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- #Ray tracing refraction vector code upgrade
- #Ray tracing refraction vector code full
- #Ray tracing refraction vector code code
- #Ray tracing refraction vector code series
#Ray tracing refraction vector code code
We tested the updated code with benchmark models where the dust self-heating is not negligible.
#Ray tracing refraction vector code series
The new version includes five major upgrades: 1) a series of optimizations for the ray-angular density and the scattered radiation source function 2) the implementation of several data and task parallelizations using hybrid MPI+OpenMP schemes 3) the inclusion of dust self-heating 4) the ability to produce surface brightness maps for observers within the models in HEALPix format 5) the possibility to set the expected numerical accuracy already at the start of the calculation. We present an extensively updated version of the purely ray-tracing 3D dust radiation transfer code DART- Ray. Fischera, Jörg Pasetto, Stefano Rushton, Mark Thirlwall, Jordan J.
#Ray tracing refraction vector code upgrade
Ray-tracing 3D dust radiative transfer with DART- Ray: code upgrade and public release Though our specific implementation uses the NIMROD extended MHD (Sovinec et al., 2004 ) and GENRAY RF (Smirnov et al., 1994 ) codes, the approach presented can be applied more generally to any code coupling requiring the mapping of ray tracing data onto Eulerian grids. In the new representation, the RF data can then be used to construct source terms in the equations of the extended MHD model, enabling quantitative modeling of RF-induced tearing mode stabilization. In this work we demonstrate a technique, based on methods of computational geometry, for mapping the ensuing RF data (associated with discrete ray trajectories) onto the finite-element/pseudospectral grid that is used to model the extended MHD physics. The scale separation enables use of the eikonal ( ray-tracing) approximation to model the RF wave propagation. Numerical modeling of this difficult multiscale problem requires the integration of separate mathematical models for each length and time scale (Jenkins and Kruger, 2012 ) the extended MHD model captures macroscopic plasma evolution while the RF model tracks the flow and deposition of injected RF power through the evolving plasma profiles. Fortunately, the use of properly tuned and directed radiofrequency waves (λ ∼ 1 mm) can eliminate these modes. Neoclassical tearing modes are macroscopic (L ∼ 1 m) instabilities in magnetic fusion experiments if unchecked, these modes degrade plasma performance and may catastrophically destroy plasma confinement by inducing a disruption. Our code can also be used in cross-checks of the more conventional methods, which can be important in tests of theory systematics in preparation for upcoming large scale structure surveys.« lessĬoupling extended magnetohydrodynamic fluid codes with radiofrequency ray tracing codes for fusion modeling
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The ray tracing methodology presented here can be used in several cosmological analysis such as Sunyaev-Zel'dovich and integrated Sachs-Wolfe effect studies as well as modified gravity. We analyse basic statistics of lensing convergence maps and find good agreement with semi-analytical methods.
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We implemented our routines in the RAMSES N-body code and tested the implementationmore » using an example of weak lensing simulation. Moroever, since it runs on the fly in the N-body run, our code can produce maps of the desired observables without storing large (or any) amounts of data for post-processing.
#Ray tracing refraction vector code full
Unlike conventional ray tracing techniques, our code takes full advantage of the time and spatial resolution attained by the N-body simulation by computing the integrals along the line of sight on a cell-by-cell basis through the AMR simulation grid. We present a ray tracing code to compute integrated cosmological observables on the fly in AMR N-body simulations. RAY-RAMSES: a code for ray tracing on the fly in N-body simulationsīarreira, Alexandre Llinares, Claudio Bose, Sownak By including refractive propagation effects due to wind and temperature, the ray tracing code is able to explain large variations in the data observed during the flight test. NASA's current predictive capabilities using the ray tracing program (RTP) are validated using helicopter noise data taken at Eglin Air Force Base in 2007. Validation of Ray Tracing Code Refraction Effects Generic characteristics of ART include the accumulation of rays to improve statistics without memory limitations, and still providing normalized values of flux and resolution in physically meaningful units. Additional tools for slope error handling and for grating efficiency calculations are also included. The code is structured in different layers, which allow its usage as part of optimization routines as well as an easy control from a graphical user interface. The Alba ray tracing code (ART) is a suite of Matlab functions and tools for the ray tracing simulation of x- ray beamlines. Nicolas, Josep Barla, Alessandro Juanhuix, Jordi