標(biāo)題: Titlebook: Comparative Aeronomy; Andrew F. Nagy,André Balogh,Ingo Mueller-Wodarg Book 2008 Springer-Verlag New York 2008 Aeronomy.Ionosphere.Meteorol [打印本頁] 作者: CHAFF 時(shí)間: 2025-3-21 17:26
書目名稱Comparative Aeronomy影響因子(影響力)
書目名稱Comparative Aeronomy影響因子(影響力)學(xué)科排名
書目名稱Comparative Aeronomy網(wǎng)絡(luò)公開度
書目名稱Comparative Aeronomy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Comparative Aeronomy被引頻次
書目名稱Comparative Aeronomy被引頻次學(xué)科排名
書目名稱Comparative Aeronomy年度引用
書目名稱Comparative Aeronomy年度引用學(xué)科排名
書目名稱Comparative Aeronomy讀者反饋
書目名稱Comparative Aeronomy讀者反饋學(xué)科排名
作者: 光亮 時(shí)間: 2025-3-21 20:52
Neutral Upper Atmosphere and Ionosphere Modeling,environments. These tools are commonly used to predict upper atmosphere and ionosphere characteristics and to interpret measurements once they are obtained. Additional applications of these tools include conducting diagnostic balance studies, converting raw measurements into useful physical paramete作者: 兵團(tuán) 時(shí)間: 2025-3-22 03:31
Modeling and Simulating Flowing Plasmas and Related Phenomena,anets, moons and comets. The three popular simulation approaches to studying these interactions are presented. Each approach provides valuable insight to these interactions. To date no one approach is capable of simulating the whole interaction region from the collisionless to the collisional regime作者: 6Applepolish 時(shí)間: 2025-3-22 07:39 作者: 字的誤用 時(shí)間: 2025-3-22 10:16 作者: Comedienne 時(shí)間: 2025-3-22 16:49
,Plasma Flow and Related Phenomena in?Planetary?Aeronomy,The features of the interaction can be very different, depending upon the properties of the incident plasma as well as the nature of the obstacle. The properties of the atmosphere/ionosphere associated with the obstacle are of particular importance into understanding the plasma interaction process, 作者: Comedienne 時(shí)間: 2025-3-22 19:31
Atmospheric Escape and Evolution of Terrestrial Planets and Satellites,ge-Main-Sequence. We show that the high EUV flux of the young Sun, depending on the thermospheric composition, the amount of IR-coolers and the mass and size of the planet, could have been responsible that hydrostatic equilibrium was not always maintained and hydrodynamic flow and expansion of the u作者: Misgiving 時(shí)間: 2025-3-23 00:17 作者: LINE 時(shí)間: 2025-3-23 02:20
Book 2008sed to signify the study of the atmosphere in general, it should be adopted with the restricted sense of the science of the upper atmosphere, for which there is no convenient short word. ” In a chapter, he wrote in a 1960 book (Chapman 1960), he give his nal and de nitive de nition, by stating that 作者: 富足女人 時(shí)間: 2025-3-23 06:24 作者: paradigm 時(shí)間: 2025-3-23 11:23
https://doi.org/10.1007/978-3-658-03010-0well as advances in theoretical modeling capabilities. Key gaps in our understanding are highlighted which ultimately call for a more comprehensive programme of observation and laboratory measurements.作者: 施加 時(shí)間: 2025-3-23 15:02
Energy Deposition in Planetary Atmospheres by Charged Particles and Solar Photons, regions. They originate outside the atmosphere and are more energetic than photoelectrons, especially at magnetized planets. The spectroscopic analysis of auroral emissions is discussed here, along with its relevance to precipitating particle diagnostics. Atmospheres can also be modified by the ene作者: Dissonance 時(shí)間: 2025-3-23 21:40
Neutral Atmospheres,well as advances in theoretical modeling capabilities. Key gaps in our understanding are highlighted which ultimately call for a more comprehensive programme of observation and laboratory measurements.作者: Lipoprotein(A) 時(shí)間: 2025-3-23 23:20 作者: Detoxification 時(shí)間: 2025-3-24 02:43
https://doi.org/10.1007/978-3-658-03010-0ecial consideration is given to the implicit assumptions underlying each model. Some of the more common numerical methods used to implement each model, the implications of these numerical methods and the resulting limitations of each simulation approach are also discussed.作者: Gratuitous 時(shí)間: 2025-3-24 09:04 作者: ACRID 時(shí)間: 2025-3-24 13:32
https://doi.org/10.1007/978-3-658-03010-0especially for non-magnetized obstacle. This paper discusses in detail the roles of the atmosphere and ionosphere systems of plasma interaction around Venus, Mars, comets and some particular satellites. The coupling between magnetosphere and ionosphere is also discussed for Earth and Giant planets.作者: multiply 時(shí)間: 2025-3-24 18:41 作者: Boycott 時(shí)間: 2025-3-24 19:34 作者: Exposition 時(shí)間: 2025-3-25 02:09
,Plasma Flow and Related Phenomena in?Planetary?Aeronomy,especially for non-magnetized obstacle. This paper discusses in detail the roles of the atmosphere and ionosphere systems of plasma interaction around Venus, Mars, comets and some particular satellites. The coupling between magnetosphere and ionosphere is also discussed for Earth and Giant planets.作者: gregarious 時(shí)間: 2025-3-25 06:56 作者: AGGER 時(shí)間: 2025-3-25 08:30 作者: Condyle 時(shí)間: 2025-3-25 12:17
Book 2008ness Media B. V. 2008 Keywords Aeronomy The term “aeronomy” has been used widely for many decades, but its origin has mostly been lost over the years. It was introduced by Sydney Chapman in a Letter to the Editor, entitled “Some Thoughts on Nomenclature”, in Nature in 1946 (Chapman 1946). In that le作者: 刪減 時(shí)間: 2025-3-25 16:33
1385-7525 blished in the journal Space Science Reviews, Volume 139, Nos 1–4. DOI: 10. 1007/s11214-008-9353-0 ? Springer Science+Business Media B. V. 2008 Keywords Aeronomy The term “aeronomy” has been used widely for many decades, but its origin has mostly been lost over the years. It was introduced by Sydney作者: 小爭(zhēng)吵 時(shí)間: 2025-3-25 21:23 作者: 責(zé)問 時(shí)間: 2025-3-26 00:48
Neutral Upper Atmosphere and Ionosphere Modeling,ere numerical modeling tools, the equations solved and key assumptions made, specified inputs and tunable parameters, their common applications, and finally their notable strengths and weaknesses. Examples of these model classes and their specific applications to individual planetary environments will be described.作者: accessory 時(shí)間: 2025-3-26 05:03
Andrew F. Nagy,André Balogh,Ingo Mueller-WodargCovers all aspects of solar system aeronomy.Presents the observations and findings of many recent space missions作者: 會(huì)犯錯(cuò)誤 時(shí)間: 2025-3-26 10:12 作者: 駕駛 時(shí)間: 2025-3-26 12:39
https://doi.org/10.1007/978-3-658-03010-0s that they produce may interact with thermospheric neutral species producing dissociation, ionization, excitation, and heating. The interaction of X-rays or keV electrons with atmospheric neutrals may produce core-ionized species, which may decay by the production of characteristic X-rays or Auger 作者: indecipherable 時(shí)間: 2025-3-26 19:29
https://doi.org/10.1007/978-3-658-03010-0environments. These tools are commonly used to predict upper atmosphere and ionosphere characteristics and to interpret measurements once they are obtained. Additional applications of these tools include conducting diagnostic balance studies, converting raw measurements into useful physical paramete作者: Schlemms-Canal 時(shí)間: 2025-3-27 00:01
https://doi.org/10.1007/978-3-658-03010-0anets, moons and comets. The three popular simulation approaches to studying these interactions are presented. Each approach provides valuable insight to these interactions. To date no one approach is capable of simulating the whole interaction region from the collisionless to the collisional regime作者: MUT 時(shí)間: 2025-3-27 04:19 作者: magnate 時(shí)間: 2025-3-27 06:30
https://doi.org/10.1007/978-3-658-03010-0range, from X-rays to radio waves. In this chapter, we present current information in various categories—measurements of the airglows of the terrestrial planets, the dayglows of the outer planets and satellites, aurora throughout the solar system, observations of cometary spectra, and the emission o作者: 上坡 時(shí)間: 2025-3-27 09:36
https://doi.org/10.1007/978-3-658-03010-0The features of the interaction can be very different, depending upon the properties of the incident plasma as well as the nature of the obstacle. The properties of the atmosphere/ionosphere associated with the obstacle are of particular importance into understanding the plasma interaction process, 作者: indubitable 時(shí)間: 2025-3-27 16:16 作者: Aprope 時(shí)間: 2025-3-27 20:26
https://doi.org/10.1007/978-3-322-97034-3emperatures can be tens of thousands of kelvins, causing thermal dissociation of H. to H. The stellar ionizing flux converts H to H.. The high temperatures also drive large escape rates of H, but for all but the planets with the smallest orbits, this flux is not large enough to affect planet evoluti作者: 不法行為 時(shí)間: 2025-3-27 22:19
Photoemission Phenomena in the Solar System,range, from X-rays to radio waves. In this chapter, we present current information in various categories—measurements of the airglows of the terrestrial planets, the dayglows of the outer planets and satellites, aurora throughout the solar system, observations of cometary spectra, and the emission of X-rays from a variety of planetary bodies.作者: GLADE 時(shí)間: 2025-3-28 04:05 作者: 個(gè)人長(zhǎng)篇演說 時(shí)間: 2025-3-28 07:46
https://doi.org/10.1007/978-3-658-03010-0This article reviews our understanding of the ionospheres in the solar system. It provides some basic information on the sources and sinks of the ionospheric plasma, its dynamics, the energetics and the coupling to the neutral atmosphere. Ionospheres in the solar system are reviewed and comparative ionospheric topics are discussed.作者: archetype 時(shí)間: 2025-3-28 13:58
https://doi.org/10.1007/978-3-322-97034-3Aeronomy is a description of the physics and chemistry of the upper atmospheres and ionospheres of planetary bodies. In this chapter we consider those processes occurring in the upper atmosphere that determine the structure of the corona and lead to molecular escape.作者: 流逝 時(shí)間: 2025-3-28 16:06
Cross Sections and Reaction Rates for Comparative Planetary Aeronomy,In this chapter we describe the current knowledge of a selection of collision processes and chemical reactions of importance to planetary aeronomy. Emphasis is placed on critical evaluation of what we know and what we wish we knew about fundamental processes required for interpretation, explanation, and modeling of atmospheric observations.作者: GONG 時(shí)間: 2025-3-28 21:13
Solar System Ionospheres,This article reviews our understanding of the ionospheres in the solar system. It provides some basic information on the sources and sinks of the ionospheric plasma, its dynamics, the energetics and the coupling to the neutral atmosphere. Ionospheres in the solar system are reviewed and comparative ionospheric topics are discussed.作者: Indict 時(shí)間: 2025-3-28 23:23 作者: 女歌星 時(shí)間: 2025-3-29 05:54 作者: exhibit 時(shí)間: 2025-3-29 09:47
