2. 您的位置
3. 首页
4. 会议论文
5. Challenges for applying EIS for the research and production of lithium-ion battery

Challenges for applying EIS for the research and production of lithium-ion battery

来源 :First Asian Symposium on Impedance Spectroscopy for Elctroch | 被引量 : 0次 | 上传用户：DZLYSSY

【摘 要】

：

Electrochemical impedance spectroscopy (EIS),which is named AC Impedance in Early electrochemical literatures,has been widely applied in the research on lithium-ion battery in the past twenty years.

【作 者】

：

Quan-Chao Zhuang 

【机 构】

：

Lithium-ion Batteries Laboratory, School of Materials Science and Engineering, China University of M

【出 处】

：

First Asian Symposium on Impedance Spectroscopy for Elctroch

【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

Electrochemical impedance spectroscopy (EIS),which is named AC Impedance in Early electrochemical literatures,has been widely applied in the research on lithium-ion battery in the past twenty years.

其他文献

The Common-origin of Kinetic Turbulence and Electron-Halo of Velocity Distribution Function in the S

Observations of solar wind show that the power spectra of magnetic fluctuations break from Kolmogorov scaling law at ion inertial length.In addition,the electron velocity distribution function of sola

会议

Extremely Large EUV Late Phase of Solar Flares

The second peak in the Fe XVI 33.5 nm line irradiance observed during solar flares by Extreme ultraviolet Variability Experiment(EVE) is known as Extreme UltraViolet(EUV) late phase.

会议

Three-Dimensional Reconstruction of the Polar Jet on 17 June 2011 and its Presence in the Background

Large jets are some of the most enigmatic features of the polar solar wind.The analyses of the Hinode XRT,SDO/AIA,and coronagraph observations show that energetic solar jetting activity has a feature

会议

What kind of ARs may produce more CMEs?

Coronal mass ejections(CMEs),as sources of transient events in solar wind,mostly originated from active regions(ARs),are believed to be different phenomena compared with flares in a same eruptive proc

会议

Heating and Acceleration of Solar Wind Ions by Turbulent Wave Spectrum in Inhomogeneous Expanding Pl

Near the Sun(＜～10Rs) the acceleration,heating,and propagation of the solar wind is likely affected by the background inhomogeneities of the magnetized plasma.

会议

Weak magnetohydrodynamic turbulenceand intermittency

Three-dimensional numerical simulation is used to investigate intermittency in incompressible weak magnetohydrodynamic turbulence with a strong uniform magnetic field b0 and zero cross-helicity.

会议

Pickup ion mediated plasmas.1)Basic model and linear waves in the solar wind and local interstellar

Pickup ions(PUIs) in the outer heliosphere and the local interstellar medium(LISM) are created by charge exchange between protons and hydrogen(H) atoms,forming a thermodynamically dominant component.

会议

Simulations of Langmuir wave decay in inhomogeneous solar wind plasmas

Langmuir turbulence excited by electron flows in solar wind plasmas is studied on the basis of numerical simulations.In particular,nonlinear wave decay processes involving ion-sound waves are consider

会议

The Origin of Electron Core-Halo Features in the Solar Wind Electron Velocity Distribution Function:

The formation of the observed core-halo feature in the solar wind electron velocity distribution function is a long-time puzzle.In this letter based on the current knowledge of nanoflares we show that

会议

Observational Perspective of the Solar Wind:A Brief Overview

This paper provides a broad observation-based overview of the physical nature of the solar wind plasma and the embedded heliospheric magnetic field. Emphasis is on the spatial and temporal structure o

会议