On thermal conduction in the solar atmosphere: An analytical solution for nonlinear diffusivity without compact support

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2024-10-31 DOI:10.1051/0004-6361/202451707
S. V. Furuseth, G. Cherry, J. Martínez-Sykora
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Abstract

Context. The scientific community employs complicated multiphysics simulations to understand the physics in solar, stellar, and interstellar media. These must be tested against known solutions to ensure their validity. Several well-known tests exist, such as the Sod shock tube test. However, a test for nonlinear diffusivity is missing. This problem is highly relevant in the solar atmosphere, where various events release energy that subsequently diffuses by Spitzer thermal conductivity.Aims. The aim is to derive an analytical solution for nonlinear diffusivity in 1D, 2D, and 3D, which allows for a nonzero background value. The solution is used to design a test for numerical solvers and study Spitzer conductivity in the solar atmosphere.Methods. There exists an ideal solution assuming zero background value. We performed an analytical first-order perturbation of this solution. The first-order solution was first tested against a dedicated nonlinear diffusion solver, whereupon it was used to benchmark the single- and multifluid radiative magnetohydrodynamics code Ebysus, used to study the Sun. The theory and numerical modeling were used to investigate the role of Spitzer conductivity in the transport of energy released in a nanoflare.Results. The derived analytical solution models nonlinear diffusivity accurately within its region of validity and approximately beyond. Various numerical schemes implemented in the Ebysus code is found to model Spitzer conductivity correctly. The energy from a representative nanoflare is found to diffuse 9 Mm within the first second of its lifetime due to Spitzer conductivity alone, strongly dependent on the electron density.Conclusions. The analytical first-order solution is a step forward in ensuring the physical validity of intricate simulations of the Sun. Additionally, since the derivation and argumentation are general, they can easily be followed to treat other nonlinear diffusion problems.
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太阳大气中的热传导非线性扩散性的解析解,无需紧凑支持
背景。科学界利用复杂的多物理场模拟来了解太阳、恒星和星际介质中的物理现象。这些模拟必须根据已知的解决方案进行测试,以确保其有效性。目前已有几种著名的测试方法,如索德冲击管测试。但是,还缺少对非线性扩散性的测试。这个问题与太阳大气高度相关,在太阳大气中,各种事件都会释放能量,这些能量随后通过斯皮策热导率扩散。目的是推导出一维、二维和三维非线性扩散率的解析解,该解析解允许非零背景值。该解决方案用于设计数值求解器的测试和研究太阳大气中的斯皮策传导性。存在一个假设背景值为零的理想解。我们对这一解法进行了一阶扰动分析。我们首先用专用的非线性扩散求解器测试了一阶解法,然后用它对用于研究太阳的单流体和多流体辐射磁流体动力学代码 Ebysus 进行了基准测试。理论和数值建模被用于研究斯皮策电导率在纳米焰释放的能量传输中的作用。推导出的解析解在其有效区域内精确地模拟了非线性扩散性,并大致超出了有效区域。在 Ebysus 代码中实施的各种数值方案都能正确模拟斯皮策电导率。研究发现,仅由于斯皮策电导率,一个代表性纳米焰的能量在其生命周期的第一秒内就扩散了 9 毫米,这与电子密度密切相关。一阶解析解在确保太阳复杂模拟的物理有效性方面向前迈进了一步。此外,由于推导和论证具有普遍性,因此可以很容易地用于处理其他非线性扩散问题。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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