柳条筐
发表于 2025-3-21 20:08:11
书目名称Microphysics of Cosmic Plasmas影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0633379<br><br> <br><br>书目名称Microphysics of Cosmic Plasmas读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0633379<br><br> <br><br>
Benign
发表于 2025-3-21 22:01:08
Solar Wind Turbulence and the Role of Ion Instabilities,obability distribution functions of different plasma parameters are not Gaussian, indicating presence of intermittency. At the moment there is no global model taking into account all these observed properties of the inertial range. At ion scales, turbulent spectra have a break, compressibility incre
公社
发表于 2025-3-22 02:21:26
Solar Surface and Atmospheric Dynamics,ism inferred from Hanle measurements are converging towards a similar description. They are both described as randomly oriented, largely transverse fields in the several hecto-Gauss range. These similarities are ever making more natural to assume that they are the same. However, and because of the l
Neuropeptides
发表于 2025-3-22 05:46:33
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训诫
发表于 2025-3-22 10:06:30
Notes on Magnetohydrodynamics of Magnetic Reconnection in Turbulent Media, the reconnecting system—can make reconnection independent on the microphysical properties of plasmas. We will also show how relaxation theory can be used to calculate the energy dissipated in turbulent reconnecting fields. As well as heating the plasma, the energy dissipated by turbulent reconnecti
incontinence
发表于 2025-3-22 16:13:49
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flourish
发表于 2025-3-22 19:47:22
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贫穷地活
发表于 2025-3-22 21:20:30
The Dynamic Quasiperpendicular Shock: Cluster Discoveries,lly dependent upon the characteristic spatial scales of the ramp and foot region provided that the shock is stationary. The process of shock formation consists of the steepening of a large amplitude nonlinear wave. At some point in its evolution the steepening is arrested by processes occurring with
insightful
发表于 2025-3-23 04:32:05
Book 2014the extensive existing knowledge of laboratory plasmas as applied to astrophysical problems are also covered. This volume is aimed at graduate students and researchers active in the areas of cosmic plasmas and space science. Originally published in Space Science Reviews journal, Vol. 278/2-4, 2013.
冒失
发表于 2025-3-23 09:24:18
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