raff淫雨霏霏
发表于 2025-3-21 19:27:23
书目名称Accretion Disks and Magnetic Fields in Astrophysics影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0143795<br><br> <br><br>书目名称Accretion Disks and Magnetic Fields in Astrophysics读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0143795<br><br> <br><br>
precede
发表于 2025-3-21 22:06:44
The Radiologic Evaluation of Renal Massesield dynamo models. Nonlinear solutions provide examples of chaotic time-dependent behaviour and illustrate the development of complicated spatial structure. However, it is difficult to extrapolate from slow rotators like the Sun to rapidly rotating, highly active stars.
喃喃诉苦
发表于 2025-3-22 00:54:07
S. Trattnig,P. Hübsch,F. Frühwaldain sequence star. These binary systems are very common, well documented by observations in the optical wavelength region since a long time. These objects are therefore particularly well suited to study properties of accretion disks.
AMITY
发表于 2025-3-22 07:54:42
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调整
发表于 2025-3-22 12:28:05
https://doi.org/10.1007/978-3-319-17539-3g profile. Our results are compared to standard theoretical and numerical models. We find that the stream of cold gas falling on the compact star forms the disk in the conventional way, a strong shock develops and penetrates deep into the disk. However, since our numerical viscosity is still high we cannot establish if spiral shocks are forming.
使成核
发表于 2025-3-22 15:14:28
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可以任性
发表于 2025-3-22 17:31:57
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bromide
发表于 2025-3-22 23:46:07
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Magnificent
发表于 2025-3-23 03:47:50
G. Stuart Rutherfoord,R. H. Hewlettby introducing a magnetodynamic picture which is related to the sweeping-magnetic-twist mechanism proposed by Uchida and Shibata (1985) for the production of molecular bipolar flows from forming stars.
初学者
发表于 2025-3-23 08:22:07
https://doi.org/10.1007/978-3-211-99763-5n especially attractive in protostellar, neutron star and AGN disks, where the traditional ‘angular momentum problem’ is most severe. It is shown that spiral shocks are also good locations for producing energetic protons, and I propose that this is the way in which the energetic particles inferred in many AGN’s are produced.