Conductive Polyaniline/Viscose Fiber Composites

来源 :2015 International Conference on Advanced Fibers and Polymer | 被引量 : 0次 | 上传用户：wangliang19910125

【摘要】

：

INTRODUCTION The discovery of conducting polymers has opened up a new promising field in material science and engineering.Among them,polyaniline(PANI) is one of the most promising conducting polymers

【作者】

：

Wang Ning Li Guodong Zhang Xingxiang Liu Dongqi

【机构】

：

Tianjin Municipal Key Lab of Fiber Modification and Functional Fiber,School of Material Science and

【出处】

：

2015 International Conference on Advanced Fibers and Polymer

【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

INTRODUCTION The discovery of conducting polymers has opened up a new promising field in material science and engineering.Among them,polyaniline(PANI) is one of the most promising conducting polymers because of its unique properties,its ease of preparation,and excellent environmental stability.[1] PANI has the utilization potential in a large number of applications.

其他文献

Numerical Study of Erosion,Heating,and Acceleration of Magnetic Cloud as Impacted by Fast Shock

Both coronal mass ejections(CMEs) and corotating interaction regions(CIRs) can be sources of space weather disaster.The impact of fast shock on magnetic cloud is a pivotal process in CME-CME interacti

会议

Solar Wind Entry into the High-latitude Magnetospheric Lobes--Cluster Observations

During the quiet time when the interplanetary magnetic field(IMF) is northward,using Cluster multi-spacecraftdata between August and October from 2002 to 2004,Shi et al.

会议

Prediction of interplanetary shocks' arrival times at Earth

Prediction of the shocks arrival times(SATs) at the Earth is very important for space weather forecast.There is a well-known SAT model,STOA,which is widely used in the space weather forecast.

会议

Comparing the PFSS coronal magnetic field prediction with the observed heliospheric magnetic field a

The solar coronal field forms an important link between the underlying source in the solar photosphere and the heliospheric magnetic field emanating away from the Sun with the solar wind.Since the cor

会议

ION KINETIC ENERGY CONSERVATION AND MAGNETIC FIELD STRENGTH CONSTANCY IN MULTI-FLUID SOLAR WIND ALFV

We investigate properties of the plasma fluid motion in the large amplitude low frequency fluctuations of highly Alfvénic fast solar wind.We show that protons locally conserve total kinetic energy whe

会议

Influence of Intermittency on the Anisotropy of Magnetic Structure Functions of Solar Wind Turbulenc

Intermittency is a significant component of solar wind turbulence,and appears to be closely connected with the spectral anisotropy of turbulence.We use the Local Intermittency Measure(LIM) to identify

会议

Magnetic cloud observations from MESSENGER and Venus Express

We present statistical findings from a recently compiled catalogue of magnetic clouds observed by the MESSENGER and Venus Express spacecraft. Despite their planetary focus, both spacecraft spent signi

会议

Solar-Cycle Statistics of Solar Wind Proton and Electron properties and coupling:Implications for So

We present a study of statistics of protons and electron properties in the solar wind at 1 AU using new Wind proton and electron data products over more than a solar cycle(1995-2009).

会议

The dispersion relations and instability thresholds of alpha particle firehose modes in the presence

In situ measurements have shown that the less-abundant alpha particles are characterized by temperature anisotropy which could drive the anisotropy-driven kinetic instabilities in the solar wind.

会议

Observed electron energetics in the expanding solar wind plasma

We present an observational analysis of cooling/heating rates of electrons in the expanding solar wind plasma.Our study is based on HELIOS spacecraft dataset ranging from 0.3 to 1 AU in the ecliptic p

会议

Conductive Polyaniline/Viscose Fiber Composites

其他学术论文