Merge branch 'develop' into molecule-refactor-for-json
This commit is contained in:
@ -29,6 +29,7 @@ OPT.
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* :doc:`ave/grid <fix_ave_grid>`
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* :doc:`ave/histo <fix_ave_histo>`
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* :doc:`ave/histo/weight <fix_ave_histo>`
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* :doc:`ave/moments <fix_ave_moments>`
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* :doc:`ave/time <fix_ave_time>`
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* :doc:`aveforce <fix_aveforce>`
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* :doc:`balance <fix_balance>`
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@ -208,6 +208,7 @@ accelerated styles exist.
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* :doc:`ave/grid <fix_ave_grid>` - compute per-grid time-averaged quantities
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* :doc:`ave/histo <fix_ave_histo>` - compute/output time-averaged histograms
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* :doc:`ave/histo/weight <fix_ave_histo>` - weighted version of fix ave/histo
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* :doc:`ave/moments <fix_ave_moments>` - compute moments of scalar quantities
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* :doc:`ave/time <fix_ave_time>` - compute/output global time-averaged quantities
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* :doc:`aveforce <fix_aveforce>` - add an averaged force to each atom
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* :doc:`balance <fix_balance>` - perform dynamic load-balancing
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296
doc/src/fix_ave_moments.rst
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296
doc/src/fix_ave_moments.rst
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@ -0,0 +1,296 @@
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.. index:: fix ave/moments
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fix ave/moments command
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=======================
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Syntax
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""""""
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.. code-block:: LAMMPS
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fix ID group-ID ave/moments Nevery Nrepeat Nfreq value1 value2 ... moment1 moment2 ... keyword args ...
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* ID, group-ID are documented in :doc:`fix <fix>` command
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* ave/moments = style name of this fix command
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* Nevery = use input values every this many time steps
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* Nrepeat = # of times to use input values for calculating averages
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* Nfreq = calculate averages every this many time steps
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* one or more input variables can be listed
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* value = v_name
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.. parsed-literal::
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c_ID = global scalar calculated by a compute with ID
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c_ID[I] = Ith component of global vector calculated by a compute with ID, I can include wildcard (see below)
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f_ID = global scalar calculated by a fix with ID
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f_ID[I] = Ith component of global vector calculated by a fix with ID, I can include wildcard (see below)
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v_name = value calculated by an equal-style variable with name
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v_name[I] = value calculated by a vector-style variable with name, I can include wildcard (see below)
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* one or more moments to compute can be listed
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* moment = *mean* or *stddev* or *variance* or *skew* or *kurtosis*, see exact definitions below.
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* zero or more keyword/arg pairs may be appended
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* keyword = *start* or *history*
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.. parsed-literal::
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*start* args = Nstart
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Nstart = invoke first after this time step
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*history* args = Nrecent
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Nrecent = keep a history of up to Nrecent outputs
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Examples
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""""""""
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.. code-block:: LAMMPS
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fix 1 all ave/moments 1 1000 100 v_volume mean stddev
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fix 1 all ave/moments 1 200 1000 v_volume variance kurtosis history 10
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Description
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"""""""""""
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.. versionadded:: TBD
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Using one or more values as input, calculate the moments of the underlying
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(population) distributions based on samples collected every few time
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steps over a time step window. The definitions of the moments calculated
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are given below.
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The group specified with this command is ignored. However, note that
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specified values may represent calculations performed by computes and
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fixes which store their own "group" definitions.
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Each listed value can be the result of a :doc:`compute <compute>` or
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:doc:`fix <fix>` or the evaluation of an equal-style or vector-style
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:doc:`variable <variable>`. In each case, the compute, fix, or variable
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must produce a global quantity, not a per-atom or local quantity.
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If you wish to spatial- or time-average or histogram per-atom
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quantities from a compute, fix, or variable, then see the :doc:`fix
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ave/chunk <fix_ave_chunk>`, :doc:`fix ave/atom <fix_ave_atom>`, or
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:doc:`fix ave/histo <fix_ave_histo>` commands. If you wish to sum a
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per-atom quantity into a single global quantity, see the :doc:`compute
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reduce <compute_reduce>` command.
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Many :doc:`computes <compute>` and :doc:`fixes <fix>` produce global
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quantities. See their doc pages for details. :doc:`Variables <variable>`
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of style *equal* and *vector* are the only ones that can be used with
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this fix. Variables of style *atom* cannot be used, since they produce
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per-atom values.
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The input values must all be scalars or vectors with a bracketed term
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appended, indicating the :math:`I^\text{th}` value of the vector is
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used.
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The result of this fix can be accessed as a vector, containing the
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interleaved moments of each input in order. If M moments are requested,
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then the moments of input 1 will be the first M values in the vector
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output by this fix. The moments of input 2 will the next M values, etc.
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If there are N values, the vector length will be N*M.
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----------
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For input values from a compute or fix or variable, the bracketed index
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I can be specified using a wildcard asterisk with the index to
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effectively specify multiple values. This takes the form "\*" or "\*n"
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or "m\*" or "m\*n". If :math:`N` is the size of the vector, then an
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asterisk with no numeric values means all indices from 1 to :math:`N`.
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A leading asterisk means all indices from 1 to n (inclusive). A
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trailing asterisk means all indices from n to :math:`N` (inclusive). A
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middle asterisk means all indices from m to n (inclusive).
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Using a wildcard is the same as if the individual elements of the vector
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or cells of the array had been listed one by one. For examples, see the
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description of this capability in :doc:`fix ave/time <fix_ave_time>`.
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----------
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The :math:`N_\text{every}`, :math:`N_\text{repeat}`, and
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:math:`N_\text{freq}` arguments specify on what time steps the input
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values will be used in order to contribute to the average. The final
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statistics are generated on time steps that are a multiple of
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:math:`N_\text{freq}`\ . The average is over a window of up to
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:math:`N_\text{repeat}` quantities, computed in the preceding portion of
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the simulation once every :math:`N_\text{every}` time steps.
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.. note::
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Contrary to most fix ave/* commands, it is not required that Nevery *
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Nrepeat <= Nfreq. This is to allow the user to choose the time
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window and number of samples contributing to the output at each
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Nfreq interval.
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For example, if :math:`N_\text{freq}=100` and :math:`N_\text{repeat}=5`
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(and :math:`N_\text{every}=1`), then on step 100 values from time steps
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96, 97, 98, 99, and 100 will be used. The fix does not compute its
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inputs on steps that are not required. If :math:`N_\text{freq}=5`,
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:math:`N_\text{repeat}=8` and :math:`N_\text{every}=1`, then values
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will first be calculated on step 5 from steps 1-5, on step 10 from 3-10,
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on step 15 from 8-15 and so on, forming a rolling average over
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timesteps that span a time window larger than Nfreq.
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----------
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If a value begins with "c\_", a compute ID must follow which has been
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previously defined in the input script. If no bracketed term is
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appended, the global scalar calculated by the compute is used. If a
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bracketed term is appended, the Ith element of the global vector
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calculated by the compute is used. See the discussion above for how I
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can be specified with a wildcard asterisk to effectively specify
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multiple values.
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If a value begins with "f\_", a fix ID must follow which has been
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previously defined in the input script. If no bracketed term is
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appended, the global scalar calculated by the fix is used. If a
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bracketed term is appended, the Ith element of the global vector
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calculated by the fix is used. See the discussion above for how I can
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be specified with a wildcard asterisk to effectively specify multiple
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values.
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Note that some fixes only produce their values on certain time steps,
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which must be compatible with *Nevery*, else an error will result.
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Users can also write code for their own fix styles and :doc:`add them to
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LAMMPS <Modify>`.
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If a value begins with "v\_", a variable name must follow which has been
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previously defined in the input script. Only equal-style or vector-style
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variables can be used, which both produce global values. Vector-style
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variables require a bracketed term to specify the Ith element of the
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vector calculated by the variable.
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Note that variables of style *equal* and *vector* define a formula which
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can reference individual atom properties or thermodynamic keywords, or
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they can invoke other computes, fixes, or variables when they are
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evaluated, so this is a very general means of specifying quantities to
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time average.
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----------
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The moments are output in the order requested in the arguments following
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the last input. Any number and order of moments can be specified,
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although it does not make much sense to specify the same moment multiple
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times. All moments are computed using a correction of the sample estimators
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used to obtain unbiased cumulants :math:`k_{1..4}` (see :ref:`(Cramer)
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<Cramer1>`). The correction for variance is the standard Bessel
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correction. For other moments, see :ref:`(Joanes)<Joanes1>`.
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For *mean*, the arithmetic mean :math:`\bar{x} = \frac{1}{n}
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\sum_{i=1}^{n} x_i` is calculated.
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For *variance*, the Bessel-corrected sample variance :math:`var = k_2 =
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\frac{1}{n - 1} \sum_{i=1}^{n} (x_i - \bar{x})^2` is calculated.
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For *stddev*, the Bessel-corrected sample standard deviation
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:math:`stddev = \sqrt{k_2}` is calculated.
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For *skew*, the adjusted Fisher--Pearson standardized moment :math:`G_1
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= \frac{k_3}{k_2^{3/2}} = \frac{k_3}{stddev^3}` is calculated.
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For *kurtosis*, the adjusted Fisher--Pearson standardized moment
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:math:`G_2 = \frac{k_4}{k_2^2}` is calculated.
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----------
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Fix invocation and output can be modified by optional keywords.
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The *start* keyword specifies that the first computation should be no
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earlier than the step number given (but will still occur on a multiple
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of *Nfreq*). The default is step 0. Often input values can be 0.0 at
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time 0, so setting *start* to a larger value can avoid including a 0.0
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in a longer series.
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The *history* keyword stores the Nrecent most recent outputs on Nfreq
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timesteps, so they can be accessed as global outputs of the fix. Nrecent
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must be >= 1. The default is 1, meaning only the most recent output is
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accessible. For example, if history 10 is specified and Nfreq = 1000,
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then on timestep 20000, the Nfreq outputs from steps 20000, 19000, ...
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11000 are available for access. See below for details on how to access
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the history values.
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For example, this will store the outputs of the previous 10 Nfreq
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time steps, i.e. a window of 10000 time steps:
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.. code-block:: LAMMPS
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fix 1 all ave/moments 1 200 1000 v_volume mean history 10
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The previous results can be accessed as values in a global array output
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by this fix. Each column of the array is the vector output of the N-th
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preceding Nfreq timestep. For example, assuming a single moment is
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calculated, the most recent result corresponding to the third input
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value would be accessed as "f_name[3][1]", "f_name[3][4]" is the 4th
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most recent and so on. The current vector output is always the first
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column of the array, corresponding to the most recent result.
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To illustrate the utility of keeping output history, consider using
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this fix in conjunction with :doc:`fix halt <fix_halt>` to stop a run
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automatically if a quantity is converged to within some desired tolerance:
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.. code-block:: LAMMPS
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variable target equal etot
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fix aveg all ave/moments 1 200 1000 v_target mean stddev history 10
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variable stopcond equal "abs(f_aveg[1]-f_aveg[1][10])<f_aveg[2]"
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fix fhalt all halt 1000 v_stopcond == 1
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In this example, every 1000 time steps, the average and standard
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deviation of the total energy over the previous 200 time steps are
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calculated. If the difference between the most recent and 10-th most
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recent average is lower than the most recent standard deviation, the run
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is stopped.
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----------
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Restart, fix_modify, output, run start/stop, minimize info
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"""""""""""""""""""""""""""""""""""""""""""""""""""""""""""
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No information about this fix is written to :doc:`binary restart files
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<restart>`.
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This fix produces a global vector and global array which can be accessed
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by various :doc:`output commands <Howto_output>`. The values can be
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accessed on any time step, but may not be current.
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A global vector is produced with the # of elements = number of moments *
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number of inputs. The moments are output in the order given in the fix
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definition. An array is produced having # of rows = length of vector
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output (with an ordering which matches the vector) and # of columns =
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value of *history*. There is always at least one column.
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Each element of the global vector or array can be either "intensive" or
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"extensive", depending on whether the values contributing to the element
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are "intensive" or "extensive". If a compute or fix provides the value
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being time averaged, then the compute or fix determines whether the value
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is intensive or extensive; see the page for that compute or fix for
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further info. Values produced by a variable are treated as intensive.
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No parameter of this fix can be used with the *start/stop* keywords of
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the :doc:`run <run>` command. This fix is not invoked during
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:doc:`energy minimization <minimize>`.
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Restrictions
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""""""""""""
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This compute is part of the EXTRA-FIX package. It is only enabled if
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LAMMPS was built with that package. See the :doc:`Build package
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<Build_package>` page for more info.
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Related commands
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""""""""""""""""
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:doc:`fix ave/time <fix_ave_time>`,
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Default
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"""""""
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The option defaults are history = 1, start = 0.
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----------
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.. _Cramer1:
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**(Cramer)** Cramer, Mathematical Methods of Statistics, Princeton University Press (1946).
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.. _Joanes1:
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**(Joanes)** Joanes, Gill, The Statistician, 47, 183--189 (1998).
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Reference in New Issue
Block a user