Titlebook: Accretion Disks and Magnetic Fields in Astrophysics; Proceedings of the E G. Belvedere Conference proceedings 1989 Springer Science+Busines

raff淫雨霏霏

书目名称Accretion Disks and Magnetic Fields in Astrophysics影响因子(影响力)




书目名称Accretion Disks and Magnetic Fields in Astrophysics影响因子(影响力)学科排名




书目名称Accretion Disks and Magnetic Fields in Astrophysics网络公开度




书目名称Accretion Disks and Magnetic Fields in Astrophysics网络公开度学科排名




书目名称Accretion Disks and Magnetic Fields in Astrophysics被引频次




书目名称Accretion Disks and Magnetic Fields in Astrophysics被引频次学科排名




书目名称Accretion Disks and Magnetic Fields in Astrophysics年度引用




书目名称Accretion Disks and Magnetic Fields in Astrophysics年度引用学科排名




书目名称Accretion Disks and Magnetic Fields in Astrophysics读者反馈




书目名称Accretion Disks and Magnetic Fields in Astrophysics读者反馈学科排名

precede

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

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

调整

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

可以任性

bromide

Magnificent

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

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.