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发表于 2025-3-21 16:53:34
书目名称Astrophysical and Laboratory Plasmas影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0163686<br><br> <br><br>书目名称Astrophysical and Laboratory Plasmas读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0163686<br><br> <br><br>
regale
发表于 2025-3-21 22:47:04
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Blanch
发表于 2025-3-22 02:25:53
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adhesive
发表于 2025-3-22 07:10:22
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MIR
发表于 2025-3-22 12:10:53
Chemically Peculiar Hot Stars in chemically peculiar stars, with an emphasis on insights provided by a generation of ultraviolet observations obtained with the . satellite. The paper concludes with an overview of the radiative diffusion mechanism which has been proposed as an explanation of the chemically peculiar phenomenon.
音乐会
发表于 2025-3-22 14:28:08
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荣幸
发表于 2025-3-22 17:05:45
Particle Attraction and Gravity the highest levels of mass loss amongst early-type stars: mass loss rates, typically, lie in the range × 10...yr.. Radiation pressure—driven winds incorporating multi-scattering in high ionisation—stratified winds may cause these levels, but additional mechanisms may also be needed.
Infant
发表于 2025-3-23 00:55:26
Wolf—Rayet Stars the highest levels of mass loss amongst early-type stars: mass loss rates, typically, lie in the range × 10...yr.. Radiation pressure—driven winds incorporating multi-scattering in high ionisation—stratified winds may cause these levels, but additional mechanisms may also be needed.
体贴
发表于 2025-3-23 05:08:01
Foundation Actionscript 3.0 Animationcorona implies a fundamental role for the magnetic field in coronal structuring and dynamics. Variability of the corona occurs on all temporal and spatial scales — at one extreme, as the result of plasma instabilities, and at the other extreme driven by the global magnetic flux emergence patterns of the solar cycle.
Congestion
发表于 2025-3-23 07:28:37
Foundation Actionscript 3.0 Animationpower them, and the accretion processes which convert this into electromagnetic radiation. Particular attention is paid to the topics of mass transfer fluctuations and of the accretion by magnetic compact stars.