灵敏 发表于 2025-3-25 07:17:56

Introduction, Objectives, and Scope,ov et al (1961, 1962), Engel (1965), Andronov and Trakhtengerts (1964), and Lutomirskiand Sudan (1966), but the problem was treated in a slightly different way which is applicable to the physical situation.

格子架 发表于 2025-3-25 08:42:55

http://reply.papertrans.cn/24/2389/238885/238885_22.png

homeostasis 发表于 2025-3-25 13:30:48

http://reply.papertrans.cn/24/2389/238885/238885_23.png

相符 发表于 2025-3-25 19:38:30

Effect of a Large Amplitude Wave Packet and Second Order Resonance on the Stimulation of VLF Emissioov et al (1961, 1962), Engel (1965), Andronov and Trakhtengerts (1964), and Lutomirskiand Sudan (1966), but the problem was treated in a slightly different way which is applicable to the physical situation.

牵连 发表于 2025-3-25 21:41:45

http://reply.papertrans.cn/24/2389/238885/238885_25.png

流浪 发表于 2025-3-26 02:52:04

http://reply.papertrans.cn/24/2389/238885/238885_26.png

optional 发表于 2025-3-26 05:59:47

http://reply.papertrans.cn/24/2389/238885/238885_27.png

Fallibility 发表于 2025-3-26 11:42:32

http://reply.papertrans.cn/24/2389/238885/238885_28.png

宇宙你 发表于 2025-3-26 12:41:24

http://reply.papertrans.cn/24/2389/238885/238885_29.png

blister 发表于 2025-3-26 17:08:39

Wind Field Probabilistic Forecastingatmosphere of atomic hydrogen visible in the resonance line Lyman α 1216 Å; the probability for excitation of this line by the flux of solar Lyman α quanta is once every few minutes, at the solar distance in question.
页: 1 2 [3] 4 5 6 7
查看完整版本: Titlebook: Cosmic Plasma Physics; Proceedings of the C Karl Schindler Conference proceedings 1972 Plenum Press, New York 1972 Plasma.electron.fields.i