Titlebook: Seminar on Concurrency; Carnegie-Mellon Univ Stephen D. Brookes,Andrew William Roscoe,Glynn Win Conference proceedings 1985 Springer-Verlag

Dopamine

书目名称Seminar on Concurrency影响因子(影响力)




书目名称Seminar on Concurrency影响因子(影响力)学科排名




书目名称Seminar on Concurrency网络公开度




书目名称Seminar on Concurrency网络公开度学科排名




书目名称Seminar on Concurrency被引频次




书目名称Seminar on Concurrency被引频次学科排名




书目名称Seminar on Concurrency年度引用




书目名称Seminar on Concurrency年度引用学科排名




书目名称Seminar on Concurrency读者反馈




书目名称Seminar on Concurrency读者反馈学科排名

新星

草本植物

GLOOM

Glynn Winskelccurred within the domains of astronomical observations, astrophysical modeling and numerical simulations, but the recent advent of high energy density facilities has added experimental control to jet studies...Front-line research on jet launching and collimation requires a highly interdisciplinary

易于

J. A. Bergstra,J. W. Klop,J. V. Tucker in the introduction, this reflects very much the quite different mode of energy transport in the two classes of source. Another parameter which also highlights the differences between the two types of jet is the velocity. This can be written in the form: .. = 430 km s...... (./..)...For class I jet

抛射物

J. Misraspeed, density, magnetic fields, collimation) must be related in a way to the properties of the very central object and its accretion disk. Early models of jet formation were based on pure hydrodynamic acceleration in the funnels of geometrically thick tori. For sub-Eddington luminosities such flows

不溶解

Ben Moszkowskispeed, density, magnetic fields, collimation) must be related in a way to the properties of the very central object and its accretion disk. Early models of jet formation were based on pure hydrodynamic acceleration in the funnels of geometrically thick tori. For sub-Eddington luminosities such flows

Costume

Christian Lengauer,Chua-Huang Huang in the introduction, this reflects very much the quite different mode of energy transport in the two classes of source. Another parameter which also highlights the differences between the two types of jet is the velocity. This can be written in the form: .. = 430 km s...... (./..)...For class I jet

Endemic

Gul Aghans. The simulations follow several 1000 Keplerian periods of the inner disk (for animated movies see http : / /www. aip. de/∼cf endt). Our model prescribes a Keplerian disk around a rotating star as a fixed boundary condition. The initial magnetic field distribution remains frozen into the star and

hypnotic

Vaughan Prattns. The simulations follow several 1000 Keplerian periods of the inner disk (for animated movies see http : / /www. aip. de/∼cf endt). Our model prescribes a Keplerian disk around a rotating star as a fixed boundary condition. The initial magnetic field distribution remains frozen into the star and