营养品
发表于 2025-3-21 20:03:25
书目名称Cosmic Plasma Physics影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0238885<br><br> <br><br>书目名称Cosmic Plasma Physics读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0238885<br><br> <br><br>
maroon
发表于 2025-3-21 23:35:56
Parametric Instabilities Generated in the Ionosphere by Intense Radio Wavesy. The energy content of 100 cubic kilometers of ionospheric plasma is of the order of 10 megawatt-secs. This estimate, coupled with an electron-ion temperature relaxation time ~ 10 secs, suggests the H. F. frequency transmitters in the megawatt power range can significantly alter the ionosphere pro
FOLLY
发表于 2025-3-22 00:50:20
Study of a Jovian Plasmasphere and the Occurrence of Jupiter Radioburstsuence of Io on the emission of the radiobursts. Duncan (1970) proposed that Io stimulates the emission when it crosses the “magnetopause” of Jupiter, Melrose (1967) suggested that the motion of Io through a “corotating region” inside the magnetosphere of Jupiter may be the cause.
寻找
发表于 2025-3-22 07:01:20
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judicial
发表于 2025-3-22 12:32:43
Universal Instability Associated with the Plasmapause and Its Role in Geomagnetic Micropulsationse theory and laboratory experiments of a non-homogeneous magnetoplasma. Drift waves excited at the plasmapause may be unstable in the direction of the electron drift and propagate eastwards nearly perpendicular to the magnetic field. The drift waves, however, tend to convert very soon to ion sound o
Texture
发表于 2025-3-22 14:26:25
Deformation and Striation of Barium Clouds in the Ionospherevoted to the theory of plasma clouds which are sufficiently large to dominate the Pederson conductivity on lines of force which pass through the cloud and sufficiently high so that K. = Ω./.. ≫ 1. Figure 1 shows the model.
Texture
发表于 2025-3-22 20:20:24
Thermal Energy Transport in the Solar Winds with the theory for collision-dominated heat transport in a fully ionized medium developed by Spitzer and Härm . A short discussion of some recent models is included to illustrate the role of thermal conduction in the expansion. In addition, a brief description of the steady state solar wind
非实体
发表于 2025-3-23 00:29:00
Influence of Neutral Interstellar Matter on the Expansion of the Solar Windially constant expansion velocity. This solution is derived from a hydrodynamical treatment of the coronal expansion that does not take into account any interaction of the solar wind plasma with neutral interstellar matter which enters the solar system. In that case the supersonic solar wind expands
Urea508
发表于 2025-3-23 02:26:18
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THROB
发表于 2025-3-23 06:11:01
Heating of the Solar Wind Ionsn influx of neutral hydrogen from the boundary of the heliospher’e. Photoionisation and charge exchange trans-form neutral hydrogen atoms into protons. The ionised hydrogen component near the Earth’s orbit is then double-peaked and unstable. The kinetic energy of the protons (originating from the ne