Titlebook: Microphysics of Cosmic Plasmas; André Balogh,Andrei Bykov,John Raymond Book 2014 Springer Science+Business Media New York 2014 Collisionle

柳條筐

書(shū)目名稱Microphysics of Cosmic Plasmas影響因子(影響力)




書(shū)目名稱Microphysics of Cosmic Plasmas影響因子(影響力)學(xué)科排名




書(shū)目名稱Microphysics of Cosmic Plasmas網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Microphysics of Cosmic Plasmas網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Microphysics of Cosmic Plasmas被引頻次




書(shū)目名稱Microphysics of Cosmic Plasmas被引頻次學(xué)科排名




書(shū)目名稱Microphysics of Cosmic Plasmas年度引用




書(shū)目名稱Microphysics of Cosmic Plasmas年度引用學(xué)科排名




書(shū)目名稱Microphysics of Cosmic Plasmas讀者反饋




書(shū)目名稱Microphysics of Cosmic Plasmas讀者反饋學(xué)科排名

Benign

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

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

訓(xùn)誡

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

flourish

貧窮地活

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

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