2. 您的位置
3. 首页
4. 会议论文
5. Quasi-periodic Fast-mode Magnetosonic Wave Trains Within Coronal Waveguides Associated with Flares/C

Quasi-periodic Fast-mode Magnetosonic Wave Trains Within Coronal Waveguides Associated with Flares/C

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：shtour

【摘 要】

：

Quasi-periodic,fast-propagating wave trains(QFPs;Liu et al.2011,2012 ApJ) are a new observational phenomenon recently discovered in the corona by SDO/AIA with extreme ultraviolet(EUV) imaging observat

【作 者】

：

Liu Wei Ofman Leon Karlicky Marian DePontieu Bart 

【机 构】

：

Lockheed Martin Solar and Astrophysics Laboratory,Palo Alto,CA,USA;Stanford University,Stanford,CA,U

【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

Quasi-periodic,fast-propagating wave trains(QFPs;Liu et al.2011,2012 ApJ) are a new observational phenomenon recently discovered in the corona by SDO/AIA with extreme ultraviolet(EUV) imaging observations.

其他文献

Transpolar arc observation after solar wind entry into high latitude magnetosphere

Recently,Cluster observations revealed the presence of new regions of solar wind plasma entry at the high latitude magnetospheric lobes tailward of the cusp region,mostly during periods of northward I

会议

Planetary turbulence:survey of Cassini data in the Saturn's magnetosheath

Turbulence is one of the most important yet not fully understood topics of modern physics.Understanding turbulence is collisionless plasmas,where kinetic effects mediate interactions between fields an

会议

The control of Martian ionopause altitude by the crustal and induced magnetic field strength

The Martian ionosphere directly interacts with solar wind due to lack of a significant intrinsic magnetic field,however,the interaction is significantly influenced by the crustal field and induced fie

会议

Interstellar Flow Direction from Pickup Ion Cut-off Dependence on Longitude,Flow Speed,and Solar Win

The precise interstellar neutral(ISN) flow direction is important because of its strong leverage on the plane subtended by the ISN vector and magnetic field,which controls the heliosphericshape and in

会议

Heliospheric boundary in the backscattered solar Lyman-alpha radiation:analysis of Voyager-1/UVS dat

UVS instrument onboard Voyager-1 has been performing measurements of the backscattered solar Lyman-alpha emissions for more than 35 years.

会议

Energetic neutral atom and interstellar flow observations with IBEX,implications on the global helio

The IBEX ribbon has been separated from the surrounding globally distributed flux(GDF),revealing ENA emission largely from the inner heliosheath.

会议

The Outer Boundary Conditions of the Heliosphere:Observations and Models ofthe Local Interstellar Cl

The complex interaction of the very local interstellar medium(VLISM) and thesolar wind is what creates the heliosphere and therefore understanding theheliosphere requires knowledge of the nature of th

会议

Global Distribution of the Solar Wind and its Evolution during Cycles 22-24L

Ground-based observations of interplanetary scintillation(IPS) enable determination of global distribution of the solar wind speed and(electron) density fluctuations(delta Ne)in a short time comparabl

会议

The coincided heliospheric current sheet and stream interface:implications for the origin and evolut

In general,the heliospheric current sheet,which defines the boundary of sunward and anti-sunward magnetic field is encased by the slow solar wind;the stream interface,which defines the boundary betwee

会议

A POSSIBLE CAUSE OF THE EXTREMELY LOW SOLAR WIND DENSITY AND MAGNETIC FIELD DURING THE 2007-2009 SOL

The unusual low solar wind density and weak magnetic field observed at the near-Earth orbit during the 2007-2009 solar minimum years has been an actively studied subject.

会议