McStas - A neutron ray-trace simulation package
McStas is a general tool for simulating neutron scattering instruments
and experiments. It is actively supported by DTU Physics
, NBI KU
scattering from a hollow-cylinder vanadium
|The plot shows the intensity of scattered neutrons (red is
highest intensity). The sample is at the center of the sphere with the
neutron beam coming from the left. Clearly seen is the shadowing effect
of the sample causing a lower intensity opposite the beam. Also seen is
the effect of the non-symmetric geometry of the sample, causing lower intensity
directly above and to the side of the sample.|
May 26th, 2020: Experimental McStas 2.6.1 and McXtrace 1.5 dockers
The combined McStas and McXtrace team have started experimenting
with using Docker's for deployment. The advantage is simplified
installation and a uniform look and feel / functionality across
If you feel like giving our experimental docker solutions a spin, have a look at
May 4th, 2020: McStas 2.6.1 released
A new minor-release of McStas, v. 2.6.1 has been built and is ready for download!
Download and installation instructions are available via our GitHub download pages.
The release adresses a few bugs found in the 2.6 release, see the related issue list at GitHub,
but is in terms of features and functionality almost identical to 2.6.
April 28th, 2020: McStas 2.6 on Ubuntu 20.04
I have tried out the McStas 2.6 release on the fresh Ubuntu 20.04
release, and my findings are these:
- Generally, the release works as expected - all of the python
tools seem to function well.
- For the legacy perl tools we have the issue that the OS-provided
PDL no longer comes with a PGPLOT plotting-bridge, which affects
mcplot.pl and mcgui.pl:
Can't locate PDL/Graphics/PGPLOT.pm in @INC (you may need to install the PDL::Graphics::PGPLOT module)
(@INC contains: /usr/share/mcstas/2.6/tools/Perl/perl/modules /usr/share/mcstas/2.6/tools/Perl/perl /etc/perl
/usr/local/lib/x86_64-linux-gnu/perl/5.30.0 /usr/local/share/perl/5.30.0 /usr/lib/x86_64-linux-gnu/perl5/5.30
/usr/share/perl5 /usr/lib/x86_64-linux-gnu/perl/5.30 /usr/share/perl/5.30 /usr/local/lib/site_perl
/usr/lib/x86_64-linux-gnu/perl-base) at /usr/share/mcstas/2.6/tools/Perl/perl/mcplotlib.pl line 23, line 207.
BEGIN failed--compilation aborted at /usr/share/mcstas/2.6/tools/Perl/perl/mcplotlib.pl line 23, line 207.
Compilation failed in require at /usr/bin/mcgui.pl line 2181, line 207.
- Of course the recommendation is to simply move to the Python
tools, but if you insist to stay with perl, please do a local
CPAN-based PDL installation like this:
sudo cpan install PDL
- Since a few releases, the default PGPLOT implementation on Ubuntu changed to Giza.
Giza seems to now be getting better, see the April
30th 2018 hint if you want the legacy PGPLOT instead.
A new minor release 2.6.1 is on the way, implementing a few bugfixes,
see our GitHub issue tracker
for more information.
February 27th, 2020: McStas 3.0beta bugfixes etc
- As we move along with the development on the mcstas-3.0 branch, you may find patched
versions of components in the Updates folder found next to the
distribution binaries at http://download.mcstas.org/mcstas-3.0beta/.
- A first bug with fix: Unfortunately, a buggy last-minute
change to the PowderN component before mcstas-3.0beta was built introduced an
error which makes it produce 0 scattered intensity. Please find
an improved version in the
above-mentioned Updates folder. Further bugfixes to this
component are expected since the component
produces scattering but has certain edge-case issues on GPU, especially at high ncount rates.
- At any time, know bugs will be listed as issues on GitHub marked
with the label of "mcstas-3.0beta"
- Please do submit issues to GitHub as you find them: This will
help in the process toward a stable, official 3.0 release!
February 25th, 2020: McStas 3.0beta technology preview available!
A technology preview for the forthcoming McStas 3.x series is now
available for testing!
Main highlights of the release are:
- New code-generation scheme based on functions instead of #defines
- Much improved compilation-times, the code is better suited for modern compilers
- In most cases a speed-up of order 20% on CPU
- Limited, experimental support for OpenACC acceleration on NVIDIA GPU's
- Speedups measured using top-notch NVIDIA V100 datacenter cards are in the range of 10-600 with respect to a single-core CPU
- In essence, you will need a Linux machine with an NVIDIA card and
the PGI compiler to make use of the GPU-support
For more details and instructions, please refer to this
document on our Wiki
- Thanks to all members of the joint McStas-McXtrace team, you guys ROCK!
- Thanks to Guido Juckeland (HZDR,DE) and Sebastian Alfthan (CSC,FI) who were behind the GPU Hackathons we participated in
- Thanks to our NVIDIA mentors Vishal Metha, Christian Hundt and Alexey Romanenko
January 24th, 2020: McStas 2.6 release!
A new release of McStas, v. 2.6 has been built and is ready for download!
Download and installation instructions are available via our GitHub download pages.
Selected highligts from the release are listed below. The full list
of changes is also available at http://mcstas.org/CHANGES_McStas.
Changes in McStas v.2.6, January 24th, 2020
- McStas 2.6 is the eight release in the 2.x series and fixes various issues with McStas 2.5, plus
- Thanks to all contributors of components, instruments etc.! This is what Open Source
and McStas is all about!
- Fixes of issues from last release:
- Plus lots of work in general, see the relevant GitHub issues
- Contribution from Tobias Weber ILL: Python-version of mcresplot.
- Updated version 1.0.0 NCrystal library from T. Kittelmann (ESS) and X.X. Cai (CSNS), distributed with McStas on Unix
platforms only. See the CHANGES document for full detail.
- MCPL library from the same authors now included at v. 1.3.0. See the CHANGES document for full detail.
- Updated version of the NXS lib from Mirko Boin HZB.
- Updated Union library from Mads Bertelsen, ESS DMSC including
- New geometries, mesh (for stl file input in Union setups) and cone (e.g. relevant for describing anvils
in pressure cells.
- New AF_HB_1D_process for modelling 1D antiferromagnetic
Heisenberg chains and PhononSimple_process for modelling
single-branchg acoustic phonons ala Phonon_simple
- New SINE2020-developed Union physics processes from Victor Laliena, Uni Zaragoza: Texture_process.comp
and IncoherentPhonon_process.comp. See DOI:10.3233/JNR-190117.
- Shieldinglogger-components from Rodion Kolevatov, IFE for
estimating gamma-production in guides:
- Contributions Dose_calculator and Shielding_calculator
- Patched versions of optics-components: Elliptic_guide_gravity_shieldinglogger, Guide_channeled_shieldinglogger,
Guide_curved_shieldinglogger, Guide_gravity_shieldinglogger, Guide_shieldinglogger
- Components patched / derived from the "scatterlogger"
framework to model Ni and Ti layers seperately:
- See DOI:10.3233/JNR-190123,
- Please note that the included Shielding- and Dose- calculators will only give sensible for guides with
borosilicate glass substrate. If the substrate is, e.g. copper, the dose rates from neutrons transmitted
through the coating and captured in the substrate will overshoot the coating contribution significantly,
so that shielding has to be enforced by few tens of centimeters of concrete.
- Guide_anyshape_r additions from Peter Link MLZ. Allows
describing geometry in OFF format with reflectivity "per" face. Test
instrument is Test_guides which has been updated to include this
- Vertical_Bender from Andrew Jackson ESS and Richard Heenan STFC. Allows modelling a multi-channel bender
that curves vertically down.
- SANS_spheres2 by Peter Willendrup, derived from Henrich Frilinghaus' SANS_benchmark2. More realistic cross-section
calculations than from e.g. Sans_spheres. templateSANS2.instr is the related test instrument.
- Updated version of Sample_nxs from Mirko Boin HZB.
- Single_magnetic_crystal.comp is an experimental magnetic csingle crystal model. Its operational model is based
on that of Single_crystal.comp but supports SF and NSF magnetic scattering. The present model only supports
the SF-NSF paradigm along a given reference vector.
- PSD_monitor_4PI_spin.comp is a version of PSD_monitor_4PI but with separate SF- and NSF-channels
- Union_test_texture.instr demonstrates use of Texture_process.comp by Victor Laliena. To be used with datafile
"coef_Four_L2.txt" found in the installation data-folder. This datafile contains texture information on Zr alloys
derived from DOI:10.1016/j.jnucmat.2018.08.003.
- Union_IncoherentPhonon_test.instr demonstrates use of IncoherentPhonon_process.comp by Victor Laliena. To be used
with datafile "dos_meV.txt" found in the installation data-folder.
- Union_test_mesh.instr demonstrates use of mesh geometry in Union
- ESS_BIFROST_shielding.instr and PSI_Focus_shielding.instr, demonstration of Shielding_logger concept from
- TasResoTest, triple-axis resolution test instrument from Tobias Weber ILL. Can be used with his new tool
- Tools_ONION, instrument to investigate q-resolution via
Mantid, by Thomas Huegle, ORNL. See also DOI:10.1016/j.nima.2019.162711 and the related python
code available at our new "snippet"
repository that should eventually replace the old "share" part of this webpage.
- templateSANS_MCPL, behaves like the normal templateSANS but dumps all events in an MCPL file.
- MCPL-oriented tool-instruments by Peter Willendrup. See the CHANGES document for full detail.
- SINE2020-developed McStas_Isotropic_Sqw, McStas_PowderN, McStas_Single_crystal by Erik Knudsen. They have
MCPL input/output and are intended for easy use of McStas samples within SIMRES.
- Test_guides has been modified to include Guide_anyshape_r from Peter Link MLZ.
- templateSANS2 serves as test instrument for SANS_spheres2.
- Test_single_magnetic_crystal.instr is a skeleton Laue camera
which exemplfies use of Single_magnetic_crystal.comp
- Klaus Lieutenant from FZJ/Vitess has collected reflectitivy-data from SwissNeutronics, Mirrotron and S-DH, analysed
these and fitted the "classical" McStas mirror-reflectivity profile to these. The resulting data have been placed
in the data directory under the filenames of
- The files are not to be used directly with reflecting components, but can instead be used as lookup-tables for
relevant parameters in each case. I.e. for a mirror of nominal m-value m_nom, use m_real, R_0, W and alpha from the
- Most other new datafiles are directly related to component- or instrument-additions and have been mentioned above.
We hope you will enjoy this new release!!!
Previous news items: 2019, 2018, 2017, 2016,
2015, 2014, 2013,
2012, 2011, 2010, 2009,
2008, 2007, 2006,
2005, 2004, 2003, 2002, 2001, 2000, 1999,
Last Modified: Tuesday, 26-May-2020 15:03:02 CEST