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cfortran.h is an easy-to-use powerful bridge between C and FORTRAN. It provides a transparent, machine independent interface between C and FORTRAN routines and global data.
This project is a fork of the CERN Program Library is a large collection of general purpose libraries/ This program is oriented to needs of a physics laboratory that is general mathematics, data analysis, detectors simulation, data-handling etc...
The project have moved and is alive at http://opencernlib.tuxfamily.org/
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Cca-forum unifies the Common Component Architecture tools and tutorial. It includes the CCA specifications, the Ccaffeine framework for HPC, and related tools. These support multilanguage scientific and parallel computing.
Software bundle to provide development of the following softwares for simulating waves, currents, transport and mixing as well as sediment transport in coastal environments and hydraulic systems: LWBouss1D/2D BoussSand1D/2D OCTEAD FunSedi1D/2D
A complete OpenCascade based MESH framework.Note this is not the original SALOME SMESH project but an effort to create a standalone mesh framework based on the existing one from SALOME project, plus adding WIN32 compatibility.
ByoDyn (http://cbbl.imim.es/ByoDyn) is a software tool for the study of biochemical networks within the framework of systems biology. SBML compatible, ByoDyn is a group effort of the Computational Biochemistry and Biophysics Lab.
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fropho calculates phonon properties in crystal, which is based on Parlinski-Li-Kawazoe method. Information of forces acting on atoms when an atom is displaced is required as input information. fropho is going to be replaced by phonopy.sourceforge.net.
The Fortran program MOLLY generates atomic positions in a molecule from those of a small number of prototype atoms and the molecule's point symmetry. It is intended as a time-saving aid in preparing input data for computational physics software.
CIVx is a free advanced PIV (Particle Imaging Velocimetry) code, developped in Fortran and C++. Input : pair of png images. Output : velocity field in NetCDF format. It is used by the UVMAT Matlab code develloped at LEGI.
Molecular Graphics and Dynamics. Molecular model builder. Part of the Ascalaph Designer http://sourceforge.net/projects/asc-designer/ project. Windows & Linux.
NOSE is a package for simulation of linear and non-linear optical and infrared spectra, including absorption, fluorescence, circular dichroism, pump-probe, photon echo and other.
A reactor solver which uses stochastic particle methods to model particle population balances. This code is developed by the CoMo group in the chemical engineering department at the university of Cambridge (como.cheng.cam.ac.uk).
MACROMS is a software to model the coastal ocean circulation and fish larvae transport for the USA Mid-Atlantic region, which covers estuaries and continental shelves of NYC, NJ, DE, MD, PA, VA and NC. Rutgers ROMS model is applied for this study.
Sandia National Laboratories’ (SNL) environmental assessment modeling tool helps optimize the design of MHK-turbine array layouts within ocean, tidal, and river systems to balance energy generation efficiency with environmental considerations. The new tool, SNL-EFDC, is an augmented version of US EPA’s Environmental Fluid Dynamics Code (EFDC) and includes; (1) a new module that simulates energy conversion (momentum withdrawal) by MHK turbine-like devices including commensurate changes in the...
A Python environment for large and sparse linear and nonlinear optimization using intuitive interfaces to linear algebra tools and subproblem solvers written in low-level languages. It provides building blocks to experiment with new ideas and algorithms.
Main Phase Modeling, MPM, is a implementation of a 2D staggered grid solution of the elastic waveequation, using a moving zone. This enables both efficient modeling of seismic wide angle data, and modeling of selected propagating phases.
A Software project to assimilate solar magnetograms into suitable physics based models of the solar wind expansion. To predict the solar wind conditions at the Earth and at outer planets. Or any space-craft location in the solar system.
FGH is program that solves vibrational Schroedinger equation using the Fourier grid hamiltonian method. The program requires potential energy surface and G-matrix defined at the uniform grid of points.