压倒
发表于 2025-3-23 12:40:10
http://reply.papertrans.cn/99/9833/983288/983288_11.png
替代品
发表于 2025-3-23 15:45:56
http://reply.papertrans.cn/99/9833/983288/983288_12.png
腼腆
发表于 2025-3-23 19:33:23
http://reply.papertrans.cn/99/9833/983288/983288_13.png
分期付款
发表于 2025-3-23 22:47:23
Interpreting the Observations of Herbig-Haro Jets observations of individual HH objects. The only models that have been developed to this point are the “internal working surface model” (in which the structures along HH jets are interpreted as working surfaces resulting from a time-variability in the ejection) or the “Kelvin-Helmholtz instability m
aspersion
发表于 2025-3-24 03:26:06
http://reply.papertrans.cn/99/9833/983288/983288_15.png
假装是我
发表于 2025-3-24 06:40:21
http://reply.papertrans.cn/99/9833/983288/983288_16.png
使激动
发表于 2025-3-24 10:46:40
http://reply.papertrans.cn/99/9833/983288/983288_17.png
Bouquet
发表于 2025-3-24 15:31:49
http://reply.papertrans.cn/99/9833/983288/983288_18.png
Confound
发表于 2025-3-24 20:22:04
http://reply.papertrans.cn/99/9833/983288/983288_19.png
GROSS
发表于 2025-3-24 23:19:07
Virtual Jets: From Self-Similar to Numerical Solutions like (1) to emphasize the huge difficulties one has to face when attempting to perform magnetohydrodynamic (MHD) numerical simulations of such discs; (2) to show how self-similar solutions can help to solve these difficulties. In particular, they allow to choose suitable boundary conditions and/or