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91.
平均应力法用于航空发动机轮盘破裂转速预测时结果一般偏大,对于带螺栓孔的轮盘破裂转速预测误差更大。考虑局部应力效应对平均应力法进行修正,引入修正因子来表征轮盘子午面平均周向应力和危险部位局部应力对轮盘破裂转速的加权影响。通过开展典型轮盘材料GH4169的光滑试样和缺口试样拉伸试验,并开展了两件模拟盘破裂转速测量试验,得到修正因子与缺口强度比的关系,然后同时采用这两种方法对某涡轮盘的破裂转速进行了预测,并开展了验证试验。试验结果表明:平均应力法预测结果偏大,误差达到了9.4%,而考虑局部应力修正后,预测值仅略低于试验值,误差仅2.67%。考虑局部应力效应的轮盘子午面破裂转速预测方法简单可靠,具有较高的工程实用价值。 相似文献
92.
93.
Saša Simić Luka Č. Popović 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We investigate the variability of the continuum and broad lines in QSO spectra (particularly in the Hβ line and continuum at λ 5100 Å) caused by microlensing of a diffuse massive structure (like an open star cluster). We modeled the continuum and line emitting region and simulate a lensing event by a star cluster located in an intervening galaxy. Such a type of microlensing event can have a significant influence on magnification and centroid shift of the broad lines and continuum source. We explore relationships between the continuum and broad line flux variability during the microlensing event. 相似文献
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95.
为解决旋转固体表面对流换热系数测试难题,设计并研发了一款基于稳态方法的自热型对流换热系数传感器。进行了管道标定实验,分别与经典经验公式以及自制的标定端进行了对比,结果发现传感器的测试存在一个稳定的比例系数,经修正后相对误差小于5%。采用数值模拟方法进一步从机理方面探究了该比例系数存在的合理性,发现在阶跃加热的情况下存在一个"热调整区",会导致对流换热的阶跃性变化,这种变化类似于"入口效应",同时这种效应不受加热段温度的影响,定性地验证了传感器测量的准确性。 相似文献
96.
通过对P25Ti O2光阳极薄膜厚度、敏化的量子点种类及量子点敏化方法研究,探讨了使用连续离子层吸附反应法的敏化方法(SILAR)时,P25Ti O2薄膜厚度与光阳极电子寿命的关系,以及量子点种类、共敏化工艺对光阳极光电性能的影响.采用电化学阻抗(EIS)、开路电压衰减(OCVD)及紫外-可见吸收方法,对影响光阳极光电性能的Ti O2薄膜厚度、量子点种类及共敏化工艺因素进行测试分析.实验结果表明:当光阳极薄膜厚度为12μm时,电子复合几率最小,光阳极的电子寿命相对最长;采用连续离子层吸附反应法(SILAR)对多种量子点共敏化的光阳极(Ti O2/Cd S/Cd Se/Zn S)与单一量子点敏化的光阳极(Ti O2/Cd S)相比,短路电流提高了34%,光转换效率提高了42%;合适的共敏化工艺也有助于提高光阳极的电子寿命、光谱吸收范围和吸收强度. 相似文献
97.
Development and calibration of heat transfer coefficient sensor for rotational state 总被引:1,自引:0,他引:1
A novel heat transfer coefficient sensor is introduced and the design, manufacture,and calibration are described.The intended application of this instrument was on a high rotational speed test disc. In the experiments,the heat transfer coefficient sensor was calibrated under static state and rotational state respectively. The calibration under the static state was accomplished in a pipe: the inside diameter (ID) was 0.048m and the total length was 4m, the distance between the sensor and the inlet of the pipe was 3.5m; the standard value was measured using a self-made calibrator. The calibration under the rotational state was accomplished using a rotating disc: the diameter and thickness of the stainless disc were 800mm and 25mm, respectively;the sensor was installed at the location of r =250mm; the rotating disc driven by a 30kW direct current motor can supply the maximum rotational speed of 3000r/min. The standard value under rotational state was provided by an approximate empirical formula. The results show that the designed sensor can measure heat transfer coefficient directly under rotational state and static state with good accuracy and stability; the correlation factor of K are constant under static state and rotational state. 相似文献
98.
99.
The ACE Magnetic Fields Experiment 总被引:2,自引:0,他引:2
Smith C.W. L'Heureux J. Ness N.F. Acuña M.H. Burlaga L.F. Scheifele J. 《Space Science Reviews》1998,86(1-4):613-632
The magnetic field experiment on ACE provides continuous measurements of the local magnetic field in the interplanetary medium.
These measurements are essential in the interpretation of simultaneous ACE observations of energetic and thermal particles
distributions. The experiment consists of a pair of twin, boom- mounted, triaxial fluxgate sensors which are located 165 inches
(=4.19 m) from the center of the spacecraft on opposing solar panels. The electronics and digital processing unit (DPU) is
mounted on the top deck of the spacecraft. The two triaxial sensors provide a balanced, fully redundant vector instrument
and permit some enhanced assessment of the spacecraft's magnetic field. The instrument provides data for Browse and high-level
products with between 3 and 6 vector s−1 resolution for continuous coverage of the interplanetary magnetic field. Two high-resolution
snapshot buffers each hold 297 s of 24 vector s−1 data while on- board Fast Fourier Transforms extend the continuous data
to 12 Hz resolution. Real-time observations with 1-s resolution are provided continuously to the Space Environmental Center
(SEC) of the National Oceanographic and Atmospheric Association (NOAA) for near- instantaneous, world-wide dissemination in
service to space weather studies. As has been our team's tradition, high instrument reliability is obtained by the use of
fully redundant systems and extremely conservative designs. We plan studies of the interplanetary medium in support of the
fundamental goals of the ACE mission and cooperative studies with other ACE investigators using the combined ACE dataset as
well as other ISTP spacecraft involved in the general program of Sun-Earth Connections.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
100.
层板冷却结构强化换热机理 总被引:8,自引:7,他引:1
应用简化的换热模型分析了影响层板冷却效果的因素,得出了燃气侧气膜冷却效率ηf,层板内部换热效率ηi和参数f是影响冷效的决定因素。为了研究层板强化换热机理,提高其内部换热效率ηi以优化层板传热设计,本文在相同的两侧换热条件和冷气密流下,对5种相同孔径、通道高度和开孔率,不同内部绕流形式的层板结构和1种双层壁结构进行了流固耦合传热计算,得到了其综合冷却效率。结果表明层板结构的综合冷却效率明显高于双层壁;冷气沿程吸热焓增带走了大部分从燃气侧进入层板的热,并且冷气与层板内表面的换热主要发生在出气板上,扰流柱的存在增加了换热面积,一定程度上增强了换热;合理设计绕流结构有利于改善层板的热均匀性。 相似文献