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류동수

Ryu, Dongsu
Astrophysics Lab.
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dc.citation.conferencePlace SA -
dc.citation.conferencePlace Cape Town -
dc.citation.title 32nd General Assembly of the International Astronomical Union -
dc.contributor.author Ryu, Dongsu -
dc.contributor.author Seo, J. -
dc.date.accessioned 2024-12-13T15:05:07Z -
dc.date.available 2024-12-13T15:05:07Z -
dc.date.created 2024-12-13 -
dc.date.issued 2024-08-13 -
dc.description.abstract A New High-Order Magnetohydrodynamic Code with a High-Order Constrained Transport Scheme

Dongsu Ryu^1, Jeongbhin Seo^2

1Depart. of Physics, College of Natural Sciences, UNIST, Rep. of Korea
2Los Alamos National Laboratory, Los Alamos, USA

We introduce a magnetohydrodynamic (MHD) code tailored for astrophysical applications. The code leverages a fifth-order finite-difference weighted essentially non-oscillatory (WENO) scheme for spatial discretization, coupled with a fourth-order strong stability-preserving Runge-Kutta (SSPRK) scheme for temporal integration. In particular, to match the high-order accuracy of the WENO scheme, we implement a novel constrained transport (CT) algorithm of high-order accuracy to enforce div(B) = 0. Here, we outline the MHD code and present its performance. We validate that with the new CT scheme, the code achieves the order of accuracy of the WENO scheme in wave decay tests, including a circularly polarized Alfven wave propagation test. Further, the code's high robustness and fidelity are demonstrated through tests involving complex flows.
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dc.identifier.bibliographicCitation 32nd General Assembly of the International Astronomical Union -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/84821 -
dc.language 영어 -
dc.publisher International Astronomical Union -
dc.title A New High-Order Magnetohydrodynamic Code with a High-Order Constrained Transport Scheme -
dc.type Conference Paper -
dc.date.conferenceDate 2023-08-06 -

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