OOMMF Home next up previous contents index
Next: Micromagnetic Problem Editor: mmProbEd Up: OOMMF eXtensible Solver Previous: OOMMF eXtensible Solver Batch

Subsections


Standard Oxs_Ext Child Classes

An Oxs simulation is built as a collection of Oxs_Ext (Oxs Extension) objects. These are defined via Specify blocks in the input MIF 2 file. The reader will find the information and sample MIF file provided in that section to be a helpful adjunct to the material presented below. Addition example MIF 2 files can be found in the directory oommf/app/oxs/examples.

This section describes the Oxs_Ext classes available in the standard OOMMF distribution, including documentation of their Specify block initialization strings, and a list of some sample MIF files from the oommf/app/oxs/examples directory that use the class. The standard Oxs_Ext objects, i.e., those that are distributed with OOMMF, can be identified by the Oxs_ prefix in their names. Additional Oxs_Ext classes may be available on your system. Check local documentation for details.

In the following presentation, the Oxs_Ext classes are organized into 8 categories: atlases, meshes, energies, evolvers, drivers, scalar field objects, vector field objects, and MIF support classes. The following Oxs_Ext classes are currently available:


Atlases

Geometric volumes of spaces are specified in Oxs via atlases, which divide their domain into one or more disjoint subsets called regions. Included in each atlas definition is the atlas bounding box, which is an axes parallel rectangular parallelepiped containing all the regions. There is also the special universe region, which consists of all points outside the regions specified in the atlas. The universe region is not considered to be part of any atlas, and the universe keyword should not be used to label any of the atlas regions.

The most commonly used atlas is the simple Oxs_BoxAtlas. For combining multiple atlases, use Oxs_MultiAtlas.

Oxs_BoxAtlas:
An axes parallel rectangular parallelepiped, containing a single region that is coterminous with the atlas itself. The specify block has the form
Specify Oxs_BoxAtlas:atlasname {
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
name regionname
}

where xmin, xmax, ... are coordinates in meters, specifying the extents of the volume being defined. The regionname label specifies the name assigned to the region contained in the atlas. The name entry is optional; if not specified then the region name is taken from the object instance name, i.e., atlasname.

Examples: sample.mif, cgtest.mif.

Oxs_ImageAtlas:
This class is designed to allow an image file to be used to define regions in terms of colors in the image. It is intended for use in conjunction with the Oxs_AtlasScalarField and Oxs_AtlasVectorField classes in circumstances where a small number of distinct species (materials) are being modeled. This provides a generalization of the mask file functionality of the 2D solver (Sec. 17.3.3).

For situations requiring continuous variation in material parameters, the script field classes should be used in conjunction with the ReadFile MIF extension command. See the ColorField sample proc in the ReadFile documentation for an example of this technique.

The Oxs_ImageAtlas Specify block has the following form:

Specify Oxs_ImageAtlas:name {
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
viewplane view
image pic
colormap {
color-1 region_name
color-2 region_name
...
color-n region_name
}
matcherror max_color_distance
}

The xrange, yrange, zrange entries specify the extent of the atlas, in meters. The viewplane view value should be one of the three two-letter codes xy, zx or yz, which specify the mapping of the horizontal and vertical axes of the image respectively to axes in the simulation. The image is scaled as necessary along each dimension to match the atlas extents along the corresponding axes. The image is overlaid through the entire depth of the perpendicular dimension, i.e., along the axis absent from the viewplane specification. The Oxs_ImageAtlas class can be used inside a Oxs_MultiAtlas object to specify regions in a multilayer structure.

The image entry specifies the name of the image file to use. If the file path is relative, then it will be taken with respect to the directory containing the MIF file. The image format may be any of those recognized by any2ppm. The file will be read directly by Oxs if it is in the P3 or P6 PPM formats, otherwise any2ppm will be automatically launched to perform the conversion.

The colormap value is an even length list of color + region name pairs. The colors may be specified in any of several ways. The most explicit is to use one of the Tk numeric formats, #rgb, #rrggbb, #rrrgggbbb or #rrrrggggbbbb, where each r, g, and b is one hex digit (i.e., 0-9 or A-F) representing the red, green and blue components of the color, respectively. For example, #F00 is bright (full-scale) red, #800 would be a darker red, while #FF0 and #FFFF00 would both be bright yellow. Refer to the Tk_GetColor documentation for details. For shades of gray the special notation grayD or greyD is available, where D is a decimal value between 0 and 100, e.g., grey0 is black and grey100 is white. Alternatively, one may use any of the symbolic names defined in the oommf/config/colors.config file, such as red, white and skyblue. When comparing symbolic names, spaces and capitalization are ignored. The list of symbolic names can be extended by adding additional files to the Color filename option in the options.tcl customization file. Finally, one color in the colormap list may optionally be the special keyword ``default''. All pixels that don't match any of the other specified colors (as determined by the matcherror option) are assigned to region paired with default.

Each of the specified colors should be distinct, but the region names are allowed to be repeated as desired. The region names may be chosen arbitrarily, except the special keyword ``universe'' is reserved for points not in any of the regions. This includes all points outside the atlas bounding box defined by the xrange, yrange, zrange entries, but may also include points inside that boundary.

Pixels in the image are assigned to regions by comparing the color of the pixel to the list of colors specified in colormap. If the pixel color is closer to a colormap color than max_color_distance, then the colors are considered matched. If a pixel color matches exactly one colormap color, then the pixel is assigned to the corresponding region. If a pixel color matches more than one colormap color, the pixel is assigned to the region corresponding to the closest match. If a pixel color doesn't match any of the colormap colors, then it is assigned to the default region, which is the region paired with the ``default'' keyword. If default does not explicitly appear in the colormap colors list, then universe is made the default region.

To calculate the distance between two colors, each color is first converted to a scaled triplet of floating point red, green, and blue values, (r, g, b) , where each component lies in the interval [0, 1] , with (0, 0, 0) representing black and (1, 1, 1) representing white. For example, (0, 0, 1) is bright blue. Given two colors in this representation, the distance is computed using the standard Euclidean norm with uniform weights, i.e., the distance between (r1, g1, b1) and (r2, g2, b2) and is

$\displaystyle \sqrt{{(r_1-r_2)^2 + (g_1-g_2)^2 + (b_1-b_2)^2}}$.

Since the difference in any one component is at most 1, the distance between any two colors is at most $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\sqrt{3}\\ \rule{1pt}{0pt}\end{array}$}$ .

As explained above, two colors are considered to match if the distance between them is less than the specified matcherror value. If max_color_distance is sufficiently small, then it may easily happen that a pixel's color does not match any of the specified region colors, so the pixel would be assigned to the default region. On the other hand, if max_color_distance is larger than $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\sqrt{3}\\ \rule{1pt}{0pt}\end{array}$}$ , then all colors will match, and no pixels will be assigned to the default region. If matcherror is not specified, then the default value for max_color_distance is 3, which means all colors match.

The following example should help clarify these matters. 

Specify Oxs_ImageAtlas:atlas {
    xrange { 0 400e-9 }
    yrange { 0 200e-9 }
    zrange { 0  20e-9 }
    image  mypic.gif
    viewplane "xy"
    colormap {
        blue   cobalt
        red    permalloy
        green  universe
        default cobalt
    }
    matcherror .1
}
Blue pixels get mapped to the ``cobalt'' region and red pixels to the ``permalloy'' region. Green pixels are mapped to the ``universe'' non-region, which means they are considered to be outside the atlas entirely. This is a fine point, but comes into play when atlases with overlapping bounding boxes are brought together inside an Oxs_MultiAtlas. To which region would an orange pixel be assigned? The scaled triplet representation for orange is (1, 0.647, 0) , so the distance to blue is 1.191 , the distance to red is 0.647 , and the distance to green is 1.06 . Thus the closest color is red, but 0.647 is outside the matcherror setting of 0.1 , so orange doesn't match any of the colors and is hence assigned to the default region, which in this case is cobalt. On the other hand, if matcherror had been set to say 1, then orange and red would match and orange would be assigned to the permalloy region.

Pixels with colors that are equidistant to and match more than one color in the colormap will be assigned to one of the closest color regions. The user should not rely on any particular selection, that is to say, the explicit matching procedure in this case is not defined.

Examples: imageatlas.mif, grill.mif.

Oxs_MultiAtlas:
This atlas is built up as an ordered list of other atlases. The set of regions defined by the Oxs_MultiAtlas is the union of the regions of all the atlases contained therein. The sub-atlases need not be disjoint, however each point is assigned to the region in the first sub-atlas in the list that contains it, so the regions defined by the Oxs_MultiAtlas are effectively disjoint.

The Oxs_MultiAtlas specify block has the form

Specify Oxs_MultiAtlas:name {
atlas    atlas_1_spec
atlas    atlas_2_spec
...
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
}

Each atlas_spec may be either a reference to an atlas defined earlier and outside the current Specify block, or else an inline, embedded atlas definition. The bounding box xrange, yrange and zrange specifications are each optional. If not specified the corresponding range for the atlas bounding box is taken from the minimal bounding box containing all the sub-atlases.

If the atlases are not disjoint, then the regions as defined by an Oxs_MultiAtlas can be somewhat different from those of the individual component atlases. For example, suppose regionA is a rectangular region in atlasA with corner points (5,5,0) and (10,10,10), and regionB is a rectangular region in atlasB with corner points (0,0,0) and (10,10,10). When composed in the order atlasA, atlasB inside an Oxs_MultiAtlas, regionA reported by the Oxs_MultiAtlas will be the same as regionA reported by atlasA, but regionB as reported by the Oxs_MultiAtlas will be the ``L'' shaped volume of those points in atlasB's regionB not inside regionA. If the Oxs_MultiAtlas is constructed with atlasB first and atlasA second, then regionB as reported by the Oxs_MultiAtlas would agree with that reported by atlasB, but regionA would be empty.

NOTE: The attributes key label is not supported by this class.

Examples: manyregions-multiatlas.mif, spinvalve.mif, spinvalve-af.mif, yoyo.mif.

Oxs_ScriptAtlas:
An atlas where the regions are defined via a Tcl script. The specify block has the form
Specify Oxs_ScriptAtlas:name {
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
regions { rname_1 rname_2 ... rname_n }
script_args { args_request }
script Tcl_script
}

Here xmin, xmax, ... are coordinates in meters, specifying the extents of the axes-parallel rectangular parallelepiped enclosing the total volume being identified. This volume is subdivided into n sub-regions, using the names as given in the regions list. The script is used to assign points to the various regions. Appended to the script are the arguments requested by script_args, in the manner explained in the User Defined Support Procedures section of the MIF 2 file format documentation. The value args_request should be a subset of {relpt rawpt minpt maxpt span }. If script_args is not specified, the default value relpt is used. When executed, the return value from the script should be an integer in the range 1 to n , indicating the user-defined region in which the point lies, or else 0 if the point is not in any of the n regions. Region index 0 is reserved for the implicit ``universe'' region, which is all-encompassing. The following example may help clarify the discussion: 

proc Octs { cellsize x y z xmin ymin zmin xmax ymax zmax } {
    set xindex [expr {int(floor(($x-$xmin)/$cellsize))}]
    set yindex [expr {int(floor(($y-$ymin)/$cellsize))}]
    set zindex [expr {int(floor(($z-$zmin)/$cellsize))}]
    set octant [expr {1+$xindex+2*$yindex+4*$zindex}]
    if {$octant<1 || $octant>8} {
       return 0
    }
    return $octant
}
Specify Oxs_ScriptAtlas:octant {
    xrange {-20e-9 20e-9}
    yrange {-20e-9 20e-9}
    zrange {-20e-9 20e-9}
    regions { VIII V VII VI IV I III II }
    script_args { rawpt minpt maxpt }
    script { Octs 20e-9 }
}
This atlas divides the rectangular volume between (- 20, - 20, - 20) and (20, 20, 20) (nm) into eight regions, corresponding to the standard octants, I through VIII. The Octs Tcl procedure returns a value between 1 and 8, with 1 corresponding to octant VIII and 8 to octant II. The canonical octant ordering starts with I as the + x, + y, + z space, proceeds counterclockwise in the + z half-space, and concludes in the - z half-space with V directly beneath I, VI beneath II, etc. The ordering computed algorithmically in Octs starts with 1 for the - x, - y, - z space, 2 for the + x, - y, - z space, 3 for the - x, + y, - z space, etc. The conversion between the two systems is accomplished by the ordering of the regions list.

Examples: manyregions-scriptatlas.mif, octant.mif, tclshapes.mif, diskarray.mif, ellipsoid-atlasproc.mif.

Oxs_EllipsoidAtlas:
Defines an ellipsoidal region with axes parallel to the coordinate axes. This functionality can be obtained using the Oxs_ScriptAtlas class with an appropriate Tcl script, but this class is somewhat easier to use and faster. The Specify block has the form
Specify Oxs_EllipsoidAtlas:atlasname {
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
name regionname
}

Here xmin, xmax, ... are coordinates in meters, specifying the bounding box for the ellipsoid. The layout of the Specify block is exactly the same as for the Oxs_BoxAtlas class, except that in this case the named region is not the whole bounding box but rather that subvolume that is the interior of the ellipsoid inscribed inside the bounding box. Points exterior to that ellipsoid are assigned to the ``universe'' region.

As in the Oxs_BoxAtlas case, the regionname entry is optional; if missing, the region name is taken from the object instance name, i.e., atlasname.

Example: ellipsoid.mif. See also ellipsoid-atlasproc.mif and ellipsoid-fieldproc.mif for equivalent examples using Tcl scripts.


Meshes

Meshes define the discretization impressed on the simulation. There should be exactly one mesh declared in a MIF 2 file. The only standard mesh available at present is
Specify Oxs_RectangularMesh:name {
cellsize { xstep ystep zstep }
atlas atlas_spec
}

This creates an axes parallel rectangular mesh across the entire space covered by atlas. The mesh sample rates along each axis are specified by cellsize (in meters). The mesh is cell-based, with the center of the first cell one half step in from the minimal extremal point (xmin,ymin,ymax) for atlas_spec. The name is commonly set to ``mesh'', in which case the mesh object may be referred to by other Oxs_Ext objects by the short name :mesh.

Examples: All MIF files contain this class.

Energies

The following subsections describe the available energy terms. In order to be included in the simulation energy and field calculations, each energy term must be declared in its own, top-level Specify block, i.e., energy terms should not be declared inline inside other Oxs_Ext objects. There is no limitation on the number of energy terms that may be specified in the input MIF file. Many of these terms have spatially varying parameters that are initialized via field_object_spec entries in their Specify initialization block.

Outputs: For each magnetization configuration, two standard outputs are provided by all energy terms: the scalar output ``Energy,'' which is the total energy in joules contributed by this energy term, and the vector field output ``Field,'' which is the pointwise field in A/m. If the code was compiled with the macro NDEBUG not defined, then there will be an additional scalar output, ``Calc count,'' which counts the number of times the term has been calculated in the current simulation. This is intended for debugging purposes only; this number should agree with the ``Energy calc count'' value provided by the evolver.


Evolvers

Evolvers are responsible for updating the magnetization configuration from one step to the next. There are two types of evolvers, time evolvers, which track Landau-Lifshitz-Gilbert dynamics, and minimization evolvers, which locate local minima in the energy surface through direct minimization techniques. Evolvers are controlled by drivers, and must be matched with the appropriate driver type, i.e., time evolvers must be paired with time drivers, and minimization evolvers must be paired with minimization drivers. The drivers hand a magnetization configuration to the evolvers with a request to advance the configuration by one step (also called an iteration). It is the role of the drivers, not the evolvers, to determine when a simulation stage or run is complete. Specify blocks for evolvers contain parameters to control all aspects of individual stepwise evolution, but stopping criteria are communicated in the Specify block of the driver, not the evolver.

There are currently three time evolvers and one minimization evolver in the standard OOMMF distribution. The time evolvers are Oxs_EulerEvolve, Oxs_RungeKuttaEvolve, and Oxs_SpinXferEvolve. The minimization evolver is Oxs_CGEvolve.

Oxs_EulerEvolve:
Time evolver implementing a simple first order forward Euler method with step size control on the Landau-Lifshitz ODE [10,12]:

\begin{displaymath} \frac{d\textbf{M}}{dt} = -\vert\bar{\gamma}\vert\,\textbf{M... ...tbf{M}\times\left(\textbf{M}\times\textbf{H}_{\rm eff}\right), \end{displaymath} (2)
where M is the magnetization, Heff is the effective field, $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\bar{\gamma}\\ \rule{1pt}{0pt}\end{array}$}$ is the Landau-Lifshitz gyromagnetic ratio, and $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\alpha\\ \rule{1pt}{0pt}\end{array}$}$ is the damping constant. The Gilbert form

\begin{displaymath} \frac{d\textbf{M}}{dt} = -\vert\gamma\vert\,\textbf{M}\time... ...ha}{M_s} \left(\textbf{M}\times\frac{d\textbf{M}}{dt}\right), \end{displaymath} (3)
where $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ is the Gilbert gyromagnetic ratio, is mathematically equivalent to the Landau-Lifshitz form under the relation $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma = (1+\alpha^2)\,\bar{\gamma}\\ \rule{1pt}{0pt}\end{array}$}$ .

The Specify block has the form

Specify Oxs_EulerEvolve:name {
alpha $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\alpha\\ \rule{1pt}{0pt}\end{array}$}$
gamma_LL $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\bar{\gamma}\\ \rule{1pt}{0pt}\end{array}$}$
gamma_G $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$
do_precess precess
min_timestep minimum_stepsize
max_timestep maximum_stepsize
fixed_spins {
atlas_spec
region1 region2 ...
}
start_dm $ \Delta$m
error_rate rate
absolute_step_error abs_error
relative_step_error rel_error
step_headroom headroom
}

All the entries have default values, but the ones most commonly adjusted are listed first.

The options alpha, gamma_LL and gamma_G are as in the Landau-Lifshitz-Gilbert ODE (2), (3), where the units on $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\bar{\gamma}\\ \rule{1pt}{0pt}\end{array}$}$ and $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ are m/A . s and $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\alpha\\ \rule{1pt}{0pt}\end{array}$}$ is dimensionless. At most one of $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\bar{\gamma}\\ \rule{1pt}{0pt}\end{array}$}$ and $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ should be specified. If neither is specified, then the default is $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ = 2.211 x 105 . (Because of the absolute value convention adopted on $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\bar{\gamma}\\ \rule{1pt}{0pt}\end{array}$}$ and $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ in (2), (3), the sign given to the value of gamma_LL or gamma_G in the Specify block is irrelevant.) The default value for $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\alpha\\ \rule{1pt}{0pt}\end{array}$}$ is 0.5, which is large compared to experimental values, but allows simulations to converge to equilibria in a reasonable time. However, for accurate dynamic studies it is important to assign an appropriate value to $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\alpha\\ \rule{1pt}{0pt}\end{array}$}$ .

The do_precess value should be either 1 or 0, and determines whether or not the precession term in the Landau-Lifshitz ODE (i.e., the first term on the righthand side in (2)) is used. If precess is 0, then precession is disabled and the simulation evolves towards equilibrium along a steepest descent path. The default value is 1.

The min_timestep and max_timestep parameters provide soft limits on the size of steps taken by the evolver. The minimum value may be overridden by the driver if a smaller step is needed to meet time based stopping criteria. The maximum value will be ignored if a step of that size would produce a magnetization state numerically indistinguishable from the preceding state. The units for min_timestep and max_timestep are seconds. Default values are 0 and 10-10 respectively.

The optional fixed_spins entry allows the magnetization in selected regions of the simulation to be frozen in its initial configuration. The value portion of the entry should be a list, with the first element of the list being either an inline atlas definition (grouped as a single item), or else the name of a previously defined atlas. The remainder of the list are names of regions in that atlas for which the magnetization is to be be fixed, i.e., M(t) = M(0) for all time t for all points in the named regions. Fields and energies are computed and reported normally across these regions. Although any atlas may be used, it is frequently convenient to set up an atlas with special regions defined expressly for this purpose.

The stepsize for the first candidate iteration in the problem run is selected so that the maximum change in the normalized (i.e., unit) magnetization m is the value specified by start_dm. The units are degrees, with default value 0.01.

The four remaining entries, error_rate, absolute_step_error, relative_step_error, and step_headroom, control fine points of stepsize selection, and are intended for advance use only. Given normalized magnetization mi(t) at time t and position i , and candidate magnetization mi(t + $ \Delta$t) at time t + $ \Delta$t , the error at position i is estimated to be

\begin{displaymath} \mbox{Error}_i = \left\vert\dot{\textbf{m}}_i(t+\Delta t) - \dot{\textbf{m}}_i(t)\right\vert\Delta t \,/\,2, \end{displaymath}

where the derivative with respect to time, $ \dot{{\textbf{m}}}$ , is computed using the Landau-Lifshitz ODE (2). First order methods essentially assume that $ \dot{{\textbf{m}}}$ is constant on the interval [t, t + $ \Delta$t] ; the above formula uses the difference in $ \dot{{\textbf{m}}}$ at the endpoints of the interval to estimate (guess) how untrue that assumption is.

A candidate step is accepted if the maximum error across all positions i is smaller than absolute_step_error, error_rate   x  $ \Delta$t , and relative_step_error   x  |$ \dot{{\textbf{m}}}_{{\rm max}}^{}$|$ \Delta$t , where |$ \dot{{\textbf{m}}}_{{\rm max}}^{}$| is the maximum value of |$ \dot{{\textbf{m}}}_{i}^{}$| across all i at time t . If the step is rejected, then a smaller stepsize is computed that appears to pass the above tests, and a new candidate step is proposed using that smaller stepsize times step_headroom. Alternatively, if the step is accepted, then the error information is used to determine the stepsize for the next step, modified in the same manner by step_headroom.

The error calculated above is in terms of unit magnetizations, so the natural units are radians or radians/second. Inside the Specify block, however, the error_rate and absolute_step_error are specified in degrees/nanosecond and degrees, respectively; they are converted appropriately inside the code before use. The relative_step_error is a dimensionless quantity, representing a proportion between 0 and 1. The error check controlled by each of these three quantities may be disabled by setting the quantity value to -1. They are all optional, with default values of -1 for error_rate, 0.2 for absolute_step_error, and 0.2 for relative_step_error.

The headroom quantity should lie in the range (0, 1) , and controls how conservative the code will be in stepsize selection. If headroom is too large, then much computation time will be lost computing candidate steps that fail the error control tests. If headroom is small, then most candidate steps will pass the error control tests, but computation time may be wasted calculating more steps than are necessary. The default value for headroom is 0.85.

In addition to the above error control tests, a candidate step will also be rejected if the total energy, after adjusting for effects due to any time varying external field, is found to increase. In this case the next candidate stepsize is set to one half the rejected stepsize.

The Oxs_EulerEvolve module provides five scalar outputs and three vector field outputs. The scalar outputs are

The vector field outputs are

Example: octant.mif.

Oxs_RungeKuttaEvolve:
Time evolver implementing several Runge-Kutta methods for integrating the Landau-Lifshitz-Gilbert ODE (2), (3), with step size control. In most cases it will greatly outperform the Oxs_EulerEvolve class. The Specify block has the form
Specify Oxs_RungeKuttaEvolve:name {
alpha $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\alpha\\ \rule{1pt}{0pt}\end{array}$}$
gamma_LL $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\bar{\gamma}\\ \rule{1pt}{0pt}\end{array}$}$
gamma_G $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$
do_precess precess
allow_signed_gamma signed_gamma
min_timestep minimum_stepsize
max_timestep maximum_stepsize
fixed_spins {
atlas_spec
region1 region2 ...
}
start_dm $ \Delta$m
start_dt start_timestep
stage_start scontinuity
error_rate rate
absolute_step_error abs_error
relative_step_error rel_error
energy_precision eprecision
min_step_headroom min_headroom
max_step_headroom max_headroom
reject_goal reject_proportion
method subtype
}

Most of these options appear also in the Oxs_EulerEvolve class. The repeats have the same meaning as in that class, and the same default values except for relative_step_error and error_rate, which for Oxs_RungeKuttaEvolve have the default values of 0.01 and 1.0, respectively. Additionally, the alpha, gamma_LL and gamma_G options may be initialized using scalar field objects, to allow these material parameters to vary spatially.

The allow_signed_gamma parameter is for simulation testing purposes, and is intended for advanced use only. There is some lack of consistency in the literature with respect to the sign of $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ . For this reason the Landau-Lifshitz-Gilbert equations are presented above (2, 3) using the absolute value of $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ . This is the interpretation used if allow_signed_gamma is 0 (the default). If instead allow_signed_gamma is set to 1, then the Landau-Lifshitz-Gilbert equations are interpreted without the absolute values and with a sign change on the $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ terms, i.e., the default value for $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ in this case is -2.211 x 105 (units are m/A . s). In this setting, if $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$ is set positive then the spins will precess backwards about the effective field, and the damping term will force the spins away from the effective field and increase the total energy. If you are experimenting with $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma>0\\ \rule{1pt}{0pt}\end{array}$}$ , you should either set $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\alpha<=0\\ \rule{1pt}{0pt}\end{array}$}$ to force spins back towards the effective field, or disable the energy precision control (discussed below).

The two controls min_step_headroom (default value 0.33) and max_step_headroom (default value 0.95) replace the single step_headroom option in Oxs_EulerEvolve. The effective step_headroom is automatically adjusted by the evolver between the min_headroom and max_headroom limits to make the observed reject proportion approach the reject_goal (default value 0.05).

The method entry selects a particular Runge-Kutta implementation. It should be set to one of rk2, rk4, rkf54, rkf54m, or rkf54s; the default value is rkf54. The rk2 and rk4 methods implement canonical second and fourth global order Runge-Kutta methods[18], respectively. For rk2, stepsize control is managed by comparing $ \dot{{\textbf{m}}}$ at the middle and final points of the interval, similar to what is done for stepsize control for the Oxs_EulerEvolve class. One step of the rk2 method involves 2 evaluations of $ \dot{{\textbf{m}}}$ .

In the rk4 method, two successive steps are taken at half the nominal step size, and the difference between that end point and that obtained with one full size step are compared. The error is estimated at 1/15th the maximum difference between these two states. One step of the rk4 method involves 11 evaluations of $ \dot{{\textbf{m}}}$ , but the end result is that of the 2 half-sized steps.

The remaining methods, rkf54, rkf54m, and rkf54s, are closely related Runge-Kutta-Fehlberg methods derived by Dormand and Prince[7,8]. In the nomenclature of these papers, rkf54 implements RK5(4)7FC, rkf54m implements RK5(4)7FM, and rkf54s implements RK5(4)7FS. All are 5th global order with an embedded 4th order method for stepsize control. Each step of these methods requires 6 evaluations of $ \dot{{\textbf{m}}}$ if the step is accepted, 7 if rejected. The difference between the methods involves tradeoffs between stability and error minimization. The RK5(4)7FS method has the best stability, RK5(4)7FM the smallest error, and RK5(4)7FC represents a compromise between the two. The default method used by Oxs_RungeKuttaEvolve is RK5(4)7FC.

The remaining undiscussed entry in the Oxs_RungeKuttaEvolve Specify block is energy_precision. This should be set to an estimate of the expected relative accuracy of the energy calculation. After accounting for any change in the total energy arising from time-varying applied fields, the energy remainder should decrease from one step of the LLG ODE to the next. Oxs_RungeKuttaEvolve will reject a step if the energy remainder is found to increase by more than that allowed by eprecision. The default value for eprecision is 1e-10. This control may be disabled by setting eprecision to -1.

The Oxs_RungeKuttaEvolve module provides the same five scalar outputs and three vector outputs as Oxs_EulerEvolve.

Examples: sample.mif, acsample.mif, varalpha.mif, yoyo.mif.

Oxs_SpinXferEvolve:
Time evolver that integrates an Landau-Lifshitz-Gilbert ODE augmented with a spin momentum term [21],

\begin{displaymath} \frac{d\textbf{m}}{dt} = -\vert\gamma\vert\,\textbf{m}\time... ...t\gamma\vert\beta\epsilon^\prime\,\textbf{m}\times\textbf{m}_p \end{displaymath} (4)
(compare to (3)), where
m = $\displaystyle \mbox{reduced magnetization, $\textbf{M}/M_s$}$  
$\displaystyle \gamma$ = Gilbert gyromagnetic ratio  
$\displaystyle \beta$ = $\displaystyle \left\vert\vphantom{\frac{\hbar}{\mu_0 e}}\right.$$\displaystyle {\frac{{\hbar}}{{\mu_0 e}}}$$\displaystyle \left.\vphantom{\frac{\hbar}{\mu_0 e}}\right\vert$$\displaystyle {\frac{{J}}{{t M_s}}}$  
mp = (unit) electron polarization direction  
$\displaystyle \epsilon$ = $\displaystyle {\frac{{P\Lambda^2}}{{(\Lambda^2+1)+(\Lambda^2-1)(\textbf{m}\cdot\textbf{m}_p)}}}$  
$\displaystyle \epsilon^{\prime}_{}$ = secondary spin tranfer term.  

In the definition of $ \beta$ , e is the electron charge in C, J is current density in A/m2 , t is the free layer thickness in meters, and Ms is the saturation magnetization in A/m.

The various parameters are defined in the Specify block, which is an extension of that for the Oxs_RungeKuttaEvolve class:

Specify Oxs_SpinXferEvolve:name {
alpha $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\alpha\\ \rule{1pt}{0pt}\end{array}$}$
gamma_LL $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\bar{\gamma}\\ \rule{1pt}{0pt}\end{array}$}$
gamma_G $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\gamma\\ \rule{1pt}{0pt}\end{array}$}$
do_precess precess
allow_signed_gamma signed_gamma
min_timestep minimum_stepsize
max_timestep maximum_stepsize
fixed_spins {
atlas_spec
region1 region2 ...
}
start_dm $ \Delta$m
stage_start scontinuity
error_rate rate
absolute_step_error abs_error
relative_step_error rel_error
energy_precision eprecision
min_step_headroom min_headroom
max_step_headroom max_headroom
reject_goal reject_proportion
method subtype
P polarization
P_fixed p_fixed_layer
P_free p_free_layer
Lambda $ \Lambda$
Lambda_fixed $ \Lambda$ _fixed_layer
Lambda_free $ \Lambda$ _free_layer
eps_prime ep
J current_density
J_profile Jprofile_script
J_profile_args Jprofile_script_args
mp p_direction
energy_slack eslack
}

The options duplicated in the Oxs_RungeKuttaEvolve class Specify block have the same meaning and default values here, with the exception of error_rate, which for Oxs_SpinXferEvolve has the default value of -1 (i.e., disabled).

The default values for P and Lambda are 0.4 and 2, respectively. If preferred, values for the fixed and free layers may be instead specified separately, through P_fixed, P_free, Lambda_fixed, and Lambda_free. Otherwise P_fixed = P_free = P and Lambda_fixed = Lambda_free = Lambda. Lambda must be larger than or equal to 1; set Lambda=1 to remove the dependence of $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\epsilon\\ \rule{1pt}{0pt}\end{array}$}$ on m . mp . If you want non-zero $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\epsilon^\prime\\ \rule{1pt}{0pt}\end{array}$}$ , it is set directly as eps_prime.

Current density J and unit polarization direction mp are required. The units on J are A/m2 . Positive J produces torque that tends to align $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\textbf{m}\\ \rule{1pt}{0pt}\end{array}$}$ towards $\mbox{\renewcommand {\arraystretch}{0}$\begin{array}[b]{@{}c@{}}\textbf{m}_p\\ \rule{1pt}{0pt}\end{array}$}$ .

Parameters J, mp, P, Lambda, and eps_prime may all be varied pointwise, but are fixed with respect to time. However, J can be multiplied by a time varying ``profile,'' to model current rise times, pulses, etc. Use the J_profile and J_profile_args options to enable this feature. The Jprofile_script should be a Tcl script that returns a single scalar. Jprofile_script_args should be a subset of {stage stage_time total_time }, to specify arguments appended to Jprofile_script on each time step. Default is the entire set, in the order as listed.

The Oxs_SpinXferEvolve module provides the same five scalar outputs and three vector outputs as Oxs_RungeKutta, plus the scalar output ``average J,'' and the vector field outputs ``Spin torque'' (which is |$ \gamma$|$ \beta$$ \epsilon$$ \left(\vphantom{\textbf{m}\times\textbf{m}_p\times\textbf{m}}\right.$m x mp x m$ \left.\vphantom{\textbf{m}\times\textbf{m}_p\times\textbf{m}}\right)$ ) and ``J*mp.'' (Development note: In the case propogate_mp is enabled, mp is actually $ \Delta_{x}^{}$$ \partial$m/$ \partial$x , where x is the flow direction and $ \Delta_{x}^{}$ is the cell dimension in that direction.)

The Oxs_SpinXferEvolve class does not include any oersted field arising from the current. Of course, arbitrary fields simulating the oersted field may be added separately as Zeeman energy terms. An example of this is contained in the spinxfer.mif sample file.

There are no temperature effects in this evolver, i.e., it is a T = 0 K code.

Note also that mp is fixed.

For basic usage, the Specify block can be as simple as 

Specify Oxs_SpinXferEvolve:evolve {
  alpha 0.014
  J 7.5e12
  mp {1 0 0}
  P 0.4
  Lambda 2
}

This class is still in early development; at this time the example files are located in oommf/app/oxs/local instead of oommf/app/oxs/examples.

Examples: spinxfer.mif, spinxfer-miltat.mif, spinxfer-onespin.mif.

Oxs_CGEvolve:
The minimization evolver is Oxs_CGEvolve, which is an in-development conjugate gradient minimizer with no preconditioning. The Specify block has the form
Specify Oxs_CGEvolve:name {
gradient_reset_angle reset_angle
gradient_reset_count count
minimum_bracket_step minbrack
maximum_bracket_step maxbrack
line_minimum_angle_precision min_prec_angle
line_minimum_relwidth relwidth
energy_precision eprecision
method cgmethod
fixed_spins {
atlas_spec
region1 region2 ...
}
}

All entries have default values.

The evolution to an energy minimum precedes by a sequence of line minimizations. Each line represents a one dimensional affine subspace in the 3N dimensional space of possible magnetization configurations, where N is the number of spins in the simulation. Once a minimum has been found along a line, a new direction is chosen that is ideally orthogonal to all preceding directions, but related to the gradient of the energy taken with respect to the magnetization. In practice the line direction sequence cannot be extended indefinitely; the parameters gradient_reset_angle and gradient_reset_count control the gradient resetting process. The first checks the angle between the new direction and the gradient. If that angle is larger than reset_angle (expressed in degrees), then the selected direction is thrown away, and the conjugate-gradient process is re-initialized with the gradient direction as the new first direction. In a similar vein, count specifies the maximum number of line directions selected before resetting the process. Because the first line in the sequence is selected along the gradient direction, setting count to 1 effectively turns the algorithm into a steepest descent minimization method. The default values for reset_angle and count are 80 degrees and 50, respectively.

Once a minimization direction has been selected, the first stage of the line minimization is to bracket the minimum energy on that line, i.e., given a start point on the line--the location of the minimum from the previous line minimization--find another point on the line such that the energy minimum lies between those two points. As one moves along the line, the spins in the simulation rotate, with one spin rotating faster than (or at least as fast as) all the others. If the start point was not the result of a successful line minimization from the previous stage, then the first bracket attempt step is sized so that the fastest moving spin rotates through the angle specified by minimum_bracket_step. In the more usual case that the start point is a minimum from the previous line minimization stage, the initial bracket attempt step size is set to the distance between the current start point and the start point of the previous line minimization stage.

The energy and gradient of the energy are examined at the candidate bracket point to test if an energy minimum lies in the interval. If not, the interval is extended, based on the size of the first bracket attempt interval and the derivatives of the energy at the interval endpoints. This process is continued until either a minimum is bracketed or the fastest moving spin rotates through the angle specified by maximum_bracket_step.

If the bracketing process is successful, then a one dimensional minimization is carried out in the interval, using both energy and energy derivative information. Each step in this process reduces the width of the bracketing interval. This process is continued until either the angle between the line direction and the computed energy gradient is within line_minimum_angle_precision degrees of orthogonal, or the width of the interval relative to the distance of the interval from the start point (i.e., the stop point from the previous line minimization process) is less than line_minimum_relwidth. In either case, the stop point, i.e., the effective minimum, is taken to be the endpoint of the final interval having smaller energy. The default value for min_prec_angle is 5 degrees, and the default value for relwidth is 1. This latter setting effectively disables the line_minimum_relwidth control, which should generally be used only as a secondary control.

If the bracketing process is unsuccessful, i.e., the check for bracketed energy minimum failed at the maximum bracket interval size allowed by maximum_bracket_step, then the maximum bracket endpoint is accepted as the next point in the minimization iteration.

Once the line minimum stop point has been selected, the next iteration begins with selection of a new line direction, as described above, except in the case where the stop point was not obtained as an actual minimum, but rather by virtue of satisfying the maximum_bracket_step constraint. In that case the orthogonal line sequence is reset, in the same manner as when the gradient_reset_angle or gradient_reset_count controls are triggered, and the next line direction is taken directly from the energy gradient.

There are several factors to bear in mind when selecting values for the parameters minimum_bracket_step, maximum_bracket_step, and line_minimum_relwidth. If minimum_bracket_step is too small, then it may take a great many steps to obtain an interval large enough to bracket the minimum. If minimum_bracket_step is too large, then the bracket interval will be unnecessarily generous, and many steps may be required to locate the minimum inside the bracketing interval. However, this value only comes into play when resetting the line minimization direction sequence, so the setting is seldom critical. It is specified in degrees, with default value 0.05.

If maximum_bracket_step is too small, then the minima will be mostly not bracketed, and the minimization will degenerate into a type of steepest descent method. On the other hand, if maximum_bracket_step is too large, then the line minimizations may draw the magnetization far away from a local energy minimum (i.e., one on the full 3N dimensional magnetization space), eventually ending up in a different, more distant minimum. The value for maximum_bracket_step is specified in degrees, with default value 10.

The line_minimum_angle_precision and line_minimum_relwidth values determine the precision of the individual line minimizations, not the total minimization procedure, which is governed by the stopping criteria specified in the driver's Specify block. However, these values are important because the precision of the line minimizations affects the the line direction sequence orthogonality. If both are too coarse, then the selected line directions will quickly drift away from mutual orthogonality. Conversely, setting either too fine will produce additional line minimization steps that do nothing to improve convergence towards the energy minimum in the full 3N dimensional magnetization space.

The energy_precision parameter estimates the relative precision of the energy computations. This is used to introduce a slack factor into the energy comparisons during the bracketing and line minimization stages, that is, if the computed energy values at two points have relative error difference smaller than eprecision, they are treated as having the same energy. The default value for eprecision is 1e-10. The true precision will depend primarily on the number of spins in the simulation. It may be necessary for very large simulations to increase the eprecision value.

The method parameter can be set to either Fletcher-Reeves or Polak-Ribiere to specify the conjugate gradient direction selection algorithm. The default is Fletcher-Reeves, which has somewhat smaller memory requirements.

The last parameter, fixed_spins, performs the same function as for the Oxs_EulerEvolve class.

The Oxs_CGEvolve module provides seven scalar outputs and two vector field outputs. The scalar outputs are

The vector field outputs are

Examples: cgtest.mif, stdprob3.mif, yoyo.mif.


Drivers

While evolvers are responsible for moving the simulation forward in individual steps, drivers coordinate the action of the evolver on the simulation as a whole, by grouping steps into tasks, stages and runs.

Tasks are small groups of steps that can be completed without adversely affecting user interface responsiveness. Stages are larger units specified by the MIF problem description; in particular, problem parameters are not expected to change in a discontinuous manner inside a stage. The run is the complete sequence of stages, from problem start to finish. The driver detects when stages and runs are finished, using criteria specified in the MIF problem description, and can enforce constraints, such as making sure stage boundaries respect time stopping criteria.

There are two drivers in Oxs, Oxs_TimeDriver for controlling time evolvers such as Oxs_RungeKuttaEvolve, and Oxs_MinDriver for controlling minimization evolvers like Oxs_CGEvolve.

Oxs_TimeDriver:
The Oxs time driver is Oxs_TimeDriver. The specify block has the form
Specify Oxs_TimeDriver:name {
evolver evolver_spec
mesh mesh_spec
Ms scalar_field_spec
m0 vector_field_spec
stopping_dm_dt torque_criteria
stopping_time time_criteria
stage_iteration_limit stage_iteration_count
total_iteration_limit total_iteration_count
stage_count number_of_stages
stage_count_check test
checkpoint_file restart_file_name
checkpoint_interval checkpoint_minutes
checkpoint_cleanup cleanup_behavior
start_iteration iteration
start_stage stage
start_stage_iteration stage_iteration
start_stage_start_time stage_time
start_stage_elapsed_time stage_elapsed_time
start_last_timestep timestep
normalize_aveM_output aveMflag
report_max_spin_angle report
}

The first four parameters, evolver, mesh, Ms and m0 provide references to a time evolver, a mesh, a scalar field and a vector field, respectively. Here Ms is the pointwise saturation magnetization in A/m, and m0 is the initial configuration for the magnetization unit spins, i.e., |m| = 1 at each point. These four parameters are required.

The next group of 3 parameters control stage stopping criteria. The stopping_dm_dt value, in degrees per nanosecond, specifies that a stage should be considered complete when the maximum | dm/dt| across all spins drops below this value. Similarly, the stopping_time value specifies the maximum ``Simulation time,'' i.e., the Landau-Lifshitz-Gilbert ODE (2), (3) time, allowed per stage. For example, if time_criteria is 1e-9, then no stage will evolve for more than 1 ns. If there were a total of 5 stages in the simulation, then the total simulation time would be not more than 5 ns. The third way to terminate a stage is with a stage_iteration_limit. This is a limit on the number of successful evolver steps allowed per stage. A stage is considered complete when any one of these three criteria are met. Each of the criteria may be either a single value, which is applied to every stage, or else a grouped list of values. If the simulation has more stages than a criteria list has entries, then the last criteria value is applied to all additional stages. These stopping criteria all provide a default value of 0, meaning no constraint, but usually at least one is specified since otherwise there is no automatic stage termination control. For quasi-static simulations, a stopping_dm_dt value in the range of 1.0 to 0.01 is reasonable; the numerical precision of the energy calculations usually makes in not possible to obtain | dm/dt| much below 0.001 degree per nanosecond.

The total_iteration_limit, stage_count and stage_count_check parameters involve simulation run completion conditions. The default value for the first is 0, interpreted as no limit, but one may limit the total number of steps performed in a simulation by specifying a positive integer value here. The more usual run completion condition is based on the stage count. If a positive integer value is specified for stage_count, then the run will be considered complete when the stage count reaches that value. If stage_count is not specified, or is given the value 0, then the effective number_of_stages value is computed by examining the length of the stopping criteria lists, and also any other Oxs_Ext object that has stage length expectations, such as Oxs_UZeeman. The longest of these is taken to be the stage limit value. Typically these lengths, along with stage_count if specified, will all be the same, and any differences indicate an error in the MIF file. Oxs will automatically test this condition, provided stage_count_check is set to 1, which is the default value. Stage length requests of 0 or 1 are ignored in this test, since those lengths are commonly used to represent sequences of arbitrary length. At times a short sequence is intentionally specified that is meant to be implicitly extended to match the full simulation stage length. In this case, the stage count check can be disabled by setting test to 0.

The checkpoint options are used to control the saving of solver state to disk; these saves are used by the oxsii and boxsi restart feature. The value of the checkpoint_file option is the name to use for the solver state file. The default is base_file_name.restart.

Cleanup of the checkpoint file is determined by the setting of checkpoint_cleanup, which should be one of normal (the default), done_only, or never. Under the normal setting, the checkpoint file is automatically deleted upon normal program termination, either because the solver reached the end of the problem, or because the user interactively terminated the problem prematurely. If cleanup_behavior is set to done_only, then the checkpoint file is only deleted if the problem endpoint is reached. If cleanup_behavior is never, then OOMMF does not delete checkpoint file; the user is responsible for deleting this file as she desires.

The checkpoint_interval value is the time in minutes between overwrites of the checkpoint file. No checkpoint file is written until checkpoint_minutes have elapsed. Checkpoint writes occur between solver iterations, so the actual interval time may be somewhat longer than the specified time. If checkpoint_minutes is 0, then each step is saved. Setting checkpoint_minutes to -1 disables checkpointing. The default checkpoint interval is 15 minutes.

The six start_* options control the problem run start point. These are intended primarily for automatic use by the restart feature. The default value for each is 0.

The normalize_aveM_output option is used to control the scaling and units on the average magnetization components Mx , My and Mz sent as DataTable output (this includes output sent to mmDataTable, mmGraph, and mmArchive). If aveMflag is true (1), then the output values are scaled to lie in the range [- 1, 1] , where the extreme values are obtained only at saturation (i.e., all the spins are aligned). If aveMflag is false (0), then the output is in A/m. The default setting is 1.

In the older MIF 2.1 format, the driver Specify block supports three additional values: basename, scalar_output_format, and vector_field_output_format. In the MIF 2.2 format these output controls have been moved into the SetOptions block. See the SetOptions documentation for details.

Oxs_TimeDriver provides 11 scalar outputs and 2 vector field outputs. The scalar outputs are

The three ``Max Spin Ang'' outputs are disabled by default. In general one should refer instead to the neighboring spin angle outputs provided by the exchange energies. However, for backward compatibility, or for simulations without any exchange energy terms, the driver spin angle outputs can be enabled by setting the report_max_spin_angle option to to 1.

The vector field outputs are

Examples: sample.mif, pulse.mif.

Oxs_MinDriver:
The Oxs driver for controlling minimization evolvers is Oxs_MinDriver. The specify block has the form
Specify Oxs_MinDriver:name {
evolver evolver_spec
mesh mesh_spec
Ms scalar_field_spec
m0 vector_field_spec
stopping_mxHxm torque_criteria
stage_iteration_limit stage_iteration_count
total_iteration_limit total_iteration_count
stage_count number_of_stages
stage_count_check test
checkpoint_file restart_file_name
checkpoint_interval checkpoint_minutes
checkpoint_cleanup cleanup_behavior
start_iteration iteration
start_stage stage
start_stage_iteration stage_iteration
start_stage_start_time stage_time
start_stage_elapsed_time stage_elapsed_time
start_last_timestep timestep
normalize_aveM_output aveMflag
report_max_spin_angle report
}

These parameters are the same as those described for the Oxs_TimeDriver class, except that stopping_mxHxm replaces stopping_dm_dt, and there is no analogue to stopping_time. The value for stopping_mxHxm is in A/m, and may be a grouped list . Choice depends on the particulars of the simulation, but typical values are in the range 10 to 0.1. Limits in the numerical precision of the energy calculations usually makes it not possible to obtain |m x H x m| below about 0.01 A/m. This control can be disabled by setting it to 0.0.

As with Oxs_TimeDriver, in the older MIF 2.1 format this Specify block supports three additional values: basename to control output filenames, and output format controls scalar_output_format and vector_field_output_format. In the MIF 2.2 format these output controls have been moved into the SetOptions block. See the SetOptions documentation for details.

Oxs_MinDriver provides 9 scalar outputs and 2 vector field outputs. The scalar outputs are

As is the case for the Oxs_TimeDriver, the three ``Max Spin Ang'' outputs are disabled by default. They can be enabled by setting the report_max_spin_angle option to to 1.

The vector field outputs are

Examples: cgtest.mif, stdprob3.mif.


Field Objects

Field objects return values (either scalar or vector) as a function of position. These are frequently used as embedded objects inside Specify blocks of other Oxs_Ext objects to initialize spatially varying quantities, such as material parameters or initial magnetization spin configurations. Units on the returned values will be dependent upon the context in which they are used.

Scalar field objects are documented first. Vector field objects are considered farther below.

Oxs_UniformScalarField:
Returns the same constant value regardless of the import position. The Specify block takes one parameter, value, which is the returned constant value. This class is frequently embedded inline to specify homogeneous material parameters. For example, inside a driver Specify block we may have 
Specify Oxs_TimeDriver {
    ...
    Ms { Oxs_UniformScalarField {
       value 8e5
    }}
    ...
}
As discussed in the section on Oxs_Ext referencing in the MIF 2 documentation, when embedding Oxs_UniformScalarField or Oxs_UniformVectorField objects, a notational shorthand is allowed that lists only the value. The previous example is exactly equivalent to 
Specify Oxs_TimeDriver {
    ...
    Ms 8e5
    ...
}
where an implicit Oxs_UniformScalarField object is created with value set to 8e5.

Examples: sample.mif, cgtest.mif.

Oxs_AtlasScalarField:
Declares values that are defined across individual regions of an Oxs_Atlas. The Specify block looks like
Specify Oxs_AtlasScalarField {
atlas atlas_spec
multiplier mult
default_value scalar_field_spec
values {
region1_label scalar_field_spec1
region2_label scalar_field_spec2
...
}
}

The specified atlas is used to map cell locations to regions; the value at the cell location of the scalar field from the corresponding values sub-block is assigned to that cell. The default_value entry is optional; if specified, and if a cell's region is not included in the values sub-block, then the default_value scalar field is used. If default_value is not specified, then missing regions will raise an error.

The scalar field entries may specify any of the scalar field types described in this (Field Objects) section. As usual, one may provide a single numeric value in any of the scalar_field_spec positions; this will be interpreted as requesting a uniform (spatially homogeneous) field with the indicated value.

If the optional multiplier value is provided, then each field value is scaled (multiplied) by the value mult.

The vector field analogue to this class is Oxs_AtlasVectorField, which is described below in the vector fields portion of this section.

Examples: diskarray.mif, ellipsoid.mif, grill.mif, spinvalve.mif, tclshapes.mif.

Oxs_LinearScalarField:
Returns a value that varies linearly with position. The Specify block has the form:
Specify Oxs_LinearScalarField {
norm value
vector { vx  vy  vz }
offset off
}

If optional value norm is specified, then the given vector is first scaled to the requested size. The offset entry is optional, with default value 0. For any given point (x, y, z) , the scalar value returned by this object will be xvx + yvy + zvz + off .

Example: spinvalve-af.mif.

Oxs_RandomScalarField:
Defines a scalar field that varies spatially in a random fashion. The Specify block has the form:
Specify Oxs_RandomScalarField {
range_min minvalue
range_max maxvalue
cache_grid mesh_spec
}

The value at each position is drawn uniformly from the range declared by the two required parameters, range_min and range_max. There is also an optional parameter, cache_grid, which takes a mesh specification that describes the grid used for spatial discretization. If cache_grid is not specified, then each call to Oxs_RandomScalarField generates a different field. If you want to use the same random scalar field in two places (as a base for setting, say anisotropy coefficients and saturation magnetization), then specify cache_grid with the appropriate (usually the base problem) mesh.

Examples: randomshape.mif, stdprob1.mif.

Oxs_ScriptScalarField:
Analogous to the parallel Oxs_ScriptVectorField class, this class produces a scalar field dependent on a Tcl script and optionally other scalar and vector fields. The Specify block has the form
Specify Oxs_ScriptScalarField:name {
script Tcl_script
script_args { args_request }
scalar_fields { scalar_field_spec ...}
vector_fields { vector_field_spec ...}
atlas atlas_spec
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
}

For each point of interest, the specified script is called with the arguments requested by script_args appended to the command, as explained in the User Defined Support Procedures section of the MIF 2 file format documentation. The value for script_args should be a subset of {rawpt relpt minpt maxpt span scalars vectors }.

If rawpt is requested, then when the Tcl proc is called, at the corresponding spot in the argument list the x, y, z values of point will be placed, in problem coordinates (in meters). The points so passed will usually be node points in the simulation discretization (the mesh), but this does not have to be the case in general. The relpt, minpt, maxpt, and span rely on a definition of a bounding box, which is an axes parallel parallelepiped. The bounding box must be specified by either referencing an atlas, or by explicitly stating the range via the three entries xrange, yrange, zrange (in meters). The minpt and maxpt arguments list the minimum and maximum values of the bounding box (coordinate by coordinate), while span provides the 3-vector resulting from (maxpt - minpt) . The relpt selection provides x_rel, y_rel, z_rel, where each element lies in the range [0, 1] , indicating a relative position between minpt and maxpt, coordinate-wise.

Each of the script_args discussed so far places exactly 3 arguments onto the Tcl proc argument list. The last two, scalars and vectors, place arguments depending on the size of the scalar_fields and vector_fields lists. The scalar_fields value is a list of other scalar field objects. Each scalar field is evaluated at the point in question, and the resulting scalar value is placed on the Tcl proc argument list, in order. The vector_fields option works similarly, except each vector field generates three points for the Tcl proc argument list, since the output from vector field objects is a three vector. Although the use of these entries appears complicated, this is a quite powerful facility that allows nearly unlimited control for the modification and combination of other field objects. Both scalar_fields and vector_fields entries are optional.

If script_args is not specified, the default value relpt is used.

Note that if script_args includes relpt, minpt, maxpt, or span, then a bounding box must be specified, as discussed above. The following example uses the explicit range method. See the Oxs_ScriptVectorField documentation for an example using an atlas specification. 

proc Ellipsoid { xrel yrel zrel } {
    set xrad [expr {$xrel - 0.5}]
    set yrad [expr {$yrel - 0.5}]
    set zrad [expr {$zrel - 0.5}]
    set test [expr {$xrad*$xrad+$yrad*$yrad+$zrad*$zrad}]
    if {$test>0.25} {return 0}
    return 8.6e5
}

Specify Oxs_ScriptScalarField {
    script Ellipsoid
    xrange { 0   1e-6 }
    yrange { 0 250e-9 }
    zrange { 0  50e-9 }

}
This Oxs_ScriptScalarField object returns 8.6e5 if the import (x,y,z) lies within the ellipsoid inscribed inside the axes parallel parallelepiped defined by (xmin=0, ymin=0, zmin=0) and (xmax=1e-6, ymax=250e-9, zmax=50e-9), and 0 otherwise. See also the discussion of the ReadFile MIF extension command for an example using an imported image file for similar purposes.

Below is one more example, illustrating the use of the vector_fields option. 

proc DotProduct { x1 y1 z1 x2 y2 z2 } {
    return [expr {$x1*$x2+$y1*$y2+$z1*$z2}]
}

Specify Oxs_FileVectorField:file1 {
    atlas :atlas
    file  file1.omf
}

Specify Oxs_UniformVectorField:dir111 {
    norm 1
    vector {1 1 1}
}

Specify Oxs_ScriptScalarField:project {
    script DotProduct
    script_args vectors
    vector_fields {:file1 :dir111}
}
The scalar field :project yields at each point in space the projection of the vector field :file1 onto the [1,1,1] direction.

Examples: antidots-filled.mif, ellipsoid-fieldproc.mif, manyregions-scriptfields.mif, manyspheres.mif, varalpha.mif.

Oxs_VecMagScalarField:
The Oxs_VecMagScalarField class produces a scalar field from a vector field by taking the norm of the vector field on a point-by-point basis, i.e.,

|$\displaystyle \mbox{\boldmath$v$}$| = $\displaystyle \sqrt{{v_x^2+v_y^2+v_z^2}}$.

The Specify block has the form:
Specify Oxs_VecMagScalarField {
field vector_field_spec
multiplier mult
offset off
}

The multiplier and offset entries are applied after the vector norm, i.e., the resulting scalar field is mult * |v | + off . The default values for mult and off are 1 and 0, respectively.

The functionality of the Oxs_VecMagScalarField class may be achieved with the Oxs_ScriptScalarField class by using the vector_fields option and a Tcl script to compute the vector norm. However, this particular functionality is needed frequently enough that a specialized class is useful. For example, this class can be used in conjunction with a vector field object to set both the saturation magnetization distribution (Ms ) and the initial magnetization: 

Specify Oxs_FileVectorField:file1 {
    atlas :atlas
    file  file1.omf
}

Specify Oxs_TimeDriver {
    basename test
    evolver :evolve
    stopping_dm_dt 0.01
    mesh :mesh
    m0 :file1
    Ms { Oxs_VecMagScalarField {
       field :file1
    }}
}

Example: sample-vecrotate.mif.

Oxs_ScriptOrientScalarField:
Scalar fields provide scalar values as a function of position across three-space. The Oxs_ScriptOrientScalarField class is used to compose a transformation on the input position before evaluation by a scalar field. The Specify block has the form:
Specify Oxs_ScriptOrientScalarField:name {
field scalar_field_spec
script Tcl_script
script_args { args_request }
atlas atlas_spec
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
}

The field argument should refer to a scalar field object. The script is a Tcl script that should return a position vector that will be sent on the field object to ultimately produce a scalar value. The arguments to the Tcl_script are determined by script_args, which should be a subset of {relpt rawpt minpt maxpt span }. If any arguments other than rawpt are requested, then the bounding box must be specified by either the atlas option, or else through the three xrange, yrange, zrange entries. The default value for script_args is relpt.

The Oxs_ScriptOrientScalarField class can be used to change the ``orientation'' of a scalar field, as in the following simple example, which reflects the :file1mag scalar field across the yz-plane: 

Specify Oxs_FileVectorField:file1 {
    atlas :atlas
    file  file1.omf
}

Specify Oxs_VecMagScalarField:file1mag {
   field :file1
}

proc Reflect { x y z xmin ymin zmin xmax ymax zmax} {
   return [list [expr {($xmax+$xmin-$x)}] $y $z]
}

Specify Oxs_ScriptOrientScalarField:reflect {
   field :file1mag
   script Reflect
   script_args {rawpt minpt maxpt}
   atlas :atlas
}
See also the Oxs_ScriptOrientVectorField class for analogous operations on vector fields.

Example: sample-reflect.mif.

Oxs_AffineOrientScalarField:
The Oxs_AffineOrientScalarField class is similar to the Oxs_ScriptOrientScalarField class, except that the transformation on the import position is by an affine transformation defined in terms of a 3x3 matrix and an offset instead of a Tcl script. Although this functionality can be obtained by an appropriate Tcl script, the Oxs_AffineOrientScalarField is easier to use and will run faster, as the underlying transformation is performed by compiled C++ instead of Tcl script.

The Specify block has the form:

Specify Oxs_AffineOrientScalarField {
field scalar_field_spec
M { matrix_entries ... }
offset { offx  offy  offz }
inverse invert_flag
inverse_slack slack
}

If F(x ) represents the scalar field specified by the field value, then the resulting transformed scalar field is F(Mx + off) . Here M is a 3x3 matrix, which may be specified by a list of 1, 3, 6 or 9 entries. If the matrix_entries list consists of a single value, then M is taken to be that value times the identity matrix, i.e., M is a homogeneous scaling transformation. If matrix_entries consists of 3 values, then M is taken to be the diagonal matrix with those three values along the diagonal. If matrix_entries is 6 elements long, then M is assumed to be a symmetric matrix, where the 6 elements specified correspond to M11 , M12 , M13 , M22 , M23 , and M33 . Finally, if matrix_entries is 9 elements long, then the elements specify the entire matrix, in the order M11 , M12 , M13 , M21 , ..., M33 . If M is not specified, then it is taken to be the identity matrix.

The offset entry is simply a 3-vector that is added to Mx . If offset is not specified, then it is set to the zero vector.

It is frequently the case that the transformation that one wants to apply is not Mx + off , but rather the inverse, i.e., M-1(x - off) . Provided M is nonsingular, this can be accomplished by setting the inverse option to 1. In this case the matrix M.M-1 is compared to the identity matrix, to check the accuracy of the matrix inversion. If any entry in M.M-1 differs from I by more than the 8-byte float machine precision (typically 2e-16) times the value of inverse_slack, then an error is raised. The default setting for invert_flag is 0, meaning don't invert, and the default setting for slack is 128.

Here is an example using Oxs_AffineOrientScalarField to rotate a field by 90 degrees counterclockwise about the z -axis. Note that the specified atlas is square in x and y , with the origin of the atlas coordinates in the center of the atlas volume. 

Specify Oxs_BoxAtlas:atlas {
  xrange {-250e-9 250e-9}
  yrange {-250e-9 250e-9}
  zrange { -15e-9  15e-9}
}

Specify Oxs_FileVectorField:file1 {
    atlas :atlas
    file  file1.omf
}

Specify Oxs_VecMagScalarField:file1mag {
   field :file1
}

Specify Oxs_AffineOrientScalarField:reflect {
   field :file1mag
   M { 0 1 0
      -1 0 0
       0 0 1 }
}

See also the Oxs_AffineOrientVectorField class for analogous operations on vector fields.

Example: sample-rotate.mif.

Oxs_AffineTransformScalarField:
Like the Oxs_AffineOrientScalarField class, this class composes an affine transform with a separate scalar field, but in this case the affine transform is applied after the field evaluation. The Specify block has the form:
Specify Oxs_AffineTransformScalarField {
field scalar_field_spec
multiplier mult
offset off
inverse invert_flag
}

If F(x ) represents the scalar field specified by the field value, then the resulting scalar field is mult*F(x ) + off . Since the output from F is a scalar, both multiplier and offset are scalars. If inverse is 1, then the transform is changed to $ \left(\vphantom{F(\mbox{\boldmath $x$})-\textrm{off}}\right.$F(x ) - off$ \left.\vphantom{F(\mbox{\boldmath $x$})-\textrm{off}}\right)$/mult , provided mult is non-zero.

The default values for mult, off, and invert_flag are 1, 0, and 0, respectively. The field value is the only required entry.

The functionality provided by Oxs_AffineTransformScalarField can also be produced by the Oxs_ScriptScalarField class with the scalar_fields entry, but the Oxs_AffineTransformScalarField class is faster and has a simpler interface. See also the Oxs_AffineTransformVectorField class for analogous operations on vector fields.

Example: sample-rotate.mif.

Oxs_ImageScalarField:
This class creates a scalar field using an image. The Specify block has the form
Specify Oxs_ImageScalarField:name {
image pic
invert invert_flag
multiplier mult
offset off
viewplane view
atlas atlas_spec
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
exterior ext_flag
}

The image is interpreted as a monochromatic map, yielding a scalar field with black corresponding to zero and white to one if invert is 0 (the default), or with black corresponding to 1 and white to 0 if invert is 1. Color images are converted to grayscale by simply summing the red, green, and blue components. A multiplier option is available to change the range of values from [0, 1] to [0,mult] , after which the offset value, if any, is added.

The viewplane is treated in the same manner as the viewplane option in the Oxs_ImageAtlas class, and should likewise take one of the three two-letter codes xy (default), zx or yz. The spatial scale is adjusted to fit the volume specified by either the atlas or xrange/yrange/zrange selections. If the specified volume does not fill the entire simulation volume, then points outside the specified volume are handled as determined by the exterior setting, which should be either a floating point value, or one of the keywords boundary or error. In the first case, the floating point value is treated as a default value for points outside the image, and should have a value in the range [0, 1] . The multiplier and offset adjustments are made to this value in the same way as to points inside the image. If ext_flag is boundary, then points outside the image are filled with the value of the closest point on the boundary of the image. If ext is error (the default), then an error is raised if a value is needed for any point outside the image.

Examples: rotatecenterstage.mif, sample-reflect.mif.

The available vector field objects are:

Oxs_UniformVectorField:
Returns the same constant value regardless of the import position. The Specify block takes one required parameter, vector, which is a 3-element list of the vector to return, and one optional parameter, norm, which if specified adjusts the size of export vector to the specified magnitude. For example,
Specify Oxs_UniformVectorField {
norm 1
vector {1 1 1}
}

This object returns the unit vector (a, a, a) , where a=1/sqrt(3), regardless of the import position.

This class is frequently embedded inline to specify spatially uniform quantities. For example, inside a driver Specify block we may have 

Specify Oxs_TimeDriver {
    ...
    m0 { Oxs_UniformVectorField {
       vector {1 0 0}
    }}
    ...
}
As discussed in the section on Oxs_Ext referencing in the MIF 2 documentation, when embedding Oxs_UniformVectorField or Oxs_UniformScalarField objects, a notational shorthand is allowed that lists only the required value. The previous example is exactly equivalent to 
Specify Oxs_TimeDriver {
    ...
    m0 {1 0 0}
    ...
}
where an implicit Oxs_UniformVectorField object is created with the value of vector set to {1 0 0 }.

Examples: sample.mif, cgtest.mif.

Oxs_AtlasVectorField:
Declares vector values that are defined across individual regions of an Oxs_Atlas. The Specify block has the form
Specify Oxs_AtlasVectorField {
atlas atlas_spec
norm magval
multiplier mult
default_value vector_field_spec
values {
region1_label vector_field_spec1
region2_label vector_field_spec2
...
}
}

Interpretation is analogous to the Oxs_AtlasScalarField specify block, except here the output values are 3 dimensional vectors rather than scalars. Thus the values associated with each region are vector fields rather than scalar fields. Any of the vector field types described in this (Field Objects) section may be used. As usual, one may provided a braced list of three numeric values to request a uniform (spatially homogeneous) vector field with the indicated value.

The optional norm parameter causes each vector value to be scaled to have magnitude magval. The optional multiplier value scales the field values. If both norm and multiplier are specified, then the field vectors are first normalized before being scaled by the multiplier value.

Examples: diskarray.mif, exchspring.mif, imageatlas.mif, spinvalve.mif.

Oxs_ScriptVectorField:
Conceptually similar to the Oxs_ScriptScalarField scalar field object, except that the script should return a vector (as a 3 element list) rather than a scalar. In addition to the parameters accepted by Oxs_ScriptScalarField, Oxs_ScriptVectorField also accepts an optional parameter norm. If specified, the return values from the script are size adjusted to the specified magnitude. If both norm and multiplier are specified, then the field vectors are first normalized before being scaled by the multiplier value.

The following example produces a vortex-like unit vector field, with an interior core region pointing parallel to the z -axis. Here the scaling region is specified using an atlas reference to an object named ``:atlas'', which is presumed to be defined earlier in the MIF file. See the Oxs_ScriptScalarField sample Specify block for an example using the explicit range option. 

proc Vortex { xrel yrel zrel } {
    set xrad [expr {$xrel-0.5}]
    set yrad [expr {$yrel-0.5}]
    set normsq [expr {$xrad*$xrad+$yrad*$yrad}]
    if {$normsq <= 0.025} {return "0 0 1"}
    return [list [expr {-1*$yrad}] $xrad 0]
}

Specify Oxs_ScriptVectorField {
    script Vortex
    norm  1
    atlas :atlas
}
See also the Oxs_MaskVectorField documentation and the discussion of the ReadFile MIF extension command

for other example uses of the Oxs_ScriptVectorField class.

Examples: cgtest.mif, ellipsoid.mif, manyregions-scriptfields.mif, sample-vecreflect.mif, stdprob3.mif, yoyo.mif.

Oxs_FileVectorField:
Provides a file-specified vector field. The Specify block has the form
Specify Oxs_FileVectorField {
file filename
atlas atlas_spec
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
spatial_scaling { xscale yscale zscale }
spatial_offset { xoff yoff zoff }
exterior ext_flag
norm magnitude
multiplier mult
}

Required values in the Specify block are the name of the input vector field file and the desired scaling parameters. The filename is specified via the file entry, which names a file containing a vector field in one of the formats recognized by avf2ovf. If atlas or xrange/yrange/zrange are specified, then the file will be scaled and translated as necessary to fit that scaling region, in the same manner as done, for example, by the Oxs_ScriptScalarField and Oxs_ScriptVectorField classes. Alternatively, one may specify spatial_scaling and spatial_offset directly. In this case the vector spatial positions are taken as specified in the file, multiplied component-wise by (xscale,yscale,zscale), and then translated by (xoff,yoff,zoff). If you want to use the spatial coordinates as directly specified in the file, use (1,1,1) for spatial_scaling and (0,0,0) for spatial_offset.

In all cases, once the input field has been scaled and translated, it is then sub-sampled (zeroth-order fit) as necessary to match the simulation mesh.

The exterior flag determines the behavior at ``exterior points'', i.e., locations (if any) in the simulation mesh that lie outside the extent of the scaled and translated vector field. The ext_flag should be either a three-vector, or one of the keywords boundary or error. If a three-vector is given, then that value is supplied at all exterior points. If ext_flag is set to boundary, then the value used is the point on the boundary of the input vector field that is closest to the exterior point. The default setting for ext_flag is error, which raises an error if there are any exterior points.

The magnitude of the field can be modified by the optional norm and multiplier attributes. If the norm parameter is given, then each vector in the field will be renormalized to the specified magnitude. If the multiplier parameter is given, then each vector in the field will be multiplied by the given scalar value. If the multiplier value is negative, the field direction will be reversed. If both norm and multiplier are given, then the field vectors are renormalized before being scaled by the multiplier value.

Examples: stdprob3.mif, yoyo.mif.

Oxs_RandomVectorField:
Similar to Oxs_RandomScalarField, but defines a vector field rather than a scalar field that varies spatially in a random fashion. The Specify block has the form:
Specify Oxs_RandomVectorField {
min_norm minvalue
max_norm maxvalue
cache_grid mesh_spec
}

The Specify block takes two required parameters, min_norm and max_norm. The vectors produced will have magnitude between these two specified values. If min_norm = max_norm, then the samples are uniformly distributed on the sphere of that radius. Otherwise, the samples are uniformly distributed in the hollow spherical volume with inner radius min_norm and outer radius max_norm. There is also an optional parameter, cache_grid, which takes a mesh specification that describes the grid used for cache spatial discretization. If cache_grid is not specified, then each call to Oxs_RandomVectorField generates a different field. If you want to use the same random vector field in two places (as a base for setting, say anisotropy axes and initial magnetization), then specify cache_grid with the appropriate (usually the base problem) mesh.

Examples: diskarray.mif, sample2.mif, randomshape.mif stdprob1.mif.

Oxs_PlaneRandomVectorField:
Similar to Oxs_RandomVectorField, except that samples are drawn from 2D planes rather than 3-space. The Specify block has the form
Specify Oxs_RandomVectorField {
plane_normal vector_field_spec
min_norm minvalue
max_norm maxvalue
cache_grid mesh_spec
}

The min_norm, max_norm, and cache_grid parameters have the same meaning as for the Oxs_RandomVectorField class. The additional parameter, plane_normal, specifies a vector field that at each point provides a vector that is orthogonal to the plane from which the random vector at that point is to be drawn. If the vector field is specified explicitly as three real values, then a spatially uniform vector field is produced and all the random vectors will lie in the same plane. More generally, however, the normal vectors (and associated planes) may vary from point to point. As a special case, if a normal vector at a point is the zero vector, then no planar restriction is made and the resulting random vector is drawn uniformly from a hollow ball in three space satisfying the minimum/maximum norm constraints.

Example: sample2.mif.

Oxs_ScriptOrientVectorField:
This class is analogous to the Oxs_ScriptOrientScalarField class. The Specify block has the form:
Specify Oxs_ScriptOrientVectorField:name {
field vector_field_spec
script Tcl_script
script_args { args_request }
atlas atlas_spec
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
}

The interpretation of the specify block and the operation of the Tcl script is exactly the same as for the Oxs_ScriptOrientScalarField class, except the input field and the resulting field are vector fields instead of scalar fields.

Note that the ``orientation'' transformation is applied to the import spatial coordinates only, not the output vector. For example, if the field value represents a shaped vector field, and the script proc is a rotation transformation, then the resulting vector field shape will be rotated as compared to the original vector field, but the output vectors themselves will still point in their original directions. In such cases one may wish to compose the Oxs_ScriptOrientVectorField with a Oxs_ScriptVectorField object to rotate the output vectors as well. This situation occurs also with the Oxs_AffineOrientVectorField class. See the Oxs_AffineTransformVectorField class documentation for an example illustrating the composition of an object of that class with a Oxs_AffineOrientVectorField object.

Example: sample-vecreflect.mif.

Oxs_AffineOrientVectorField:
This class is analogous to the Oxs_AffineOrientScalarField class. The Specify block has the form:
Specify Oxs_AffineOrientVectorField {
field vector_field_spec
M { matrix_entries ... }
offset { offx  offy  offz }
inverse invert_flag
inverse_slack slack
}

The interpretation of the specify block and the affine transformation is exactly the same as for the Oxs_AffineOrientScalarField class, except the input field and the resulting field are vector fields instead of scalar fields.

As explained in the Oxs_ScriptOrientVectorField documentation, the ``orientation'' transformation is applied to the import spatial coordinates only, not the output vector. If one wishes to rotate the output vectors, then a Oxs_AffineTransformVectorField object may be applied with the opposite rotation. See that section for an example.

Examples: yoyo.mif, sample-vecrotate.mif.

Oxs_AffineTransformVectorField:
This class applies an affine transform to the output of a vector field. It is similar to the Oxs_AffineTransformScalarField class, except that in this case the affine transform is applied to a vector instead of a scalar. The Specify block has the form:
Specify Oxs_AffineTransformVectorField {
field vector_field_spec
M { matrix_entries ... }
offset { offx  offy  offz }
inverse invert_flag
inverse_slack slack
}

Because the output from field is a 3-vector, the transform defined by M and offset requires M to be a 3x3 matrix and offset to be a 3-vector. Thus, if v (x ) represents the vector field specified by the field value, then the resulting vector field is M.v (x ) + off .

M is described by a list of from one to nine entries, in exactly the same manner as for the Oxs_AffineOrientVectorField and Oxs_AffineOrientScalarField classes. The interpretation of offset, inverse, and inverse_slack is also the same. In particular, if invert_flag is 1, then the resulting vector field is M-1.$ \left(\vphantom{\mbox{\boldmath $v$}(\mbox{\boldmath $x$})-\textbf{off}}\right.$v (x ) - off$ \left.\vphantom{\mbox{\boldmath $v$}(\mbox{\boldmath $x$})-\textbf{off}}\right)$ .

The following example illustrates combining a Oxs_AffineTransformVectorField with a Oxs_AffineOrientVectorField to completely rotate a vector field. 

Specify Oxs_BoxAtlas:atlas {
  xrange {-80e-9 80e-9}
  yrange {-80e-9 80e-9}
  zrange {0  40e-9}
}
proc Trap { x y z } {
     if {$y<=$x && $y<=0.5} {return [list 0 1 0]}
     return [list 0 0 0]
}
Specify Oxs_ScriptVectorField:trap {
   script Trap
   atlas :atlas
}
Specify Oxs_AffineOrientVectorField:orient {
   field :trap
   M { 0 -1 0
       1  0 0
       0  0 1 }
   offset { -20e-9 0 0 }
   inverse 1
}
Specify Oxs_AffineTransformVectorField:rot {
   field :orient
   M { 0 -1 0
       1  0 0
       0  0 1 }
}
proc Threshold { vx vy vz } {
   set magsq [expr {$vx*$vx+$vy*$vy+$vz*$vz}]
   if {$magsq>0} {return 8e5}
   return 0.0
}
Specify Oxs_ScriptScalarField:Ms {
  vector_fields :rot
  script Threshold
  script_args vectors  
}
Specify Oxs_TimeDriver {
 m0 :rot
 Ms :Ms
 stopping_dm_dt 0.01
 evolver :evolve
 mesh :mesh
}
The base field here is given by the Oxs_ScriptVectorField:trap object, which produces a vector field having a trapezoidal shape with the non-zero vectors pointing parallel to the y -axis. The :orient and :rot transformations rotate the shape and the vectors counterclockwise 90 degrees. Additionally, the offset option in :orient translates the shape 20 nm towards the left. The original and transformed fields are illustrated below.

Original field Rotate field

Example: sample-vecrotate.mif.

Oxs_MaskVectorField:
Multiplies a vector field pointwise by a scalar vector field (the mask) to produce a new vector field. The Specify block has the form:
Specify Oxs_MaskVectorField {
mask scalar_field_spec
field vector_field_spec
}

This functionality can be achieved, if in a somewhat more complicated fashion, with the Oxs_ScriptVectorField class. For example, given a scalar field :mask and a vector field :vfield, this example using the Oxs_MaskVectorField class 

Specify Oxs_MaskVectorField {
   mask :mask
   field :vfield
}
is equivalent to this example using the Oxs_ScriptVectorField class 
proc MaskField { m vx vy vz } {
   return [list [expr {$m*$vx}] [expr {$m*$vy}] [expr {$m*$vz}]]
}
Specify Oxs_ScriptVectorField {
  script MaskField
  script_args {scalars vectors}
  scalar_fields { :mask }
  vector_fields { :vfield }
}
Of course, the Oxs_ScriptVectorField approach is easily generalized to much more complicated and arbitrary combinations of scalar and vector fields.

Example: rotatecenterstage.mif.

Oxs_ImageVectorField:
This class creates a vector field using an image. The Specify block has the form
Specify Oxs_ImageVectorField:name {
image pic
multiplier mult
vx_multiplier xmult
vy_multiplier ymult
vz_multiplier zmult
vx_offset xoff
vy_offset yoff
vz_offset zoff
norm norm_magnitude
viewplane view
atlas atlas_spec
xrange { xmin xmax }
yrange { ymin ymax }
zrange { zmin zmax }
exterior ext_flag
}

The image is interpreted as a three-color map, yielding a vector field where each (x,y,z) component is determined by the red, green, and blue color components, respectively....

The viewplane, atlas, xrange/yrange/zrange, and exterior are treated the same as for the Oxs_ImageScalarField class

Examples: NONE.

MIF Support Classes

Oxs_LabelValue:
A convenience object that holds label + value pairs. Oxs_LabelValue objects may be referenced via the standard attributes field in other Specify blocks, as in this example: 
Specify Oxs_LabelValue:probdata {
  alpha 0.5
  start_dm 0.01
}
Specify Oxs_EulerEvolve {
  attributes :probdata
}
The Specify block string for Oxs_LabelValue objects is an arbitrary Tcl list with an even number of elements. The first element in each pair is interpreted as a label, the second as the value. The attribute option causes this list to be dropped verbatim into the surrounding object. This technique is most useful if the label + value pairs in the Oxs_LabelValue object are used in multiple Specify blocks, either inside the same MIF file, or across several MIF files into which the Oxs_LabelValue block is imported using the ReadFile MIF extension command.

Examples: The MIF files sample-rotate.mif and sample-reflect.mif use the Oxs_LabelValue object stored in the sample-attributes.tcl file.

Refer to the MIF 2 documentation for details on the base format specification.

OOMMF Home next up previous Contents index

OOMMF Documentation Team
September 28, 2012