期刊
ASTROPHYSICAL JOURNAL
卷 666, 期 2, 页码 1277-1283出版社
UNIV CHICAGO PRESS
DOI: 10.1086/518828
关键词
magnetic fields; MHD; shock waves; Sun : chromosphere
We present the results of numerical simulations of shock wave-driven jets in the solar atmosphere. The dependence of observable quantities such as maximum velocity and deceleration on parameters such as the period and amplitude of initial disturbances and the inclination of the magnetic field is investigated. Our simulations show excellent agreement with observations, and shed new light on the correlation between velocity and deceleration and on the regional differences found in observations.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据