Plasma Blobs and Turbulence Impacting Magnetic Confinement(A Short Review)  

作　　者：Rahele Zadfathollah Seyed Kamal Mousavi Balgehshiri Ali Zamani Paydar Bahman Zohuri 

机构地区：[1]Department of Physics,K.N.Toosi University of Technology,Tehran,P.O.BOX 15875-4416,Iran [2]Physics and Energy Engineering Department,Amirkabir University of Technology,Tehran,Iran [3]Galaxy Advanced Engineering,Albuquerque,New Mexico 87111,United States of America

出　　处：《Journal of Energy and Power Engineering》2023年第1期1-10,共10页能源与动力工程（美国大卫英文）

摘　　要：Space-based plasma(i.e.,a highly ionized gas or the fourth state of matter)blobs are isolated pockets of this highly ionized gas made up of charged particles.These blobs are believed to have a substantial impact on the structure and dynamics of the cosmos and can be seen in a variety of astronomical objects,including stars,galaxies,and the intergalactic medium.Some plasma blobs are connected to intense phenomena like magnetic reconnection,shock waves,and supernovae,while others may be the result of more passive processes like cooling and gravitational collapse.In both astrophysics and plasma physics,there is ongoing research on the characteristics and behavior of plasma blobs.This phenomenon has a very adverse effect on tokamak-based MCF(magnetic confinement fusion),which is the subject of this short review paper.

关 键 词：Plasma blobs plasma edge INTERSTELLAR magnetic reconnection TOKAMAK MCF 

分 类 号：P14[天文地球—天体物理]