Magnetic fields below, on and above the solar surface
Magnetic fields below, on and above the solar surface
复制标题
太阳表面下方、上方和上方的磁场
DOI：
--
复制
发表时间：
2000
期刊：
影响因子：
--
通讯作者：
A. Title
中科院分区：
文献类型：
--
作者：
A. Title
太阳是唯一可以被详细研究的恒星。过去十年见证了太阳能数据范围、数量和质量的革命。协调的定量观测将深层内部的过程与外层大气的过程联系起来。数值模拟和理论模拟结果与观测结果非常吻合。太阳现在教给我们的最重要的一课是，定量测量与数值模拟和理论的并行发展，可以对密度、压力、温度和等离子体β在很大范围内发生的复杂非线性现象产生物理理解。了解太阳的物理特性是解开天体物理学难题的关键。
The Sun is the only star that can be studied in detail. The last decade saw a revolution in the scope, amount, and the quality of solar data. Coordinated quantitative observations link the processes in the deep interior to those in the outer atmosphere. Numerical simulations and theoretical modelling have produced detailed agreement with observations. The most important lesson the Sun is now teaching us is that the parallel development of quantitative measurements with numerical simulation and theory can produce a physical understanding of the complex nonlinear phenomena that occur over a wide range in densities, pressures, temperatures and plasma betas. Understanding the physics of the Sun is a major key to unravelling puzzles throughout astrophysics.