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Using the fully vectorial effective index method, we calculate the effective refractive index for different air hole size.
Based on the Cagniard deHoop method we calculate the magnetic field and plasma flow time series observed by a satellite.
By using a finite volume-based computational method, we calculate the flow field as well as species concentration field before and after improvement of the thermal design, respectively.
By a convenient numerical fitting method, we calculate a set of kinetic parameters which are afterwards put into the theoretical equations for dc and the impedance.
Using the ACE-ISDF method, we calculate the defect energy levels for a 1000-atom systemn system with a vacancy using the HSE06 hybrid exchange-correlation functional, which yields quantitative agreement with a recent large scale GW calculation for this large system.
Using the same method, we calculate the upper bound on single-hop delay/jitter/effective bandwidth.
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By use of the TransCount method we calculated absolute transcript concentrations from spotted oligoarray intensities, enabling direct comparisons with tag counts obtained with MPSS and SAGE.
To test the validity of this method, we calculated the light transmission through sub-wavelength structures by the finite-difference time-domain (FDTD) method and point source method.
As an illustration of this method, we calculated γ for quiet and disturbed conditions using the Nagoya multidirectional muon detector.
For different communities from each cluster method, we calculated the normalized mutual information among LCBN, SBN and HGNC gene family to compare the three methods.
Using the PCA method, we calculated the eigenvalues of all six factors included in the three dimensions used in this study.
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Since I tried Ludwig back in 2017, I have been constantly using it in both editing and translation. Ever since, I suggest it to my translators at ProSciEditing.

Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com