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851.
852.
《中国航空学报》2022,35(8):1-6
The autonomous and controllable Dual Synthetic Jet Actuator (DSJA) is firstly integrated into the Unmanned Aerial Vehicle (UAV), and flight tests without the deflection of rudders are carried out to verify the viability of DSJA to control the attitudes of UAV during cruising. DSJA is improved into an actuator with two diaphragms and three cavities, which has higher energy levels. Actuators, differentially distributed on both sides of the wings, are installed on the trailing edge close to the wing tips. Flight tests, containing Differential Circulation Control (DCC) using double-side actuators, Positive Circulation Control (PCC) using left-side actuators and Negative Circulation Control (NCC) using right-side actuators, are implemented at cruising speed of 25 m/s. Results show that roll attitude control without rudders could be realized by DSJAs. DCC and NCC can generate the rightward roll and yaw angular velocity, prompting UAV to turn right. The stronger controlling ability can be achieved by DCC, with the maximum roll angular velocity of 15.62 (°)/s. PCC can generate a rightward roll moment, but a leftward yaw moment will be produced at the same time. Leftward yaw induces the leftward rolling moment, which weakens the roll control effect, making UAV keep to yaw to the left with a small slope. 相似文献
853.
Mg粉/CO2粉末发动机是火星探测中较为理想的原位资源利用方案,为了掌握Mg/CO2粉末发动机稳定点火燃烧特性,在考虑氧化层厚度对Mg颗粒熄火影响的基础上,基于涡耗散/有限速率模型建立了点火燃烧模型,并应用数值计算方法研究了Mg粉颗粒粒径(5μm, 10μm, 15μm, 20μm和25μm)、入口预混气流雷诺数(1500, 2000, 2500, 3000和3500)和CO2/Mg氧燃比(0.5, 1, 1.5, 2和2.5)对Mg粉/CO2动态点火燃烧的影响。计算结果表明:雷诺数和氧燃比恒定时,随着粒径从5μm增加到10μm,平均温度升高,平均点火时间延长,燃烧效率增加;随着粒径从10μm增加到25μm,平均温度降低,平均点火时间延长,燃烧效率减少。粒径和氧燃比恒定时,平均温度随雷诺数增加而下降;平均点火时间和燃烧效率随雷诺数增加基本不变。粒径和雷诺数恒定,随着氧燃比从0.5增大到1.5,平均温度升高;随着氧燃比从1.5增大到2.5,平均温度下降;平均点火时间和燃烧效率随氧燃比增大基本不变。 相似文献
854.
The present study proposes a segmented cooling-stream injection structure based on a certain coolant mass flow rate, and numerically investigates the effect of segmented cooling-stream injection on supersonic film cooling. The results indicate that without shock-wave impingement and with helium as the coolant, segmented cooling-stream injection can reduce the mixing between the mainstream and the cooling stream to produce better cooling performance than single injection, especially at larger coo... 相似文献
855.
《中国航空学报》2022,35(12):117-129
The Dual Synthetic Jet Actuator (DSJA) is used to develop a new type of lift enhancement device based on circulation control, and to control the flow over the two-dimensional (2D) NACA0015 airfoil. The lift enhancement device is composed of a DSJA and a rounded trailing edge (Coanda surface). The two outlets of the DSJA eject two jets (Jet 1 and Jet 2). Jet 1 ejects from the upper trailing edge, which increases the circulation of airfoil with the help of the Coanda surface. Jet 2 ejects from the lower trailing edge, which acts as a virtual flap. The Reynolds number based on the airfoil chord length and free flow velocity is 250000. The results indicate that the circulation control method based on Dual Synthetic Jet (DSJ) has good performance in lift enhancement, whose control effect is closely related to momentum coefficient and reduced frequency. With the increase of the reduced frequency, the control effect of the lift enhancement is slightly reduced. As the momentum coefficient increases, the control effect becomes better. When the angle of attack is greater than 4°, the increments of lift coefficients under the control of DSJ are larger than those under the control of the steady blowing at a same momentum coefficient. The maximum lift augmentation efficiency can reach 47 when the momentum coefficient is 0.02, which is higher than the value in the case with steady blowing jet circulation control. 相似文献
856.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(5):2240-2251
This study examines the occurrences rate of geomagnetic storms during the solar cycles (SCs) 20–24. It also investigates the solar sources at SCs 23 and 24. The Disturbed storm time (Dst) and Sunspot Number (SSN) data were used in the study. The study establishes that the magnitude of the rate of occurrences of geomagnetic storms is higher (lower) at the descending phases (minimum phases) of solar cycle. It as well reveals that severe and extreme geomagnetic storms (Dst < -250 nT) seldom occur at low solar activity but at very high solar activity and are mostly associated with coronal mass ejections (CMEs) when occurred. Storms caused by CME + CH-HSSW are more prominent during the descending phase than any other phase of the solar cycle. Solar minimum features more CH-HSSW- associated storms than any other phase. It was also revealed that all high intensity geomagnetic storms (strong, severe and extreme) are mostly associated with CMEs. However, CH-HSSW can occasionally generate strong storms during solar minimum. The results have proven that CMEs are the leading cause of geomagnetic storms at the ascending, maximum and the descending phases of the cycles 23 and 24 followed by CME + CH-HSSW. The results from this study indicate that the rate of occurrence of geomagnetic storms could be predicted in SC phases. 相似文献