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Titlebook: Venus Aeronomy; C. T. Russell Book 1991 Kluwer Academic Publishers 1991 Aeronomy

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发表于 2025-3-21 18:53:17 | 显示全部楼层 |阅读模式
书目名称Venus Aeronomy
编辑C. T. Russell
视频video
图书封面Titlebook: Venus Aeronomy;  C. T. Russell Book 1991 Kluwer Academic Publishers 1991 Aeronomy
描述For almost three decades since Mariner 2 flew by the planet in December 1962, Venus has been the subject of intense investigation by both the Soviet and American space programs. Since the intrinsic magnetic field of Venus is exceedingly weak, if it exists at all, we expect many phenomena of the upper atmosphere and ionosphere of Venus to differ from their terrestrial counterparts. While flybys and landings of the many Venus missions provided useful data on these phenomena, orbital missions were needed for their detailed investigation. Such orbital missions were provided by the Soviet program with Veneras 9 and 10 in October 1975 and by the United States with the Pioneer Venus Orbiter in December 1978. Originally designed for a prime mission of only 243 days, the Pioneer Venus Orbiter is still functioning over a decade later, providing data nearly - hours a day through one of the most active solar cycles to date. We expect these transmis­ sions to continue until September 1992 when gravitation perturbations will lower the periapsis of the PVO orbit so that the spacecraft will be lost to the atmosphere. The Venera 9 and 10 and the Pioneer Venus observations have led to an explosion o
出版日期Book 1991
关键词Aeronomy
版次1
doihttps://doi.org/10.1007/978-94-011-3300-5
isbn_softcover978-94-010-5457-7
isbn_ebook978-94-011-3300-5
copyrightKluwer Academic Publishers 1991
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Venus Lightning,tning and signals above the electron gyrofrequency but at very low altitudes that may be due to the near field of the lightning. The VLF observations suggest that Venus lightning must be an intra-cloud phenomenon which is most frequent in the afternoon and evening sector. The occurrence rate is likely to be greater than on Earth.
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The Structure of the Venus Ionosphere,ts dynamics, and its magnetic properties. We also discuss some of the limitations that the orbit has placed on the spatial and temporal coverage of the ionosphere. For the benefit of future users of the data some of the factors which affect the measurement accuracies are discussed in an Appendix.
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Magnetic Fields in the Ionosphere of Venus,n developed to describe them over the last decade. The models for the ‘large-scale’ ionospheriç field have developed to the advanced stage of one-dimensional, self-consistent, multi-fluid MHD models which provide a detailed picture of the field in the subsolar region for specific upper boundary cond
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Plasma Waves at Venus,t whistler-mode waves in the magnetosheath of the planet may be an important source of energy for the topside ionosphere. Plasma waves are also associated with thickening of the ionopause current layer. Current-generated waves in plasma clouds may provide anomalous resistance resulting in electron a
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Venus Lightning,c signals detected by all 4 Venera landers are most readily explained as generation by lightning. The Venera 9 spectrometer appears to have observed a lightning storm on one occasion. The Pioneer Venus plasma wave instrument detects waves both below the electron gyrofrequency that may be due to ligh
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