prick-test 发表于 2025-3-26 23:08:21

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vitreous-humor 发表于 2025-3-27 02:57:10

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愤怒事实 发表于 2025-3-27 05:57:21

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讲个故事逗他 发表于 2025-3-27 10:52:55

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.

Phonophobia 发表于 2025-3-27 16:05:36

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.

genesis 发表于 2025-3-27 18:57:13

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.

Integrate 发表于 2025-3-27 22:32:11

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Angioplasty 发表于 2025-3-28 04:26:17

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.

MOCK 发表于 2025-3-28 08:59:55

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construct 发表于 2025-3-28 14:26:41

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查看完整版本: Titlebook: Giant Planets of Our Solar System; Atmospheres, Composi Patrick G. J. Irwin Book 2009Latest edition Springer-Verlag Berlin Heidelberg 2009