变成小松鼠
发表于 2025-3-21 18:29:18
书目名称Magnetic Fields and Star Formation影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0621226<br><br> <br><br>书目名称Magnetic Fields and Star Formation读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0621226<br><br> <br><br>
entrance
发表于 2025-3-21 23:14:42
Turbulence in the Star-Forming Interstellar Medium: Steps Toward Constraining Theories with Observat a rapid pace, aided in part by numerical simulations. These increased capabilities on both fronts open new opportunities for strengthening the links between observation and theory, and for meaningful comparisons between the two.
Trigger-Point
发表于 2025-3-22 04:15:03
The Tiny-Scale Atomic Structure: Gas Cloudlets or Scintillation Phenomenon ?ns of B0823+26 and B1133+16 are similar on scales of 10–20, 350 and 500 AU. The large number of non detections of the tiny scale atomic structure suggests that the AU-sized structure is not ubiquitous in the interstellar medium.
繁殖
发表于 2025-3-22 05:21:40
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insecticide
发表于 2025-3-22 12:09:30
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Axon895
发表于 2025-3-22 15:27:02
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Console
发表于 2025-3-22 19:08:45
Magnetic Flux Transport in the ISM through Turbulent Ambipolar Diffusionether turbulence can enhance the ambipolar diffusion rate sufficiently to explain the observed weak correlations. The numerical method is based on a gas-kinetic scheme with very low numerical diffusivity, thus allowing us to separate numerical and physical diffusion effects.
conjunctiva
发表于 2025-3-22 22:42:57
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讨好美人
发表于 2025-3-23 04:54:05
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注视
发表于 2025-3-23 09:10:18
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