【摘 要】
：
We propose a new and elegant approach to study the cusps by using remote X-ray imaging,which is now possible thanks to the relatively recent discovery of solar wind charge exchange(SWCX) X-ray emissio
【机 构】
：
University College London/MSSL,UK National Space
【出 处】
：
The Fourteenth International Solar Wind Conference (第十四届国际太阳
论文部分内容阅读
We propose a new and elegant approach to study the cusps by using remote X-ray imaging,which is now possible thanks to the relatively recent discovery of solar wind charge exchange(SWCX) X-ray emission,found to be occurring in the vicinity of the Earths magnetosphere and especially in the day-sidemagnetosheath and the cusps,where the exospheric neutrals density is high.
其他文献
Shock auroras have been focused on recently,since they are considered as one important way of transferring energy from solar wind to the magnetosphere.
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)
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
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.
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
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
Electron acceleration in a drastically evolved current sheet of solar coronal conditionsis investigated via the combined 2.5-D resistiveMHD and test particle approaches.
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
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-
The evolution of Solar Energetic Particle(SEP) events is characterized by particle varying spatial and energy distributions.In many cases,it is of primary importance to evaluate how the performance of