表示向下 发表于 2025-3-23 10:18:00

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推崇 发表于 2025-3-23 17:57:01

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CHANT 发表于 2025-3-23 20:49:31

Planetary Dynamos,these cosmic bodies. Similar processes are believed to produce a wide variety of other cosmic magnetic fields, including the fields of the Sun and stars. At present, we understand the basic physical processes involved in dynamo magnetic field generation. However, a detailed understanding still elude

glomeruli 发表于 2025-3-23 22:15:41

Boundary Determinations from Low Frequency Magnetic Field Measurements, a shock wave forms upstream of the object and the solar wind field is distorted and draped over the obstacle. For magnetic bodies, this interaction produces three distinct regions of space: the solar wind, the magnetosphere of the body, and the magnetosheath or shocked solar wind between the solar

Antimicrobial 发表于 2025-3-24 02:40:24

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催眠药 发表于 2025-3-24 10:26:48

Thermal History of Planetary Materials in the Solar Nebula,volution of the solar nebula. Particularly, this stage regulated the abundance and composition of volatiles absorbed by planetesimals and incorporated into planets, and the composition and texture of the primitive meteorites — chondrites.

Commentary 发表于 2025-3-24 13:59:52

Giant Planet Formation,anets are formed through quasi-static contraction of massive envelopes. On the other hand, Wuchterl (1991) obtained the results that giant planets should undergo a dynamical phase and cannot have massive envelopes like the present Jupiter and Saturn because dynamical oscillation would eject envelope mass.

folliculitis 发表于 2025-3-24 15:36:45

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决定性 发表于 2025-3-24 19:59:10

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defeatist 发表于 2025-3-25 01:07:03

Jiulong Ma,Xiaogang Qi,Lifang Liuanets are formed through quasi-static contraction of massive envelopes. On the other hand, Wuchterl (1991) obtained the results that giant planets should undergo a dynamical phase and cannot have massive envelopes like the present Jupiter and Saturn because dynamical oscillation would eject envelope mass.
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查看完整版本: Titlebook: Comparative Planetology with an Earth Perspective; Proceedings of the F Moustafa T. Chahine,Michael F. A’Hearn,Neil L. Nic Conference proce