特邀阿拉巴马大学胡强教授到我校作学术报告

题目：Grad-Shafranov （GS） 磁云重构的应用和最新进展

时间：6月4日下午3：00-

地点：尚贤楼808

欢迎广大师生前来参加。

数学与统计学院

2014年6月3日

内容概括：

In this talk, I will discuss the basic features and procedures of Grad-Shafranov (GS) reconstruction technique as applied to in-situ observations of magnetic flux ropes embedded within large-scale Interplanetary Coronal Mass Ejections (ICMEs). The method is capable of deriving a fully two-dimensional cross-section of a cylindrical structure utilizing both magnetic and plasma measurements along the spacecraft path across the structure. The method has been applied to examine various magnetic flux-rope structures and to connect with solar source region properties. Recent progress includes more detailed study of the twist distributions within flux ropes. We will discuss the results for a number of events and their implications for the formation and origination of magnetic flux ropes on the Sun.

胡强教授简介：

1989 - 1994, B.S., in Space Physics, USTC
1994 - 1997, M.S., in space physics, 中科院空间中心
1997 － 2001, Ph.D., in Engineering Sciences, Dartmouth College
2001- 2003, Postdoc, Bartol Research Institute, Univ. of Delaware
2004-2009, Research Scientist, Institute of Geophysics and Planetary Phys., Univ of California, Riverside
2009-2012, Research Scientist, Center of Space Plasma and Aeronomic Research, UAH
2012 - present, Assistant Professor, Department of Space Science, UAH