这两类太阳风探测仪都是通过测量太阳风粒子的E/Q谱的空间分布来确定太阳风速度、温度和数密度。
Both of the two kinds of detectors can obtain the spectral of E/Q ofions. Then the velocity, temperature and density distributions can be obtained by E/Qspectral.
当打在旅行者1号前端的带电粒子速度等于飞船自身速度时，研究人员意识到此时总的向外的太阳风速已经变成了零。
When the speed of the charged particles hitting the outward face of Voyager 1 matched the spacecraft's speed, researchers knew that the net outward speed of the solar wind was zero.
当打在旅行者1号前端的带电粒子速度等于飞船自身速度时，研究人员意识到此时总的向外的太阳风速已经变成了零。
When the speed of the charged particles hitting the outward face of Voyager 1 matched the spacecraft's speed, researchers knew that the net outward speed of the solar wind was zero.
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