Solar Orbiter-Exploring the Sun-Heliosphere Connection

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:zouxudong163
下载到本地 , 更方便阅读
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
Solar Orbiter, the first mission of ESAs Cosmic Vision 2015-2025 programme, promises to deliver groundbreaking science with previously unavailable observational capabilities provided by a suite of in-situ and remote-sensing instruments in a unique orbit.
其他文献
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
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
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
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
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
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 carries important information on the electron acceleration location and scattering in the interplanetary medium.Here we present a comprehensi
会议
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
Electron acceleration in a drastically evolved current sheet of solar coronal conditionsis investigated via the combined 2.5-D resistiveMHD and test particle approaches.
会议
Corotating interaction regions(CIRs) are produced as a result of the interaction between fast and slow solar-wind streams,and quite ubiquitous in every region of the heliosphere.Observations shown tha
会议