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標(biāo)題: Titlebook: Atmospheric and Space Sciences: Ionospheres and Plasma Environments; Volume 2 Erdal Yi?it Book 2018 The Author(s) 2018 Atmospheric dynamics [打印本頁(yè)]

作者: Pessimistic    時(shí)間: 2025-3-21 16:43
書(shū)目名稱(chēng)Atmospheric and Space Sciences: Ionospheres and Plasma Environments影響因子(影響力)




書(shū)目名稱(chēng)Atmospheric and Space Sciences: Ionospheres and Plasma Environments影響因子(影響力)學(xué)科排名




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書(shū)目名稱(chēng)Atmospheric and Space Sciences: Ionospheres and Plasma Environments網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱(chēng)Atmospheric and Space Sciences: Ionospheres and Plasma Environments被引頻次




書(shū)目名稱(chēng)Atmospheric and Space Sciences: Ionospheres and Plasma Environments被引頻次學(xué)科排名




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作者: Urologist    時(shí)間: 2025-3-21 23:37

作者: 文藝    時(shí)間: 2025-3-22 01:14
Book 2018research) students and young researchers that would like to gain quick insight into the basics of space sciences and current research. In combination?with the first volume, it also is a useful tool for professors who would like to develop a course in atmospheric and space physics.
作者: 諄諄教誨    時(shí)間: 2025-3-22 05:06

作者: Glycogen    時(shí)間: 2025-3-22 09:24
K. K. Loewit,H.-G. Kraft,A. Ortliebelecromagnetic spectrum is composed of a broad range of wavelengths from low-frequency radio waves (.10?MHz) to very high-frequency gamma rays (.10.?Hz). Finally the concept of phase space and collisions between particles of different species are discussed.
作者: 消息靈通    時(shí)間: 2025-3-22 13:10

作者: 分離    時(shí)間: 2025-3-22 18:22
Transport Processes in Plasma,r a given condition of ambient field. It is an important factor for the energetics of the ionospheric plasma and its coupling to the neutrals. The approach of magnetohydrodynamics (MHD) combines plasma physics with the fluid approximation. While most fluid models for the neutrals prescribe electric
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作者: 樂(lè)器演奏者    時(shí)間: 2025-3-23 06:56

作者: cravat    時(shí)間: 2025-3-23 11:17
Atmospheric and Space Sciences: Ionospheres and Plasma EnvironmentsVolume 2
作者: 周年紀(jì)念日    時(shí)間: 2025-3-23 17:20
2191-5369 ences and current research. In combination?with the first volume, it also is a useful tool for professors who would like to develop a course in atmospheric and space physics.978-3-319-62005-3978-3-319-62006-0Series ISSN 2191-5369 Series E-ISSN 2191-5377
作者: cancellous-bone    時(shí)間: 2025-3-23 21:41

作者: ADORN    時(shí)間: 2025-3-23 23:25
B. Beri?,S. Aleksi?,M. Marjanovi?,F. Krancr a given condition of ambient field. It is an important factor for the energetics of the ionospheric plasma and its coupling to the neutrals. The approach of magnetohydrodynamics (MHD) combines plasma physics with the fluid approximation. While most fluid models for the neutrals prescribe electric
作者: 得意牛    時(shí)間: 2025-3-24 04:09
New aspects in post-coital contraception,cannot be neglected. A Chapman layer is a first order approximation of production of ionization by the absorption of solar energy, which is a good description for the lower ionosphere (. regions), but higher up in the . region transport becomes important. Qualitatively, Earth’s and Mars ionospheres
作者: 結(jié)果    時(shí)間: 2025-3-24 07:12
Human Ovarian Follicular Antigens,n appreciable role for the energy and momentum budget of the thermosphere, while planetary waves modulate lower thermospheric variability over long time scales. During geomagnetic storms, which are a prominent manifestation of space weather, the thermosphere and ionosphere undergo substantial dynami
作者: 辯論的終結(jié)    時(shí)間: 2025-3-24 14:28

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作者: 抗生素    時(shí)間: 2025-3-24 20:15

作者: 手銬    時(shí)間: 2025-3-25 02:51
Planetary Ionospheres, whose dynamics produces complex current systems, depending on ambient electric fields, and collisional properties, and gyration around magnetic fields. In terms of the vertical extent, the ionosphere coincides with the thermosphere, where the neutral species are diffusively separated, owing to stro
作者: 彎彎曲曲    時(shí)間: 2025-3-25 04:02
Dynamics of the Atmosphere-Ionosphere System,ma densities. The upper atmosphere and ionosphere continuously interact with each other in a two-way nonlinear manner. It is therefore increasingly common to refer to them as the atmosphere-ionosphere system. Overall, the state and evolution of the atmotsphere-ionosphere system is influenced by mete
作者: Grating    時(shí)間: 2025-3-25 08:38
https://doi.org/10.1007/978-3-319-62006-0Atmospheric dynamics; Atmospheric and ionospheric science; Fluid dynamics and atmospheric and space sc
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SpringerBriefs in Earth Scienceshttp://image.papertrans.cn/b/image/164660.jpg
作者: 尾巴    時(shí)間: 2025-3-26 03:24
L. G. Keith,R. Bailey,G. S. Bergerervable universe consists of plasma. Closer to Earth, i.e., in the solar-terrestrial environment, the solar wind, the magnetosphere, and the ionosphere are the most studied plasma environments. Plasma processes are greatly influenced by ambient electromagnetic fields and, in analogy with neutral pla
作者: 一再煩擾    時(shí)間: 2025-3-26 06:24
K. K. Loewit,H.-G. Kraft,A. Ortlieb, magnetic fields, and Maxwell equations, which self-consistently relate these fields to each other, are introduced. Charged particles are sources of electric fields and moving charged particles can generate magnetic fields. The most obvious manifestation of electromagnetic fields is the light. The
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作者: 惡名聲    時(shí)間: 2025-3-26 14:33

作者: Cuisine    時(shí)間: 2025-3-26 20:04
Human Ovarian Follicular Antigens,ma densities. The upper atmosphere and ionosphere continuously interact with each other in a two-way nonlinear manner. It is therefore increasingly common to refer to them as the atmosphere-ionosphere system. Overall, the state and evolution of the atmotsphere-ionosphere system is influenced by mete
作者: osculate    時(shí)間: 2025-3-27 00:52
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