笨拙处理
发表于 2025-3-23 12:28:30
Artur Akhmetov,Anna Burova,Natalia Makhankova,Alexey Ponomarenko nearby late-type stars. Both numbers refer to the ISM within about 100 pc of the Sun, which samples warm clouds located within the Local Bubble. Outside of the Local Bubble at distances of 200 to 500 pc, analyses of far-UV spectra obtained with the IMAPS instrument indicate a much wider range of D/
浪荡子
发表于 2025-3-23 17:39:00
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愚笨
发表于 2025-3-23 19:56:37
Elizaveta Markovskaya,Elena Smolina nearby late-type stars. Both numbers refer to the ISM within about 100 pc of the Sun, which samples warm clouds located within the Local Bubble. Outside of the Local Bubble at distances of 200 to 500 pc, analyses of far-UV spectra obtained with the IMAPS instrument indicate a much wider range of D/
ALLEY
发表于 2025-3-23 22:19:57
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易于出错
发表于 2025-3-24 05:15:54
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没收
发表于 2025-3-24 09:55:03
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似少年
发表于 2025-3-24 14:45:50
Sergey Dubinin plasma parameters may well be quite different in the Sun‘s atmosphere, a cometary tailor Jupiter‘s magnetosphere, but many of the basic processes are similar and it is by studying them in different environments that we come to understand them more deeply. Furthermore, direct in situ measurements of plasma pr978-90-277-2138-9978-94-009-5482-3
策略
发表于 2025-3-24 15:04:50
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陈旧
发表于 2025-3-24 19:29:00
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Mendacious
发表于 2025-3-24 23:40:15
Konstantin Krinichanskyf dynamical stability, comets and meteors, meteorites and asteroids, and concludes with an extensive discussion of extrasolar planets. ..The contents of .Solar System Astrophysics: A Text for the Science of Pla978-0-387-73155-1Series ISSN 0941-7834 Series E-ISSN 2196-9698