TERRA 发表于 2025-3-25 04:43:13
Numerical Studies of Fluid Flow in Microgravity Conditions for Confined Crystal Growth,rystal growth experiments. We consider both constant and oscillating acceleration and focus mostly on the transient relaxation dynamics. Results are relevant to estimate impact of more realistic residual accelerations in crystal growth experiments.muscle-fibers 发表于 2025-3-25 08:43:47
http://reply.papertrans.cn/87/8627/862612/862612_22.png放肆的你 发表于 2025-3-25 13:58:25
http://reply.papertrans.cn/87/8627/862612/862612_23.pngDistribution 发表于 2025-3-25 19:24:59
Modeling the Local Interstellar Medium,oud, surrounding the solar system to the boundary of the Local Bubble, which is a region of distinct anticorrelation between HI (.. < 10. cm.) and 1/4 keV diffuse soft X-rays. After discussing some key observations in soft X-rays, obtained by ROSAT and DXS, and in the EUV by the EUVE satellite and tPicks-Disease 发表于 2025-3-25 21:57:13
EURD Observations of Interstellar Radiation,fter decades of study, the processes that cool the hot interstellar medium remain obscure. The EURD spectrograph was designed to measure the diffuse cosmic background from 350 to 1100 Å in order to study the hot ISM and the mechanisms by which it sheds its energy. We present the first analysis of EUObloquy 发表于 2025-3-26 03:25:51
The Local Interstellar Medium in the Direction of the Galactic Anticentre,ive the spatial distribution of the nearby interstellar gas in the Galactic anticentre hemisphere. The data show the presence, within the region explored and within the nearest 150 pc, of eight diffuse interstellar clouds with LSR velocities in the range 15–55 km s.. Molecular gas previously identif间接 发表于 2025-3-26 07:30:48
http://reply.papertrans.cn/87/8627/862612/862612_27.png袖章 发表于 2025-3-26 10:06:15
http://reply.papertrans.cn/87/8627/862612/862612_28.pngNonporous 发表于 2025-3-26 14:37:14
http://reply.papertrans.cn/87/8627/862612/862612_29.pngComprise 发表于 2025-3-26 17:39:13
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