Titlebook: Auroral Plasma Physics; G?tz Paschmann,Stein Haaland,Rudolf Treumann Book 2003 Springer Science+Business Media Dordrecht 2003 HTS.Planet.R

租期

書目名稱Auroral Plasma Physics影響因子(影響力)




書目名稱Auroral Plasma Physics影響因子(影響力)學(xué)科排名




書目名稱Auroral Plasma Physics網(wǎng)絡(luò)公開度




書目名稱Auroral Plasma Physics網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Auroral Plasma Physics被引頻次




書目名稱Auroral Plasma Physics被引頻次學(xué)科排名




書目名稱Auroral Plasma Physics年度引用




書目名稱Auroral Plasma Physics年度引用學(xué)科排名




書目名稱Auroral Plasma Physics讀者反饋




書目名稱Auroral Plasma Physics讀者反饋學(xué)科排名

吞下

https://doi.org/10.1007/978-94-007-0127-4 and energy transfer processes: magnetospheric/ionospheric coupling, Alfvén waves. In Chapter 2, we summarized the visible manifestations of these processes; here, using the theoretical tools provided in Chapter 3, we study the underlying plasma physics.

farewell

Remote Sensing of Auroral Arcs,e and ultraviolet imagers on polar-orbiting satellites, ground-based all-sky and meridian-scanning photometer arrays, ground-based magnetometer arrays, coherent backscatter radar measurements of ionospheric convection, and incoherent-scatter radar measurements of the ionospheric density, velocity and temperature distribution.

左右連貫

In Situ Measurements in the Auroral Plasma, and energy transfer processes: magnetospheric/ionospheric coupling, Alfvén waves. In Chapter 2, we summarized the visible manifestations of these processes; here, using the theoretical tools provided in Chapter 3, we study the underlying plasma physics.

1FAWN

cardiac-arrest

insipid

Introduction, the present book. With a better understanding, we can enjoy the beauty of aurorae in a much deeper sense, just like music opens for those who are willing to invest their time to understand the structure and dynamics of the musical system.

圓錐體

Tsjalling Swierstra,Jozef Keulartzgions are essential in producing auroral forms: a generator region located far out in the magnetosphere, where magnetospheric energy is tapped to power the aurora, and an acceleration region located some 1000s of km above the atmosphere, where electrical energy is converted into particle kinetic energy.

熱烈的歡迎

Antecedent

Athanasios Zavras DMD, DDS, MS, DrMedScduring times of magnetospheric activity, such as storms and substorms. Although a full treatment of the storm or substorm physics is beyond the scope of this book, we discuss in this chapter how the magnetospheric activity is related to the auroral phenomena. The basic ways how the magnetosphere controls auroral dynamics are: