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学术报告

德国马普所Hardi Peter博士学术报告

NOV
28

德国马普所Hardi Peter博士将于本周作两次学术报告,全面介绍太阳过渡区的观测和模拟的最新进展。

报告一:
时间:2011年11月11日上午10:00
地点:北京大学物理大楼北415
题目:The Solar Transition Region - A Key to Understand the Corona

报告二:
时间:2011年11月16日下午3:00
地点:北京大学物理大楼北415
题目:Structure and Dynamics of the Solar Corona

田晖博士学术报告

NOV
28

时间:2011年11日下午2:30
地点:北京大学物理大楼北415
题目:Ubiquitous high-speed solar coronal outflows revealed by both imaging and spectroscopic observations

赵学溥教授学术报告

NOV
28

2011年10月19日下午2:30在北京大学物理北楼415由赵学溥教授作学术报告。

报告内容: 关于太阳风的最新进展。

Dong-Hun Lee教授学术报告

OCT
17

本周Dong-Hun Lee教授的两个学术报告:

1、EMIC wave coupling in space
时间:2011年10月19日下午4:00
地点:物理北楼415

2、Nonlinear MHD Waves in Space
时间:2011年10月20日下午4:00
地点:物理北楼415

9月27日Tony Lui教授作学术报告

OCT
17

2011年9月27日下午2:00 Geroge Parks学术报告。

报告题目:Energy source for auroral electrons from two proposed substorm onset process

摘要:There are two main processes in the tail that are proposed to link electron precipitation for the auroral arc during substorms. These are current disruption/dipolarization (CDD) and magnetic reconnection (MR). To provide further clues in differentiating these two processes, we examine the electron energy spectrum and the associated total field-aligned energy flux during six CDD events and compare them with five MR events. It is found that (1) the total field-aligned electron energy flux from CDD sites is generally high enough to account for the energy flux required to produce bright auroral arcs and (2) the total field-aligned electron energy flux from MR sites is generally a factor of one to two orders of magnitude lower than that from CDD sites. These results favor a direct link between the CDD sites and the substorm arcs. Further acceleration by other mechanisms is considered with the result that inclusion of other mechanisms is unlikely to alter the differences obtained in this analysis.

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