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径向束射功率四极管4CX15000/8281
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作者 李应凤 《旭光技术》 1994年第1期28-36,共9页
关键词 功率四极管 4CX1500A/8281 径向束射 结构
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Radial explosion strain and its fracture effect from confined explosion with charge of cyclonite 被引量:2
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作者 徐国元 段乐珍 +1 位作者 古德生 闫长斌 《Journal of Central South University of Technology》 EI 2004年第4期429-433,共5页
Instrumented experiments were conducted in concrete models to study the explosion-induced radial strain and fracture effect of rock-like media under confined explosion with a charge of cyclonite. As a charge was explo... Instrumented experiments were conducted in concrete models to study the explosion-induced radial strain and fracture effect of rock-like media under confined explosion with a charge of cyclonite. As a charge was exploded, two different radial strain waves were sequentially recorded by a strain gage at a distance of 80 mm from the center of charge. Through the attenuation formula of the maximum compressive strain(εrmax), the distribution of εrmax and its strain rate( ) between the charge and gage were obtained. The effect of the two waves propagating outwards on the radial fracture of surrounding media was discussed. The results show that the two waves are pertinent to the loading of shock energy (Es) and bubble energy (Eb) against concrete surrounding charge, respectively. The former wave lasts for much shorter time than the latter. The peak values of εrmax and of the former are higher than those of the latter, respectively. 展开更多
关键词 confined explosion loading radial strain radial fracture CONCRETE shock energy bubble energy
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Constraints on Non-Radial Oscillation Modes by Symmetry Energy Slope 被引量:1
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作者 周颖 文德华 《Communications in Theoretical Physics》 SCIE CAS CSCD 2014年第4期469-474,共6页
The effect of the nuclear symmetry energy slope on the non-radial oscillation f-modes in neutron stars is calculated and discussed. Based on a conservative range of the symmetry energy slope constrained by the experim... The effect of the nuclear symmetry energy slope on the non-radial oscillation f-modes in neutron stars is calculated and discussed. Based on a conservative range of the symmetry energy slope constrained by the experiment and theoretical analysis, a constraint on the frequency and damping time of the gravitational radiation from the f-mode in neutron star is obtained. It is also shown that a higher symmetry energy slope corresponds with a smaller frequency and a longer damping time. Meanwhile, a new set of parameters is given to present the universal properties of the scaled frequency and damping time. 展开更多
关键词 neutron star symmetry energy oscillation modes
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