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{{Expand|time=2013-02-13T07:55:33+00:00 }} {{noteTA |1 = zh-hans:等离子体; zh-hant:電漿; |2 = zh-hans:阿尔文波; zh-hant:阿耳芬波; }} '''阿尔文波''',又称'''剪切阿尔文波''',是[[等离子体]]中的一种沿[[磁场]]方向传播的[[波]],这种波的[[頻率 (物理學)|频率]]远低于等离子体的回旋频率,是一种[[线偏振]]的低频[[横波]]。处在磁场中的导电流体在垂直于磁场的方向上受到局部扰动时,沿着磁感线方向的磁张力提供恢复力,就会激发阿尔文波。阿尔文波是由瑞典物理学家[[汉尼斯·阿尔文]]首先预言的,因此得名。后来[[隆德奎斯特]]({{lang|en|Lundquist}})使用1特斯拉左右的磁场在水银中观察到了阿尔文波,列纳尔特({{lang|en|Lehnert}})使用液态钠也证实了阿尔文波的存在。 [[File:Observations_Reshape_Basic_Plasma_Wave_Physics.webm|缩略图|运动的阿尔文波。]] [[File:Alfven-wave-double-layer.gif|缩略图|A cluster of double layers forming in an Alfvén wave, about a sixth of the distance from the left.<br />图例:<br /><span style="color:red">红色</span>=electrons<br /><span style="color:green">绿色</span>=ions<br /><span style="color:gold">黄色</span>=electric potential<br /><span style="color:orange">橙色</span>=parallel electric field<br /><span style="color:hotpink">粉色</span>=charge density<br /><span style="color:blue">蓝色</span>=magnetic field]] 阿尔文波的[[色散关系]]为: :<math>\omega^2=k^2v_A^2\cos^2\theta</math> 这样的波称为斜阿尔文波。''θ''=0时是沿着磁感线的方向传播的,称为阿尔文波。此时阿尔文波的[[相速度]]为: :<math>v_A=\frac{B}{\sqrt{\mu_0\rho_0}}</math> 称为'''阿尔文速度''',其中''μ''<sub>0</sub>是等离子体的[[磁导率]],''ρ''<sub>0</sub>是离子的密度。在垂直于磁感线的方向上阿尔文波不能传播。 == 阿尔文时间 == 在[[等离子体物理]]中, 阿尔文时间<math> \tau_A </math>是波动现象的一个重要时标。它和阿尔文速度的关系为: :<math>\tau_A = \frac{a}{v_A}</math> 式中<math> a </math> 代表了系统的特征尺度。例如,<math> a </math> 是[[托卡马克]]中较小的环的半径。 == 参见 == *[[压缩阿尔文波]] == 延伸阅读 == * {{Citation |last=Alfvén |first=H. |title=Existence of electromagnetic-hydrodynamic waves |journal=[[Nature (journal)|Nature]] |date=1942 |volume=150 |issue=3805 |pages=405–406 |doi=10.1038/150405d0 |bibcode = 1942Natur.150..405A }} * {{Citation |last=Alfvén |first=H. |title=Cosmic Plasma |location=Holland |publisher=Reidel |date=1981 |isbn=90-277-1151-8 }} * {{Citation |last=Aschwanden |first=M. 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