名字 发表于 2025-3-23 11:53:10
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2- and 3-D Simulations of Magnetocentrifugal Disk-Winds: Acceleration and Stabilityct launching conditions on the disk, such as the distributions of magnetic flux and mass ejection rate, are poorly known. They could be constrained from observations at large distances, provided that a robust model is available to link the observable properties of the jets and winds at the large disFacet-Joints 发表于 2025-3-23 21:25:51
Hh 111 Stis Observations and Their Analysis Using Analytical and Numerical Modelsupersonic proper motions. These structures, we believe, are the result of a variable ejection from the source, which leads to the formation of . or small bowshock within the jet beam. In this paper we present a long-slit spectrum of Herbig-Haro object HH 111 obtained with STIS and an interpretationconceal 发表于 2025-3-24 01:35:06
http://reply.papertrans.cn/51/5009/500886/500886_14.pngBravura 发表于 2025-3-24 02:36:25
Three-Dimensional Simulations of Jets From Keplerian Disks: Stability Issues. We investigate the outflow that arises from a magnetized accretion disk that is initially in hydrostatic balance with its surrounding cold corona. Our simulations show that jets maintain their long-term stability through a self-limiting process wherein the average Alfvénic Mach number within the jalabaster 发表于 2025-3-24 07:04:50
Mhd Simulations of Jets From Accretion Disksly. Although it was considered that this kind of simulations only shows the transient phenomena of jets, we found that the outflow and accretion flow reached a quasi-steady state by performing a long-term calculation in a large calculation region. Though the final stage is not exactly the steady staVOC 发表于 2025-3-24 10:47:22
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