ordinary 
    kriging, 2 = simple kriging with a locally varying mean, 3 = kriging with an 
    external drift, or 4 = collocated cokriging with one secondary variable) 
    used throughout the loop over all nodes. SK is required by theory; only in 
    cases where the number of original data found in the neighborhood is large 
    enough can OK be used without the risk of spreading data values beyond their 
    range of influence 
    <LI><B>rho:</B> correlation coefficient to use for collocated cokriging 
    (used only if <B>ktype</B> = 4). 
    <LI><B>secfl:</B> the file for the locally varying mean, the external drift 
    variable, or the secondary variable for collocated cokriging (the secondary 
    variable must be gridded at the same resolution as the model being 
    constructed by <TT>sgsim</TT>). 
    <LI><B>nst</B> and <B>c0:</B> the number of semivariogram structures and the 
    isotropic nugget constant. 
    <LI>For each of the <B>nst</B> nested structures one must define <B>it</B>, 
    the type of structure; <B>cc</B>, the <I>c</I> parameter; 
    <B>ang1,ang2,ang3</B>, the angles defining the geometric anisotropy; 
    <B>aa_hmax</B>, the maximum horizontal range; <B>aa_hmin</B>, the minimum 
    horizontal range; and <B>aa_vert</B>, the vertical range. </LI></UL>
  <DT><IMG height=14 alt=o src="GSLIB Help SGSIM.files/ball.red.gif" width=14> 
  <STRONG>Application notes:</STRONG> 
  <UL>
    <LI>This program requires standard normal data and writes standard normal 
    simulated values. Normal score transform and back transform are to be 
    performed outside of this program 
    <LI>Recall that the power model is not a legitimate model for a 
    multiGaussian phenomenon and it is not allowed in <TT>sgsim</TT> 
    <LI>The semivariogram model is that of the normal scores. The kriging 
    variance is directly interpreted as the variance of the conditional 
    distribution; consequently, the nugget constant <B>c0</B> and <B>c</B> 
    (sill) parameters should add to 1.0. </LI></UL></DT></DL><IMG height=8 alt=--- 
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