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金星电离层的热结构和主要离子成分:金星轨道飞行器的首次 RPA 结果。

Thermal Structure and Major Ion Composition of the Venus Ionosphere: First RPA Results from Venus Orbiter.

出版信息

Science. 1979 Feb 23;203(4382):757-63. doi: 10.1126/science.203.4382.757.

Abstract

Thermal plasma quantities measured by, the retarding potential analyzer (RPA) are, together with companion Pioneer Venus measurements, the first in situ measurements of the Venus ionosphere. High ionospheric ion and electron temperatures imply significant solar wind heating of the ionosphere. Comparison of the measured altitude profiles of the dominant ions with an initial modlel indicates that the ionosphere is close to diffusive equilibrium. The ionopause height was observed to vary from 400 to 1000 kilometers in early orbits. The ionospheric particle pressure at the ionopause is apparently balanced at a solar zenith angle of about 70 degrees by the magnetic field pressure with little contribution from energetic solar wind particles. The measured ratio of ionospheric scale height to ionopause radius is consistent with that inferred from previously measured bow shock positions.

摘要

由阻滞电位分析仪(RPA)测量的热等离子体参数,以及先驱者金星的测量结果,是金星电离层的首次原位测量。高电离层离子和电子温度意味着电离层受到了太阳风的显著加热。将测量到的主要离子的高度分布与初始模型进行比较表明,电离层接近扩散平衡。在早期轨道中,观测到离子层顶高度从 400 公里到 1000 公里不等。在太阳天顶角约 70 度处,离子层顶处的离子体压力显然与磁场压力平衡,而高能太阳风粒子的贡献很小。测量到的电离层尺度高度与离子层顶半径的比值与先前测量的弓形激波位置推断出的结果一致。

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