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### Environment details
If you are already running SDV, please indicate the following details about the environment in
which you are running it:
* SDV version:
* Python version:
* Operating S…
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Hi everyone,
Since it was first proposed in 2008 by P. Schmid ([Dynamic mode decomposition of numerical and experimental data, _J. Fluid Mech._, 2008](https://hal-polytechnique.archives-ouvertes.fr…
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Dear Yury A. Mishin,
I am sorry to bother you. I am a PhD student in Peking University of China. At present, I am using I2VIS code to conduct a research about the fate of subducted continental curst…
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For easier development and optimization we should have a PMSM motor and power stage simulation that we can run our control algorithms on. These algorithms should be the same ones we use on the real co…
esden updated
13 years ago
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can you clarify what you mean by the 'biological' begin/end position to use in your model?
there are a couple of ways that could be interpreted from the current documentation:
1. the begin/end of wh…
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The Jupyter Notebook is an open-source web application that allows you
to create and share documents that contain live code, equations,
visualizations and narrative text. Uses include: data cleaning…
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We recommend the following two patterns for modeling a range of magnitudes. Note that the class `gist:Magnitude` is not used, because a magnitude represents an exact value, whereas a range is a specif…
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Hi,
I am reporting a convergence issue with the omega transport equation of the k-ω SST turbulence model in Nalu-Wind. I’ve attached non-linear residual plots for NASA’s canonical case: the subsoni…
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Implementation of cluster abundance cosmological prediction with CCL as a backend for:
1. cluster count in mass (respectively mass proxy) and redshift bins (for binned likelihood)
2. cluster count f…
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Hi,
I would like to better understand how the factor scores are estimated in the lavPredict function depending on the type and method arguments.
I didn't find references in rdrr.io or in CRAN. C…