2. 您的位置
3. 首页
4. 会议论文
5. Electron Acceleration in a Dynamically Evolved Current Sheet of Solar Coronal Conditions

Electron Acceleration in a Dynamically Evolved Current Sheet of Solar Coronal Conditions

来源 :The Fourteenth International Solar Wind Conference (第十四届国际太阳 | 被引量 : 0次 | 上传用户：simeifang

【摘 要】

：

Electron acceleration in a drastically evolved current sheet of solar coronal conditionsis investigated via the combined 2.5-D resistiveMHD and test particle approaches.

【作 者】

：

Shaohua Zhang A.M.Du Xueshang Feng Xin Cao Quanming Lu Liping Yang Gengxiong Chen 

【机 构】

：

Institute of Geology and Geophysics,CAS,Beijing 100029,China;Beijing Institute of Satellite Environm

【出 处】

：

The Fourteenth International Solar Wind Conference (第十四届国际太阳

【发表日期】

：

2015年5期

下载到本地 , 更方便阅读

下载此文 赞助VIP

声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架

论文部分内容阅读

Electron acceleration in a drastically evolved current sheet of solar coronal conditionsis investigated via the combined 2.5-D resistiveMHD and test particle approaches.

其他文献

Response of dayside magnetosphere and ionosphere to solar wind dynamic pressure pulse

We showed the response processes of dayside magnetosphere and the ground magnetic fields to the sudden increase of solar wind dynamic pressure with THEMIS and GOES observations.

会议

The Engetic Particles in Shock-ICME In

In 2008,Shen et al.reported that the intensity of the solar energetic particles(SEP) in the shock-MC interaction structure would increase greatly.

会议

Study of Solar Wind driving on the fractality of the Earth's magnetosphere through an MHD shell

In a previous work,we have studied the temporal evolution of geomagnetic activity,by calculating af ractal dimension from Dst data(Domínguez et all,JGR 119,5(2014)}.The fractal dimension decreases dur

会议

Characteristic Signatures of Radial or Local Acceleration of relativistic electron in earth radiatio

Radiation belt science has several enigmatic issues among which is the yet unexplained electron acceleration in the million electron Volt(MeV) energy range.

会议

Exploring the possible relationship between field-line currents and shock auroras

Shock auroras have been focused on recently,since they are considered as one important way of transferring energy from solar wind to the magnetosphere.

会议

Special position of crossing the magnetopause in the distant magnetotail-Windsock effect

Combining with ARTEMIS(P1 and P2),Wind and other satellites data,we present the discovery of high-speed flow of high density in the distant tail under the northward interplanetary magnetic field(IMF)

会议

Simulation of Quiet-Sun Hard X-rays Related to Solar Wind Superhalo Electrons

Here we present an estimate of the quiet-sun HXR emission from electrons accelerated in nanoflares.First,we assume that some ofthe accelerated electrons in nanoflareswould travel downwards and collide

会议

Solar Wind Superhalo Electrons at Quiet times

High-energy superhalo electrons are present in the interplanetary medium even in the absence of any solar activity,carrying important information on electron acceleration in the solar wind.

会议

The Angular Distribution of Solar Wind Superhalo Electrons at Quiet Times

The angular distribution of solar wind superhalo electrons carries important information on the electron acceleration location and scattering in the interplanetary medium.Here we present a comprehensi

会议

INTERPRETATION OF THE TIME-INTENSITY PROFILE OF THE 15 MARCH 2013 SOLAR ENERGETIC PARTICLE EVENT WIT

The coronal mass ejection(CME) event on March 15,2013 is one of the few solar events in cycle 24 that produced a large solar energetic particle(SEP) event and severe geomagnetic activity.Observations

会议