• 不 限
  • 期刊论文
  • 硕博论文
  • 会议论文
  • 报 纸
  • 英文论文
  2. 您的位置
  3. 首页
  4. 会议论文
  5. Effect of the Interplanetary Medium on Nanodust Observations by the Solar Terrestrial Relations Obse

Effect of the Interplanetary Medium on Nanodust Observations by the Solar Terrestrial Relations Obse

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：xiansong2001
【摘 要】
：
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
【作 者】
：
G.Le Chat K.Issautier A.Zaslavsky F.Pantellini N.Meyer-Vernet S.Belheouane M.Maksimovic 
【机 构】
：
LESIA-Observatoire de Paris,CNRS,UPMC Univ.Paris 6,Univ.Paris Diderot,5 Place Jules Janssen,92195 Me
【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
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 detected using radio and plasma wave instruments because they move at roughly the solar wind speed.
其他文献
泡生法和热交换法蓝宝石不同生长阶段的数值模拟研究
分别针对典型的泡生法和热交换法蓝宝石单晶生长的不同生长阶段的温场、流场和固液界面形状进行数值模拟研究，模拟采用CGSim软件。模拟结果表明：在泡生法蓝宝石生长中，在靠近坩埚壁面和生长界面的熔体内，等温线分布密集，温度梯度较大。
会议
蓝宝石泡生法热交换法温场与流场数值模拟
Pb(In1/2Nb1/2)O3-PbTiO3晶体生长与性能表征
采用助熔剂坩埚下降法生长出最大尺寸为20×20×35mm3 的Pb(In1/2Nb1/2)O3-PbTiO3(PIN-PT)二元单晶,晶体外形呈现出自然生长面.XRD分析表明,该晶体具有纯钙钛矿相结构；利用电子探针显微分析仪(EPMA)分析了单晶的组成,在生长方向上PT含量存在差异,表明晶体生长过程中存在组分分凝；对单晶进行了定向并测试了其介电、压电、铁电性能,其中[001]方向单晶的室温相对介电
会议
PIN-PT坩埚下降法晶体生长性能表征
Effects of electron drifts on the collisionless damping of kinetic Alfvén waves in the solar wind
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
会议
THE NATURE OF CME-FLARE ASSOCIATED CORONAL DIMMING
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
会议
IMF control of the location of Venusian bow shock location
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.
会议
Simulating Mercury's interaction with the solar wind and the Hermean magnetosphere
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
会议
A Real-Time Global Solar Wind Boundary From Remotely-Sensed IPS Data For Driving 3D-MHD Models
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
会议
Inner-Source Heavy Pickup Ions:Results from SOHO/CELIAS/CTOF Measurements
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
会议
Magnetospheric vortices and their global effect after a negative solar wind dynamic pressure decreas
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
会议
Statistic result of Russell-Mcferren effect under northward IMF
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
会议