Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Development of a High-order Flux Reconstruction Framework for Solar and Astrophysical Magnetohydrodynamics: Methods and Benchmarks

  • Authors: Rayan Dhib, Firas Ben Ameur, Matteo Parsani, Andrea Lani, Stefaan Poedts

Rayan Dhib et al 2026 The Astrophysical Journal Supplement Series 283 .

  • Provider: AAS Journals

Caption: Figure 3.

Evolution of the Orszag–Tang vortex problem. The pressure field is shown at times (from top to bottom) t = 0.25 and t = 0.5, and on the right are the corresponding distributions of α (the blending coefficient).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse