Command-line tools#
In addition to the Python API, flatspin comes with a set of powerful command-line tools. These are installed automatically as part of the flatspin package.
If you find that the commands are not available in your shell automatically, you may need to modify your PATH
variable.
The location of the command-line tools varies based on the operating system and installation method.
If you installed flatspin in your home directory (using pip install --user
):
export PATH=$PATH:$HOME/.local/bin
The command-line tools can be understood from the flatspin architecture:
In the figure, the arrows indicate data flow between the components:
The input encoder translates input to a field protocol (series of external fields).
The runner perturbs the ASI model according to the field protocol, and saves the results.
The results are stored in a dataset
Analysis tools read and process the dataset.
Note
A good understanding of the concepts introduced in the rest of this User Guide is beneficial to effectively use the command-line tools.
Running simulations#
flatspin simulations can be run directly from the command line, using the commands flatspin-run
and flatspin-run-sweep
.
These tools were designed to be flexible enough to allow for a range of different simulation scenarios.
Some notable features include:
Results are stored in the standard dataset format for later analysis.
All simulation parameters can be specified from the command-line.
Input encoders are used to define the external field.
Parameter sweeps can be defined to run many simulations in one go.
Simulations may be run in parallel on a compute cluster.
flatspin-run
#
To run a single flatspin simulation, use flatspin-run
.
Let us start with a simple example:
flatspin-run -o /tmp/flatspin/myrun -m SquareSpinIceClosed \
-e Triangle -p H=100e-3 -p phase=-90 -p phi=30 -p periods=1
Run 1/1: outdir=SquareSpinIceClosed.npz
Completed 80 steps in 0:00:00.925894
The -o/--basepath
argument specifies the directory where simulation results will be stored as a dataset.
This directory should not already exist, and will be automatically created by flatspin-run
.
The -m/--model
argument refers to the model class to use.
You may also specify your own model class by providing the full module path, e.g., -m mymodels.MySpinIce
.
The -e/--encoder
argument specifies the input encoder to use for defining the field protocol.
In the example, the Triangle
encoder is used which results in a linear ramped external field.
For a list of available encoders, see flatspin-run --list-encoders
.
You may also specify your own encoder class by providing the full module path, e.g., -e myencoders.MyEncoder
.
The -p/--param
arguments are parameters to the model, the runner and the encoder:
-p H=100e-3
sets the amplitude of the external field to 100 mT-p phase=-90
sets the phase of the triangle wave to -90°-p phi=30
sets the angle of the external field to 30°-p periods=1
sets the number of field cycles to 1
For a list of available parameters, append --list-params
to the flatspin-run
command.
The runner#
The runner
is responsible for running the simulation.
In simplified pseudocode, the runner does the following:
model = ModelClass(model_params)
encoder = EncoderClass(encoder_params)
h_ext = encoder(input)
for h in h_ext:
model.set_h_ext(h)
model.relax()
if should_sample:
record current state of the model
save recorded states as tables in the dataset
As you can see, the external field is what drives the simulation.
Each value of h_ext
is immediately followed by a call to model.relax()
, which flips any spins in response to the new field value.
Parameters#
The parameters passed by the -p/--param
arguments are consumed in the following order:
The model class (passed to the constructor)
The runner (passed to
flatspin.runner.run()
)The encoder class (passed to
Encoder.set_params()
It is assumed that there is never overlap between the parameter names for the model, runner and encoders.
For a list of available parameters, append --list-params
to the flatspin-run
command.
Documentation for each parameter can be found in the model class
, the runner
and the corresponding encoder class flatspin.encoder
.
Parameter values are evaluated as Python code (using eval).
Values may use numpy code, e.g., -p param=np.random.rand()
.
Some additional utility functions are also available, see flatspin.cmdline.param_globals
.
Input#
The input
to the encoder may provided in a few different ways:
Passed directly as an array:
-p input=[0.3, 0.5, 1.0]
Created indirectly:
-p periods=P
which is short-hand for-p input=[1]*P
Loaded from file:
-p input=myinput.csv
which is read withread_table()
. To select a specific column to use:-p input_key=column_name
.
Selecting the sample rate: spp
and timesteps
#
The encoder may produce many h_ext
values for each input
value.
The number of h_ext
values is typically controlled by the timesteps
encoder parameter.
For example, the Triangle
encoder uses timesteps=100
by default, meaning there will be 100 h_ext
field values per input
value.
The spp
runner parameter determines how often the state of the model should be sampled (and saved).
The parameter name spp
is an abbreviation for samples per period, and specifies the number samples per input period.
In the Triangle
example, we can use -p spp=100
to sample the model state after every h_ext
value, or
-p spp=50
to sample every other h_ext
value, or -p spp=1
to sample once for each input
value (sampled at the beginning of the input).
Some care must be taken when choosing spp
such that it is compatible with timesteps
.
It is the users responsibility to ensure that spp
evenly divides timesteps
(a warning is generated if it does not).
Time-varying parameters#
Some model parameters may also be modified dynamically over time.
Time-varying parameters can be defined by adding a _t
suffix to the parameter name, for example:
flatspin-run ... -p temperature_t='[400, 350, 300]'
will create a time-varying temperature with three values.
The length of all time-varying parameters must match the length of the input
.
Currently, the following time-varying parameters are supported:
alpha_t
, hc_t
, m_therm_t
, spin_t
, temperature_t
, therm_timescale_t
, threshold_t
The external field must be created using the input encoder, i.e., h_ext_t
is not allowed.
flatspin-run-sweep
#
Often we wish to explore how an ASI changes behavior under different parameters. Parameter sweeps is a simple and effective way to systematically explore the effect of one or multiple parameters.
flatspin-run-sweep
accepts a list of parameters to sweep, and runs a series of flatspin simulations using the given parameter values.
Continuing our simple example, we sweep the field strength H
:
flatspin-run-sweep -o /tmp/flatspin/mysweep -m SquareSpinIceClosed \
-e Triangle -p phase=-90 -phi=30 -p periods=1 \
-s 'H=[80e-3, 84e-3, 88e-3, 92e-3]'
Starting sweep with 4 runs
Run 1/4: H=0.08 outdir=SquareSpinIceClosed.000000.npz
Completed 24 steps in 0:00:00.707233
Run 2/4: H=0.084 outdir=SquareSpinIceClosed.000001.npz
Completed 38 steps in 0:00:00.838193
Run 3/4: H=0.088 outdir=SquareSpinIceClosed.000002.npz
Completed 44 steps in 0:00:00.766781
Run 4/4: H=0.092 outdir=SquareSpinIceClosed.000003.npz
Completed 80 steps in 0:00:00.923469
The -s/--sweep
argument in the above command specifies a sweep of the parameter H
with a list of values ranging from 80 mT to 92 mT.
Note how the invocation of flatspin-run-sweep
is identical to flatspin-run
, with the addition of -s/--sweep
.
Multiple parameters may be swept by providing multiple -s/--sweep
arguments, in which case all combinations of parameter values will be swept.
For example, the command:
flatspin-run-sweep ... -s 'phi=[0, 30, 45]' -s 'H=[80e-3, 84e-3, 88e-3, 92e-3]'
would sweep the two parameters phi
and H
, starting with phi=0, H=80e-3
, then phi=0, H=84e-3
, and so on until finally phi=45, H=92e-3
is reached.
The above sweep would result in a total of 12 flatspin runs.
In addition, each run may be repeated N
times with -n/--repeat N
.
This is useful when simulating stochastic systems, e.g., with disorder or thermal fields enabled.
Distributed running#
As the number of parameters grow, it may be beneficial to distribute the simulations onto a compute cluster to run them in parallel.
Distributed running is supported both by flatspin-run
and flatspin-run-sweep
with the -r dist
argument.
flatspin uses SLURM to submit cluster jobs.
Currently you need to edit the file flatspin.slurm.sh
to configure flatspin for your particular cluster.
Other job schedulers should be possible with minimal code changes.
Analysis tools#
A set of analysis tools are included in flatspin, which all operate on datasets such as those produced by flatspin-run
and flatspin-run-sweep
.
flatspin-inspect
#
flatspin-inspect
is a handy tool to quickly get an overview of the contents of a dataset.
For example, let us have a look at the sweep we created above:
flatspin-inspect -b /tmp/flatspin/mysweep -l
Dataset: mysweep
params:
alpha=0.001
astroid_resolution=1801
attempt_freq=1000000000.0
disorder=0
edge=symmetric
encoder=flatspin.encoder.Triangle
flip_mode=max
H=1
H0=0
h_ext=(0, 0)
hc=0.2
init=polarized
input=1
input_key=nan
lattice_spacing=1
m_therm=7.567999999999999e-17
neighbor_distance=1
opencl_device=0
opencl_platform=0
periods=1
phase=-90
phi=30
random_prob=0.5
random_seed=0
size=(4, 4)
spin_axis=nan
spp=100
sw_b=0.41
sw_beta=1.5
sw_c=1
sw_gamma=3.9
switching=sw
temperature=0
therm_timescale=1
timesteps=100
use_cuda=False
use_opencl=False
info:
command: /builds/flatspin/flatspin/.tox/docs/bin/flatspin-run-sweep -o /tmp/flatspin/mysweep -m SquareSpinIceClosed -e Triangle -p phase=-90 -p phi=30 -p periods=1 -s 'H=[80e-3, 84e-3, 88e-3, 92e-3]'
data_format: npz
model: flatspin.model.SquareSpinIceClosed
model_name: SquareSpinIceClosed
version: 2.5.dev2+g10f633c
index:
H outdir
0 0.080 SquareSpinIceClosed.000000.npz
1 0.084 SquareSpinIceClosed.000001.npz
2 0.088 SquareSpinIceClosed.000002.npz
3 0.092 SquareSpinIceClosed.000003.npz
The output of flatspin-inspect -l
consists of three parts:
Parameter listing
params
: A list of all the parameters used in the run. Notice how this listing contains parameters that were not specified in theflatspin-run-sweep
command. These parameters record the default values at the dataset creation time.Information
info
: Miscellaneous information about the run, including the fullflatspin-run-sweep
command.The
index
of the runs in the dataset: the index contains one column for each swept parameter.
Tip
If the -b/--datapath
argument is omitted, the flatspin analysis tools will look for a dataset in the current working directory.
Tables included in a run#
Let us have a look at what tables are available within each run:
flatspin-inspect -b /tmp/flatspin/mysweep
[0] H=0.08 outdir=SquareSpinIceClosed.000000.npz:
tables (11): energy[t], geometry, h_ext[t], hc, init, input[t], mag[t], params, spin[t], stats, steps[t]
[1] H=0.084 outdir=SquareSpinIceClosed.000001.npz:
tables (11): energy[t], geometry, h_ext[t], hc, init, input[t], mag[t], params, spin[t], stats, steps[t]
[2] H=0.088 outdir=SquareSpinIceClosed.000002.npz:
tables (11): energy[t], geometry, h_ext[t], hc, init, input[t], mag[t], params, spin[t], stats, steps[t]
[3] H=0.092 outdir=SquareSpinIceClosed.000003.npz:
tables (11): energy[t], geometry, h_ext[t], hc, init, input[t], mag[t], params, spin[t], stats, steps[t]
From the output above, we can see that each run in the dataset contains quite a few tables.
Tables marked with a [t]
contain time-dependent data.
Below is a short description of the tables, with references to the releated model attributes or methods.
Table |
Description |
---|---|
|
Energy over time |
|
Position and angle of each spin |
|
External field over time |
|
Thermal field over time (if |
|
Coercive fields of each spin |
|
Initial state of each spin |
|
Input over time |
|
Magnetization vectors over time |
|
Parameter listing |
|
Time-varying parameters over time (if any) |
|
Spin state over time |
|
Run statistics |
|
Cumulative number of steps over time |
Subset and filter#
Just like the flatspin dataset API, we can select a subset of the dataset with -i/--subset
or -s/--filter
:
flatspin-inspect -b /tmp/flatspin/mysweep -i 1:2
[1] H=0.084 outdir=SquareSpinIceClosed.000001.npz:
tables (11): energy[t], geometry, h_ext[t], hc, init, input[t], mag[t], params, spin[t], stats, steps[t]
[2] H=0.088 outdir=SquareSpinIceClosed.000002.npz:
tables (11): energy[t], geometry, h_ext[t], hc, init, input[t], mag[t], params, spin[t], stats, steps[t]
flatspin-inspect -b /tmp/flatspin/mysweep -s H=0.084
[1] H=0.084 outdir=SquareSpinIceClosed.000001.npz:
tables (11): energy[t], geometry, h_ext[t], hc, init, input[t], mag[t], params, spin[t], stats, steps[t]
In fact, all the flatspin analysis tools support a common set of command-line options, such as -i/--subset
, -s/--filter
and -l/--list
.
flatspin-plot
#
For quickly plotting data from a dataset, flatspin-plot
is your friend.
Let us plot the external field over time from the myrun
dataset created earlier:
flatspin-plot -b /tmp/flatspin/myrun -x t -y h_ext
Similarly, we can plot data from multiple runs:
flatspin-plot -b /tmp/flatspin/mysweep -k H -x t -y h_ext
Plot everything from a given table with -g/--table
:
flatspin-plot -b /tmp/flatspin/myrun -x t -g energy
Rudimentary functions are also supported, e.g., to sum of all the spins over time:
flatspin-plot -b /tmp/flatspin/mysweep -k H -x t -y 's=sum(spin*)'
… or the same data plotted as a heatmap:
flatspin-plot -b /tmp/flatspin/mysweep -k H -x t -z 's=sum(spin*)'
Arbitrary columns may be used on the x-axis:
flatspin-plot -b /tmp/flatspin/myrun -x 'mx=sum(mag*x)' -y 'my=sum(mag*y)'
See flatspin-plot --help
for a full list of options.
flatspin-vectors
#
Use flatspin-vectors
to animate spin vectors over time.
The time steps to include can be limited using -t start:stop:step
.
In the command below we include all time steps, and draw vectors as arrows.
flatspin-vectors -b /tmp/flatspin/myrun -t ::1 --style=arrow
It is often useful to compare results from multiple runs.
When the dataset contains multiple runs, flatspin-vectors
animates them side by side in a montage:
flatspin-vectors -b /tmp/flatspin/mysweep -t ::1 --style=arrow
It is also possible to create a montage over time, where each image corresponds to the same run at different points in time.
Montage over time is enabled with -a/--animate-dataset
.
When the images become small, it is a good idea to use the default --style=image
, which results in a grid based visualization instead.
flatspin-vectors -b /tmp/flatspin/myrun -t ::1 -a
By default, flatspin-vectors
animates the spin vectors, but other quantities can be specified with -q/--quantity
:
flatspin-vectors -b /tmp/flatspin/myrun -t ::1 --style=arrow -q h_ext
Apply a grid#
A grid may be applied to the vectors to produce an aggregate view with -g/--grid
.
Below we apply a 2x2
grid and sum the vectors in each grid cell:
flatspin-vectors -b /tmp/flatspin/myrun -t ::1 -a -g 2
The different color shades in the images above are caused by each grid cell having a different number of spins.
For the square closed geometry, we can obtain vertex magnetization by first cropping away the spins at the edges (-c/--crop 1
), and then apply a sliding 3x3 window with a step size of 2 (-w/--window 3 2
):
flatspin-vectors -b /tmp/flatspin/myrun -t ::1 -a -c 1 -w 3 2
For other geometries, the above windowing trick may not be applicable to find vertices.
The flatspin-vertices
tool is similar to flatspin-vectors
, but employs vertex detection to correctly visualize vertex magnetization for all the included geometries.
Other tools#
In this guide, we have introduced some of the most commonly used command-line tools in flatspin.
Several other tools are included, available with the flatspin-
prefix.
For a full list of command-line tools, see Command-line reference.