Titlebook: Unstable Current Systems and Plasma Instabilities in Astrophysics; Proceedings of the 1 Mukul R. Kundu,Gordon D. Holman Conference proceedi

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書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics影響因子(影響力)




書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics影響因子(影響力)學(xué)科排名




書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics被引頻次




書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics被引頻次學(xué)科排名




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書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics年度引用學(xué)科排名




書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics讀者反饋




書(shū)目名稱Unstable Current Systems and Plasma Instabilities in Astrophysics讀者反饋學(xué)科排名

blister

Magnetic Flux Ropes of Venus: A Paradigm for Helical Magnetic Structures in Astrophysical Systemspes may be unstable to the helical kink mode. Statistics of rope distribution and orientation also support this instability picture. The results of investigations into the direct measurements of Venus flux ropes may be relevant to certain astrophysical phenomena that must be observed remotely.

intrigue

Computer Simulation of Reconnection in Planetary Magnetospheressed on two-dimensional steady state models and linear analytic theory. The three-dimensional models in particular have also added a lot more information on the reconnection process and the structure of flow, magnetic fields, and currents including many features that are consistent with observations and empirical models of geomagnetic substorms.

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Introductory Remarks and astrophysicists, to permit cross-fertilization of knowledge and ideas on related problems. These problems refer to understanding collective effects and their signatures in unstable magnetized plasmas. Similar processes play an important role in problems as diverse as the stability of jets in ex

gimmick

Sleep-Paralysis

Patchy Reconnection and Magnetic Ropes in Astrophysical Plasmaschy, forming tubes of twisted flux. The passage of one of these twisted tubes has been called a flux transfer event. Similar twisted tubes, or flux ropes, are formed at Venus by velocity shear. These tubes become so highly twisted that they become kink unstable. The presence of the kink instability

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Magnetic Flux Ropes of Venus: A Paradigm for Helical Magnetic Structures in Astrophysical Systemsrgely magnetic field-free ionosphere of the planet. They are so named because of their helical magnetic structure, which in turn is due to primarily field-aligned currents within the rope. Empirical models can be used to examine the current structure in detail, and these models indicate that flux ro

螢火蟲(chóng)

Coma704

hyperuricemia