標(biāo)題: Titlebook: Giant Planets of Our Solar System; Atmospheres, Composi Patrick G. J. Irwin Book 2009Latest edition Springer-Verlag Berlin Heidelberg 2009 [打印本頁] 作者: Colossal 時間: 2025-3-21 20:04
書目名稱Giant Planets of Our Solar System影響因子(影響力)
書目名稱Giant Planets of Our Solar System影響因子(影響力)學(xué)科排名
書目名稱Giant Planets of Our Solar System網(wǎng)絡(luò)公開度
書目名稱Giant Planets of Our Solar System網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Giant Planets of Our Solar System被引頻次
書目名稱Giant Planets of Our Solar System被引頻次學(xué)科排名
書目名稱Giant Planets of Our Solar System年度引用
書目名稱Giant Planets of Our Solar System年度引用學(xué)科排名
書目名稱Giant Planets of Our Solar System讀者反饋
書目名稱Giant Planets of Our Solar System讀者反饋學(xué)科排名
作者: 全國性 時間: 2025-3-21 22:51 作者: 亞當(dāng)心理陰影 時間: 2025-3-22 03:31 作者: carbohydrate 時間: 2025-3-22 06:27
Dynamical processes,erial are transported, not just vertically, but horizontally as well. In this chapter we will consider the basic equations of fluid motion in rotating planetary atmospheres and see how these theoretical considerations relate to the observed winds, clouds, and storm systems observed in the atmospheres of the giant planets.作者: 錯 時間: 2025-3-22 09:07
Book 2009Latest editionen extensively updated following the Cassini mission results for Jupiter/Saturn and the newest ground-based measurements for Uranus/Neptune as well as on the latest development in the theories on planet formation..作者: d-limonene 時間: 2025-3-22 16:04 作者: d-limonene 時間: 2025-3-22 17:05 作者: reperfusion 時間: 2025-3-22 23:10
Introduction,in Jean Joseph Le Verrier (1811–1877) to independently predict the presence of a further planet, and Neptune was subsequently discovered close to its predicted position by Johann Gottfried Galle (1812–1910) in 1846. The mean observable properties of the outer planets are listed in Table 1.1.作者: AWE 時間: 2025-3-23 02:55
Future of giant planet observations,ew measurements are expected in the next few years which will further improve our understanding of these giant worlds, and how they formed from circumplanetary disks. Some of the key questions concerning the atmospheres of the giant planets that still remain are作者: certain 時間: 2025-3-23 09:29
Book 2009Latest editionheories of their formation are reviewed and their recently observed temperature, composition and cloud structures are contrasted and compared with simple thermodynamic, radiative transfer and dynamical models. The instruments and techniques that have been used to remotely?measure their atmospheric p作者: AVOW 時間: 2025-3-23 09:44 作者: 憤世嫉俗者 時間: 2025-3-23 15:49
Radiative transfer processes in outer planetary atmospheres,rom specific flyby and orbiting spacecraft missions. There are two main components of the observed spectra that provide atmospheric information: reflected sunlight from the cloud and haze layers, and thermal emission from the atmosphere itself.作者: Resistance 時間: 2025-3-23 21:58 作者: Immobilize 時間: 2025-3-24 01:15
https://doi.org/10.1007/978-3-476-05388-6ng”. As the universe expanded and cooled, numerous particle physics processes and particle-antiparticle annihilations occurred (e.g., Krane, 1996). After about . = 6 s, the universe consisted of some number . protons, . electrons, 0.16. neutrons, 10.. photons, and 10.. neutrinos, all at a temperatur作者: 喊叫 時間: 2025-3-24 04:51 作者: 有其法作用 時間: 2025-3-24 10:24 作者: 細(xì)查 時間: 2025-3-24 12:11 作者: 玩笑 時間: 2025-3-24 18:30 作者: 導(dǎo)師 時間: 2025-3-24 21:53 作者: wall-stress 時間: 2025-3-25 01:02 作者: 頌揚(yáng)本人 時間: 2025-3-25 04:21 作者: Silent-Ischemia 時間: 2025-3-25 08:48
Formation of the giant planets,ng”. As the universe expanded and cooled, numerous particle physics processes and particle-antiparticle annihilations occurred (e.g., Krane, 1996). After about . = 6 s, the universe consisted of some number . protons, . electrons, 0.16. neutrons, 10.. photons, and 10.. neutrinos, all at a temperatur作者: vasospasm 時間: 2025-3-25 11:43
Evolution processes in outer planet atmospheres,er or lesser extent) evolved over time through the action of a number of possible processes including thermal escape, cometary bombardment, and internal differentiation. In this chapter we will outline the principal evolution mechanisms and estimate their effects on the present-day composition of th作者: 小丑 時間: 2025-3-25 18:53
Vertical structure of temperature, composition, and clouds,. Remote-sounding and . observations of the vertical profiles of pressure, temperature, and composition provide constraints on vertical motion, mixing, heat sources, deep composition, and photochemistry. These observations are complemented by observations of vertical cloud structure.作者: Flatter 時間: 2025-3-25 23:39
Dynamical processes,scussed transport mechanisms such as convection and eddy mixing. Of course the real atmospheres of planets are three-dimensional and thus to understand fully the observations of ground-based telescopes and spacecraft missions, we need to understand how planetary atmospheres move and how heat and mat作者: hereditary 時間: 2025-3-26 00:19
Radiative transfer processes in outer planetary atmospheres,are available were made from the . entry probe, which sampled a single, probably not very representative, region of the planet, namely a 5 μm hotspot. Hence, the bulk of our knowledge of the composition, cloud structure, and dynamics of these planets has not come from direct measurements, but instea作者: 泄露 時間: 2025-3-26 05:49
Sources of remotely sensed data on the giant planets,sorption features of different gases (and theoretically aerosols) are visible in these spectra. Clearly much can be learned about the atmospheres from observing the spectra of these planets, and in this chapter we will review the measurements that have been made to date and how they may be used.作者: Cupidity 時間: 2025-3-26 09:35 作者: IRATE 時間: 2025-3-26 13:22
https://doi.org/10.1007/978-3-540-85158-5AAS; AGU; Cloud; DPS; EGU; giant planets; planetary atmospheres; solar system; temperature作者: 情愛 時間: 2025-3-26 18:30 作者: prick-test 時間: 2025-3-26 23:08 作者: vitreous-humor 時間: 2025-3-27 02:57 作者: 憤怒事實(shí) 時間: 2025-3-27 05:57 作者: 講個故事逗他 時間: 2025-3-27 10:52
Wolfgang Strengmann-Kuhn,Richard Hauser. Remote-sounding and . observations of the vertical profiles of pressure, temperature, and composition provide constraints on vertical motion, mixing, heat sources, deep composition, and photochemistry. These observations are complemented by observations of vertical cloud structure.作者: Phonophobia 時間: 2025-3-27 16:05
Wolfgang Simler,Christine Riel-Sommersorption features of different gases (and theoretically aerosols) are visible in these spectra. Clearly much can be learned about the atmospheres from observing the spectra of these planets, and in this chapter we will review the measurements that have been made to date and how they may be used.作者: genesis 時間: 2025-3-27 18:57
Formation of the giant planets,ng”. As the universe expanded and cooled, numerous particle physics processes and particle-antiparticle annihilations occurred (e.g., Krane, 1996). After about . = 6 s, the universe consisted of some number . protons, . electrons, 0.16. neutrons, 10.. photons, and 10.. neutrinos, all at a temperature of approximately 10. K.作者: Integrate 時間: 2025-3-27 22:32 作者: Angioplasty 時間: 2025-3-28 04:26
Vertical structure of temperature, composition, and clouds,. Remote-sounding and . observations of the vertical profiles of pressure, temperature, and composition provide constraints on vertical motion, mixing, heat sources, deep composition, and photochemistry. These observations are complemented by observations of vertical cloud structure.作者: MOCK 時間: 2025-3-28 08:59 作者: construct 時間: 2025-3-28 14:26 作者: 間諜活動 時間: 2025-3-28 16:33
Alexander Rühr,Benedikt Berger,Thomas Hessund Figurationstheorie – angewendet. .Am Ende steht die Darstellung eines systemtheoretischen Modells zur Prozessanalyse und dessen Anwendung auf Merkmale und Auswirkungen der computer978-3-531-15630-9978-3-531-91842-6作者: LINES 時間: 2025-3-28 22:11 作者: iodides 時間: 2025-3-29 00:07 作者: 含沙射影 時間: 2025-3-29 03:37
