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Magnetohydrodynamic Process in Solar Activity
  • ISSN号：2095-0349
  • 期刊名称：Theor. Appl. Mech. Lett.
  • 时间：2014
  • 页码：052001-
  • 分类：P182.9[天文地球—天文学] P182.62[天文地球—天文学]
  • 作者机构：[1]Naftonal Astronomical Observatories, Key Lab of Solar Activity,Chinese Academy of Sciences, Beijing 100012, China
  • 相关基金：This work was supported by the National Natural Science Foundations of China （11173033, 11221063, 2011CB811401, 11221063, and 11373004） and the Knowledge Innovation Program of the CAS （ KJCX2- EW-T07）.
  • 相关项目：太阳爆发活动的关键科学问题研究
作者： Wang, J. X., & Jiang, J.|
关键词： 太阳活动, 日冕物质抛射, 等离子体物理, 太阳大气, 太阳物理学, 天体物理学, 磁流体, 能量释放, solar magnetic field, solar activity, magnetohydrodynamics, numerical simulation
中文摘要：

Magnetohydrodynamics is one of the major disciplines in solar physics.Vigorous magnetohydrodynamic process is taking place in the solar convection zone and atmosphere. It controls the generating and structuring of the solar magnetic fields, causes the accumulation of magnetic non-potential energy in the solar atmosphere and triggers the explosive magnetic energy release, manifested as violent solar flares and coronal mass ejections. Nowadays detailed observations in solar astrophysics from space and on the ground urge a great need for the studies of magnetohydrodynamics and plasma physics to achieve better understanding of the mechanism or mechanisms of solar activity. On the other hand, the spectacular solar activity always serves as a great laboratory of magnetohydrodynamics.In this article, we reviewed a few key unresolved problems in solar activity studies and discussed the relevant issues in solar magnetohydrodynamics.

英文摘要：

Magnetohydrodynamics is one of the major disciplines in solar physics. Vigorous magnetohydrodynamic process is taking place in the solar convection zone and atmosphere. It controls the generating and structuring of the solar mag- netic fields, causes the accumulation of magnetic non-potential energy in the solar atmosphere and triggers the explosive magnetic energy release, manifested as vi- olent solar flares and coronal mass ejections. Nowadays detailed observations in solar astrophysics from space and on the ground urge a great need for the studies of magnetohydrodynamics and plasma physics to achieve better understanding of the mechanism or mechanisms of solar activity. On the other hand, the spectac- ular solar activity always serves as a great laboratory of magnetohydrodynamics. In this article, we reviewed a few key unresolved problems in solar activity studies and discussed the relevant issues in solar magnetohydrodynamics.

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期刊信息
  • 《力学快报：英文版》
  • 主管单位:中国科学院
  • 主办单位:中国科学院力学研究所、中国力学学会
  • 主编：李家春
  • 地址：北京市海淀区北四环西路15号
  • 邮编：100190
  • 邮箱：taml@cstam.org.cn
  • 电话：010-82543904
  • 国际标准刊号：ISSN：2095-0349
  • 国内统一刊号：ISSN：11-5991/O3
  • 邮发代号:82-766
  • 获奖情况:
  • 国内外数据库收录:
  • 美国化学文摘（网络版）
  • 被引量:6