Skip to main content

SasView application

Project description

Logo

Latest Release Last Commit Website Status License

General

SasView is a Small Angle Scattering (SAS) analysis package for the analysis of 1D and 2D scattering data directly in inverse space. The focus was originally on neutron data (SANS) but has been used for X-rays as well and includes a tool for determining a slit resolution for the SAXSess instrument. SasView also includes PrView to invert SAS data to P(r), a resolution calculator, and a scattering length density calculator among others tools. A simple plugin mechanism is available for users to add custom models.

Citing and Acknowledging SasView

If you found this software useful to your work please cite and/or acknowledge its use in your publications. The latest instructions for citing and acknowledging are available on our website.

Citing SasView

Install instructions

Users

Users can install SasView either from the installers listed on the SasView website, or directly from the packages distributed by pip.

Install using pip inside a virtual environment in the current directory:

python -m venv .venv # create the environment
. .venv/bin/activate # activate the environment on linux and MacOS
# .venv\Scripts\activate & REM Windows: activate environment

python -m pip install sasview

python -m sas   # launch the gui

Install using uv for your user:

uv tool install sasview

uvx sasview   # launch the gui

Note: To launch SasView, it needs to be installed. Running SasView from a source directory is not supported.

Developers

The installation instructions for developers can be found here. Installing the development-version of SasView with conda is currently not supported. NOTE: In case you want to contribute, please also checkout the DevelopersNotes.

Getting Started

Scripting

This section is a small scripting example in SasView to check your installation. We will fit a simple sphere model. For this first lets synthesize input data.

import numpy as np
from sasmodels.bumps_model import Model
from sasmodels.core import load_model
from sasmodels.direct_model import call_kernel

# define q vector
q = np.logspace(-3, -0.1, 200)

# define the model
exp_model = load_model("sphere")
exp_pars = {
    "radius": 50,
    "sld": 1,
    "sld_solvent": 6,
    "scale": 1,
    "background": 0.001,
}

# calculate intensities
Iq = call_kernel(exp_model.make_kernel([q]), exp_pars)

# calculate errors and normalize data
max_counts = 1e7  # approximate number of counts at first q values
norm = Iq[0] / max_counts
counts = np.random.poisson((Iq / norm).astype(int))
errors = np.sqrt(counts) * norm
data = counts * norm
dataset = np.array([q, data, errors]).T

# saving the data
header = (
    "Neutron-like data generated for model "
    + exp_model.info.name
    + " with parameters:\n"
)
for key in exp_pars.keys():
    header += key + " = " + str(exp_pars[key]) + "\n"
header += "Q\t counts\t error"

np.savetxt("scattering.txt", dataset, fmt="%12.6e", delimiter="\t", header=header)

...and now let's do the fitting. We will optimize the scale, radius and background starting from an inital values close to the ground truth.

import matplotlib.pyplot as plt
from sasmodels.bumps_model import Model, Experiment
from sasmodels.core import load_model
from sasmodels.data import load_data
from bumps.fitters import fit
from bumps.names import FitProblem

# defining the  model to fit
fit_pars = {
    "radius": 80,
    "sld": 1,
    "sld_solvent": 6,
    "scale": 0.900,
    "background": 0.05,
}
fit_kernel = load_model("sphere")
fit_model = Model(fit_kernel, **fit_pars)

## setting fitting ranges
fit_model.radius.range(10, 1000)
fit_model.scale.range(1e-3, 10)
fit_model.background.range(1e-9, 0.1)

# load the data we synthesized above
exp_data = load_data("scattering.txt")

# Setup the experiments, sharing the same model across all datasets.
M = Experiment(data=exp_data, model=fit_model, name="MyAwsomeFit")

problem = FitProblem(M)

plt.figure()
problem.plot(view=True)

# fit the results
result = fit(problem, method="dream")

print(f"Final chisq {problem.chisq()}\n")
problem.plot()
for k, v, dv in zip(problem.labels(), result.x, result.dx):
    print(f"{k} : {v:.4f} +- {dv:.4f}")
plt.show()

This simple fit should results in a $\chi^2$ close to one.

image

Resources

In case you are just getting started or you want to contribute please checkout some selected resources.

Project details


Download files

Download the file for your platform. If you're not sure which to choose, learn more about installing packages.

Source Distribution

sasview-6.2.0b1.tar.gz (71.4 MB view details)

Uploaded Source

Built Distribution

If you're not sure about the file name format, learn more about wheel file names.

sasview-6.2.0b1-py3-none-any.whl (74.6 MB view details)

Uploaded Python 3

File details

Details for the file sasview-6.2.0b1.tar.gz.

File metadata

  • Download URL: sasview-6.2.0b1.tar.gz
  • Upload date:
  • Size: 71.4 MB
  • Tags: Source
  • Uploaded using Trusted Publishing? No
  • Uploaded via: twine/6.2.0 CPython/3.13.11

File hashes

Hashes for sasview-6.2.0b1.tar.gz
Algorithm Hash digest
SHA256 512ba6b4c4f939f1cbb1188c410af7de9aa16f50f3a1fb711a79fdfa69c45a46
MD5 9fd1f3326d5bdd642b23d72396a70831
BLAKE2b-256 fe867910c95e3210cbadd8229d4df61d0fbbbecc6918aba1538574621fbd9a6f

See more details on using hashes here.

File details

Details for the file sasview-6.2.0b1-py3-none-any.whl.

File metadata

  • Download URL: sasview-6.2.0b1-py3-none-any.whl
  • Upload date:
  • Size: 74.6 MB
  • Tags: Python 3
  • Uploaded using Trusted Publishing? No
  • Uploaded via: twine/6.2.0 CPython/3.13.11

File hashes

Hashes for sasview-6.2.0b1-py3-none-any.whl
Algorithm Hash digest
SHA256 eb3a9ee70296656c91c6bbf4259539883a46459aa33dbd03d7d850284a582894
MD5 fb5b3c998924df1e6a967c2ccbf0d0f9
BLAKE2b-256 e4f0ea3ae15a009b787c338a43ed9c64bba601a3b869c71d4d5c48db84f24488

See more details on using hashes here.

Supported by

AWS Cloud computing and Security Sponsor Datadog Monitoring Depot Continuous Integration Fastly CDN Google Download Analytics Pingdom Monitoring Sentry Error logging StatusPage Status page