Temperature and flow velocity of the interplanetary gases along solar radii
Temperature and flow velocity of the interplanetary gases along solar radii
复制标题
沿太阳半径行星际气体的温度和流速
DOI：
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发表时间：
1979
期刊：
影响因子：
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通讯作者：
D. Judge
中科院分区：
文献类型：
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作者：
F. Wu;D. Judge
利用修正了损耗函数的Danby-Camm公式，计算了氢和氦在行星际空间沿太阳半径的速度分布。根据这些分布，确定了行星际气体的径向温度和径向速度。描述了由于电荷交换和光致电离引起的太阳引力和电离损耗对气体温度和速度的影响。
The velocity distributions along solar radii for hydrogen and helium in interplanetary space are calculated by using the Danby-Camm formula modified with a loss function. From these distributions the radial temperature and radial flow velocity of the interplanetary gases are determined. The effects of solar gravitation and ionization loss, due to charge exchange and photoionization, on the gas temperature and velocity are described.