基于tms320f28027的逆变电源制作

实现直流转交流的电压变换装置称为逆变器。传统的逆变器由单片机输出SPWM控制,程序设计与电路设计复杂。本文拟采用属于DSP的tms320f28027作为控制系统。利用其强大的浮点计算能力及功能齐全,高精度的外设模块在极大地简化电路与程序设计的情况下可方便地对逆变器进行精准控制。包括全桥逆变电路,LC滤波电路的主电路在DSP接收反馈并进行PI计算后输出相应的SPWM的情况下可输出正弦波交流电压。依据设计方案制作了样机,实验结果证明样机能输出纯净的正弦波电压,能够满足设计指标要求

AMT起步过程中离合器模糊自适应控制技术研究

针对电控机械式自动变速器（Automated Mechanical Transmission,AMT）中离合器起步过程控制不精确,易导致离合器磨损严重,车辆产生较大冲击等关键问题,以AMT离合器为研究对象,以减小冲击度和滑磨功为目标提出了一种模糊自适应控制方法。先采用模糊控制对含有不确定参数的离合器控制问题进行具体分析,再采用自适应控制理论以输入参数为控制对象对模糊控制规则进行修正。并将其与传统模糊控制器的控制效果对比,通过仿真和试验验证该控制策略的有效性。结果表明,模糊自适应控制器在车辆起步过程中比模糊控制器更精确有效,能在一定程度上降低车辆冲击度和离合器滑磨功,减小离合器摩擦片的磨损,从而显著提高其驾驶性能

Amplitude analysis of the decays D0 → π+π−π+π− and D0 → π+π−π0π0*

Using e+e− annihilation data corresponding to an integrated luminosity of 2.93 fb−1 taken at the center-of-mass energy √s = 3.773 GeV with the BESIII detector, a joint amplitude analysis is performed on the decays D0 → π+π−π+π− and D0 → π+π−π0π0 (non-η). The fit fractions of individual components are obtained, and large interferences among the dominant components of the decays D0 → a1(1260)π, D0 → π(1300)π, D0 → ρ(770)ρ(770), and D0 → 2(ππ)S are observed in both channels. With the obtained amplitude model, the CP-even fractions of D0 → π+π−π+π− and D0 → π+π−π0π0 (non-η) are determined to be (75.2 ± 1.1stat. ± 1.5syst.) % and (68.9 ± 1.5stat. ± 2.4syst.)%, respectively. The branching fractions of D0 → π+π−π+π− and D0 → π+π−π0π0 (non-η) are measured to be (0.688 ± 0.010stat. ± 0.010syst.)% and (0.951 ± 0.025stat. ± 0.021syst.)%, respectively. The amplitude analysis provides an important model for the binning strategy in measuring the strong phase parameters of D0 → 4π when used to determine the CKM angle γ(φ3) via the B− → DK− decay

Measurement of integrated luminosity of data collected at 3.773 GeV by BESIII from 2021 to 2024

We present a measurement of the integrated luminosity e+e- of collision data collected by the BESIII detector at the BEPCII collider at a center-of-mass energy of Ecm = 3.773 GeV. The integrated luminosities of the datasets taken from December 2021 to June 2022, from November 2022 to June 2023, and from October 2023 to February 2024 were determined to be 4.995±0.019 fb-1, 8.157±0.031 fb-1, and 4.191±0.016 fb-1, respectively, by analyzing large angle Bhabha scattering events. The uncertainties are dominated by systematic effects, and the statistical uncertainties are negligible. Our results provide essential input for future analyses and precision measurements