A 3D radiative transfer framework: VII. Arbitrary velocity fields in the Eulerian frame
A. M. Seelmann, P.H. Hauschildt, E. Baron

TL;DR
This paper introduces a 3D radiative transfer method for arbitrary velocity fields in the Eulerian frame, implemented in the PHOENIX/3D code, enabling efficient large-scale astrophysical simulations.
Contribution
It presents a novel Eulerian approach for 3D radiative transfer with arbitrary velocities, compatible with existing computational frameworks.
Findings
Method is validated against 1D co-moving frame code.
Requires minimal additional memory.
Suitable for large-scale applications with thousands of wavelength points.
Abstract
A solution of the radiative-transfer problem in 3D with arbitrary velocity fields in the Eulerian frame is presented. The method is implemented in our 3D radiative transfer framework and used in the PHOENIX/3D code. It is tested by comparison to our well- tested 1D co-moving frame radiative transfer code, where the treatment of a monotonic velocity field is implemented in the Lagrangian frame. The Eulerian formulation does not need much additional memory and is useable on state-of-the-art computers, even large-scale applications with 1000's of wavelength points are feasible.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsComputer Graphics and Visualization Techniques · Radiative Heat Transfer Studies · Advanced Optical Sensing Technologies
