维修性验证是装备维修性工作的重要组成部分,平均修复时间(mean time to repair,MTTR)是维修性定量要求验证的主要参数。本文从国内外装备MTTR验证标准和手册发展情况以及装备MTTR验证常用方法两个方面综述了MTTR验证方法的国内外研究...维修性验证是装备维修性工作的重要组成部分,平均修复时间(mean time to repair,MTTR)是维修性定量要求验证的主要参数。本文从国内外装备MTTR验证标准和手册发展情况以及装备MTTR验证常用方法两个方面综述了MTTR验证方法的国内外研究进展。介绍了美国国防部、国际电工委员会和国内相关机构颁布的MTTR验证标准和手册的发展情况,分析了标准和手册中的MTTR验证方法。总结归纳了装备MTTR验证的常用方法及应用情况,包括基于实物装备的验证方法和基于虚拟现实的验证方法。在此基础上概括了装备MTTR验证方法的研究特点,展望了未来的研究方向,并给出了研究建议。展开更多
In this paper, we consider the application of the equation of non-classical mathematical physics to magneto-hydrodynamic equilibrium (in the case of a mixed magnetic field) for magnetic stars. First, we give the neces...In this paper, we consider the application of the equation of non-classical mathematical physics to magneto-hydrodynamic equilibrium (in the case of a mixed magnetic field) for magnetic stars. First, we give the necessary concepts about the equation of non-classical mathematical physics and the possibility of their applicability to astrophysical problems. The conditions of magneto-hydrodynamic equilibrium are determinate, and self-consistence provides the means to derive the corresponding partial differential equations describing this equilibrium in a magnetosphere magnetic star. Namely, this process is to the non-classical equations of mathematical physics in cases of types. Keldysh-Tricomi, a common case equation of non-classical type, is at first introduced by the author. Using the two main physical efficiencies of MHD. A mathematical model of a poloidal-toroidal mixed magnetic field for magnetic stars is constructed, and this model is classified with respect to degenerating case equations. According to Hopf’s theorem, Maxwell’s equation and the magnetic force balance equation constructed equilibrium conditions of the poloidal-toroidal of the magnetic field for a magnetic star. At the same time, the taken example, which is the self-consistency of this model by observation dates, is investigated. At first, in an application, the method of straight lines for recurrent formulas of calculation of magnetic flux and stream functions is used. The physical means, the corresponding singular point of the sonic line, cutoff, and resonance phenomena are considered. In this case, a general solution equation is found, which is interpreted by this phenomenon as a cutoff, resonance. Finally, this obtained solution gives the conditions of magneto-hydrodynamic equilibrium on the magnetosphere of magnetic stars. Methodology and obtained equations are new approaches that are at first considered.展开更多
文摘维修性验证是装备维修性工作的重要组成部分,平均修复时间(mean time to repair,MTTR)是维修性定量要求验证的主要参数。本文从国内外装备MTTR验证标准和手册发展情况以及装备MTTR验证常用方法两个方面综述了MTTR验证方法的国内外研究进展。介绍了美国国防部、国际电工委员会和国内相关机构颁布的MTTR验证标准和手册的发展情况,分析了标准和手册中的MTTR验证方法。总结归纳了装备MTTR验证的常用方法及应用情况,包括基于实物装备的验证方法和基于虚拟现实的验证方法。在此基础上概括了装备MTTR验证方法的研究特点,展望了未来的研究方向,并给出了研究建议。
文摘In this paper, we consider the application of the equation of non-classical mathematical physics to magneto-hydrodynamic equilibrium (in the case of a mixed magnetic field) for magnetic stars. First, we give the necessary concepts about the equation of non-classical mathematical physics and the possibility of their applicability to astrophysical problems. The conditions of magneto-hydrodynamic equilibrium are determinate, and self-consistence provides the means to derive the corresponding partial differential equations describing this equilibrium in a magnetosphere magnetic star. Namely, this process is to the non-classical equations of mathematical physics in cases of types. Keldysh-Tricomi, a common case equation of non-classical type, is at first introduced by the author. Using the two main physical efficiencies of MHD. A mathematical model of a poloidal-toroidal mixed magnetic field for magnetic stars is constructed, and this model is classified with respect to degenerating case equations. According to Hopf’s theorem, Maxwell’s equation and the magnetic force balance equation constructed equilibrium conditions of the poloidal-toroidal of the magnetic field for a magnetic star. At the same time, the taken example, which is the self-consistency of this model by observation dates, is investigated. At first, in an application, the method of straight lines for recurrent formulas of calculation of magnetic flux and stream functions is used. The physical means, the corresponding singular point of the sonic line, cutoff, and resonance phenomena are considered. In this case, a general solution equation is found, which is interpreted by this phenomenon as a cutoff, resonance. Finally, this obtained solution gives the conditions of magneto-hydrodynamic equilibrium on the magnetosphere of magnetic stars. Methodology and obtained equations are new approaches that are at first considered.
