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首页> 外文期刊>The Astrophysical journal >SOLAR WIND ELECTRIC FIELDS IN THE ION CYCLOTRON FREQUENCY RANGE
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SOLAR WIND ELECTRIC FIELDS IN THE ION CYCLOTRON FREQUENCY RANGE

机译:离子回旋频率范围内的太阳风电场

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Measurements of fluctuations of electric fields in the frequency range from a fraction of 1 to 12.5 Hz are presented and corrected for the Lorentz transformation of magnetic fluctuations to give the electric fields in the plasma frame. The electric fields are large enough to provide the dominant force on the ions of the solar wind in the region near the ion cyclotron frequency of protons, larger than the force due to magnetic fluctuations. They provide sufficient velocity-space diffusion or heating to counteract conservation of magnetic moment in the expanding solar wind to maintain nearly isotropic velocity distributions.
机译:给出了从1到12.5 Hz的频率范围内的电场波动的测量结果,并针对磁波动的Lorentz变换进行了校正,以给出等离子体框架中的电场。电场足够大,可以在质子的离子回旋加速器频率附近的区域中对太阳风的离子提供主力,该主力大于由磁波动引起的力。它们提供了足够的速度空间扩散或加热,以抵消膨胀的太阳风中的磁矩守恒,从而保持接近各向同性的速度分布。

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