abandon 发表于 2025-3-21 18:53:17
书目名称Venus Aeronomy影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0981062<br><br> <br><br>书目名称Venus Aeronomy读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0981062<br><br> <br><br>权宜之计 发表于 2025-3-21 22:23:33
http://reply.papertrans.cn/99/9811/981062/981062_2.png兴奋过度 发表于 2025-3-22 02:04:23
http://reply.papertrans.cn/99/9811/981062/981062_3.pngfleeting 发表于 2025-3-22 06:46:17
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.BLUSH 发表于 2025-3-22 12:47:24
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.表两个 发表于 2025-3-22 13:25:02
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http://reply.papertrans.cn/99/9811/981062/981062_7.pngGlycogen 发表于 2025-3-23 00:45:13
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 condacrophobia 发表于 2025-3-23 03:58:42
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带伤害 发表于 2025-3-23 07:48:27
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