由磁流体耦合引起的日球染层中的气流生成
天体物理学
2009-11-07 v1 等离子体物理
摘要
证明了广义磁力-伯努利机制可通过将等离子体压力能转化为动能，有效生成日球染层中的高速气流。在合理的高度和实际的等离子体参数下，伴随显著的压力下降，气流速度会出现锐利的放大。
引用
@article{arxiv.astro-ph/0204311,
title = {Generation of Flows in the Solar Chromosphere Due to Magnetofluid Coupling},
author = {Swadesh M. Mahajan and Komunela I. Nikol'skaya and Nana L. Shatashvili and Zensho Yoshida},
journal= {arXiv preprint arXiv:astro-ph/0204311},
year = {2009}
}
备注
11 pages of text and 2 figures. Submitted to The Astrophysical Journal Letters