颂扬本人
发表于 2025-3-25 04:21:39
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Silent-Ischemia
发表于 2025-3-25 08:48:26
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
vasospasm
发表于 2025-3-25 11:43:28
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
小丑
发表于 2025-3-25 18:53:15
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.
Flatter
发表于 2025-3-25 23:39:17
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
hereditary
发表于 2025-3-26 00:19:22
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
泄露
发表于 2025-3-26 05:49:36
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.
Cupidity
发表于 2025-3-26 09:35:36
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IRATE
发表于 2025-3-26 13:22:18
https://doi.org/10.1007/978-3-540-85158-5AAS; AGU; Cloud; DPS; EGU; giant planets; planetary atmospheres; solar system; temperature
情爱
发表于 2025-3-26 18:30:32
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