【摘 要】
：
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.
【机 构】
：
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,School of
【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 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.
其他文献
Collisionless dissipation of anisotropic Alfvénic turbulence has been a promising candidate to solve the solar wind heating problem.Extensive studies have examined kinetic properties of Alfvén waves i
Coronal mass ejections(CMEs) are often accompanied by coronal dimming evident in extreme ultraviolet(EUV) and soft X-ray observations.The locations of dimming are sometimes considered to map footpoint
The interplanetary magnetic field(IMF) frozen in the solar wind,together with the solar EUV radiation,can significantly affect the location of Venusian bow shock.
Mercury has a weak but global magnetic field made of two main components,a dipolar and a quadrupolar ones [1-3].The weakness of the planetary field combined with the smallness of the planet leads to a
The UCSD interplanetary scintillation(IPS) remote-sensing analyses of the heliosphere have regularly measured and reconstructed 3D solar wind structure for nearly two decades.These analyses enable a r
Inner-source pickup ions are most likely created by the interaction of solar wind ions with interplanetary dust particles in the inner heliosphere,but their detailed production mechanism is still puzz
Using multi-point data from THEMIS,we report a magnetospheric vortex driven by a negative solar wind dynamic pressure pulse.The observed vortex,which was induced by a negative solar wind dynamic press
The Russell-Mcferren(R-M) effect is one of the best candidates to explain the seasonal variation in geomagnetic activity,which consider θ the angle between Z axis in geocentric solar magnetospheric(GS
Dust particles provide an important part of the matter composing the interplanetary medium;their mass flux at 1 AU is similar to that of the solar wind.Dust grains of nanometer size-scale can be detec
Solar wind controls the shape and motion of the terrestrial bow shock.Numerous observations of the the bow shock during last decades of spacecraft measurements are summarized in several bow shock mode