租期
发表于 2025-3-21 17:27:50
书目名称Auroral Plasma Physics影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0165587<br><br> <br><br>书目名称Auroral Plasma Physics读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0165587<br><br> <br><br>
吞下
发表于 2025-3-22 00:15:19
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
发表于 2025-3-22 04:10:09
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.
左右连贯
发表于 2025-3-22 08:33:37
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
发表于 2025-3-22 09:51:50
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cardiac-arrest
发表于 2025-3-22 16:09:04
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insipid
发表于 2025-3-22 20:29:40
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.
圆锥体
发表于 2025-3-22 23:27:10
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.
热烈的欢迎
发表于 2025-3-23 04:34:56
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Antecedent
发表于 2025-3-23 07:51:29
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: