The direct torque control of the dual star induction motor(DTC-DSIM) using conventional PI controllers is characterized by unsatisfactory performance, such as high ripples of torque and flux, and sensitivity to parame...The direct torque control of the dual star induction motor(DTC-DSIM) using conventional PI controllers is characterized by unsatisfactory performance, such as high ripples of torque and flux, and sensitivity to parametric variations. Among the most evoked control strategies adopted in this field to overcome these drawbacks presented in classical drive, it is worth mentioning the use of the second order sliding mode control(SOSMC) based on the super twisting algorithm(STA) combined with the fuzzy logic control(FSOSMC). In order to realize the optimal control performance, the FSOSMC parameters are adjusted using an optimization algorithm based on the genetic algorithm(GA). The performances of the envisaged control scheme, called G-FSOSMC, are investigated against G-SOSMC, G-PI and BBO-FSOSMC algorithms. The proposed controller scheme is efficient in reducing the torque and flux ripples, and successfully suppresses chattering. The effects of parametric uncertainties do not affect system performance.展开更多
We implemented a 3-3-1 algorithm in order to provide safe and simple self-titration in patients who newly initiated BOT as well as who were already on BOT and evaluated its utility in clinical setting. A total of 46 p...We implemented a 3-3-1 algorithm in order to provide safe and simple self-titration in patients who newly initiated BOT as well as who were already on BOT and evaluated its utility in clinical setting. A total of 46 patients, 21 patients in the newly-initiated group and 25 patients in the existing BOT group performed dose adjustment using 3-3-1 algorithm. HbA1c was significantly improved 4 weeks after the initiation from 8.5% ± 1.2% at baseline to 7.3% ± 0.7% at the final evaluation (p 0.01, vs. Baseline). The average daily insulin units increased throughout the study period from 10.1 ± 6.7 at baseline to 14.6 ± 8.9 units at the final evaluation. Weight didn’t significantly change throughout the study (p = 0.12). The incidents of hypoglycemia were 0.8/month during the insulin dose self-adjustment period and 0.4/month during the follow-up period. The 3-3-1 algorithm using insulin glargine provided a safe and simple dose adjustment and demonstrated its utility in patients who were newly introduced to insulin treatment as well as who were already on BOT.展开更多
To improve the quality of the illumination distribution,one novel indoor visible light communication(VLC)system,which is jointly assisted by the angle-diversity transceivers and simultaneous transmission and reflectio...To improve the quality of the illumination distribution,one novel indoor visible light communication(VLC)system,which is jointly assisted by the angle-diversity transceivers and simultaneous transmission and reflection-intelligent reflecting surface(STAR-IRS),has been proposed in this work.A Harris Hawks optimizer algorithm(HHOA)-based two-stage alternating iteration algorithm(TSAIA)is presented to jointly optimize the magnitude and uniformity of the received optical power.Besides,to demonstrate the superiority of the proposed strategy,several benchmark schemes are simulated and compared.Results showed that compared to other optimization strategies,the TSAIA scheme is more capable of balancing the average value and variance of the received optical power,when the maximal ratio combining(MRC)strategy is adopted at the receiver.Moreover,as the number of the STAR-IRS elements increases,the optical power variance of the system optimized by TSAIA scheme would become smaller while the average optical power would get larger.This study will benefit the design of received optical power distribution for indoor VLC systems.展开更多
The central compact object XMMU J173203.3-344518 in the supernova remnant HESS J1731-347 challenges conventional neutron star models due to its low mass M=0.77_(-0.17)^(+0.20)M■and high redshifted surface temperature...The central compact object XMMU J173203.3-344518 in the supernova remnant HESS J1731-347 challenges conventional neutron star models due to its low mass M=0.77_(-0.17)^(+0.20)M■and high redshifted surface temperature T_(s)^(∞)=156_(-6)^(+6)e V (1.81_(-0.07)^(+0.07)×10^(6)K).We investigate the observational properties of XMMU J173203.3-344518 within a color-flavor-locked(CFL) phase strange star model.We construct a thermal evolution model of the CFL phase strange star,along with heating due to the viscous dissipation of r-mode oscillations.Employing one of th most widely used quark matter equations of state,we characterize the star properties by the strange quark mas(ms),effective bag constant (Beff),perturbative QCD correction (a4),and pairing gap (Δ).Our analysi demonstrates that the observed properties of XMMU J173203.3344518 can be explained by r-mode heating with CFL strange star,provided that the initial spin period is shorter than 18 ms.We constrain the r-mode saturation amplitude to 8×10^(-3)–1.4×10^(-2)and predict a current spin period of 6–9 ms for an initial period of 1 ms.Thi rapid rotation is consistent with the absence of detected pulsations.The r-mode instability window remains robus across a wide range of pairing gap values (5–200 MeV),providing a reliable framework for interpretation regardless of microscopic uncertainties.Our results support the identification of XMMU J173203.3344518 as rapidly rotating,low-mass CFL phase strange star,demonstrating the importance of r-mode heating in the therma evolution of compact objects with exotic dense matter.展开更多
基金Project supported by the LEB Research LaboratoryDepartment of Electrical Engineering,University of Batna 2, Algeria。
文摘The direct torque control of the dual star induction motor(DTC-DSIM) using conventional PI controllers is characterized by unsatisfactory performance, such as high ripples of torque and flux, and sensitivity to parametric variations. Among the most evoked control strategies adopted in this field to overcome these drawbacks presented in classical drive, it is worth mentioning the use of the second order sliding mode control(SOSMC) based on the super twisting algorithm(STA) combined with the fuzzy logic control(FSOSMC). In order to realize the optimal control performance, the FSOSMC parameters are adjusted using an optimization algorithm based on the genetic algorithm(GA). The performances of the envisaged control scheme, called G-FSOSMC, are investigated against G-SOSMC, G-PI and BBO-FSOSMC algorithms. The proposed controller scheme is efficient in reducing the torque and flux ripples, and successfully suppresses chattering. The effects of parametric uncertainties do not affect system performance.
文摘We implemented a 3-3-1 algorithm in order to provide safe and simple self-titration in patients who newly initiated BOT as well as who were already on BOT and evaluated its utility in clinical setting. A total of 46 patients, 21 patients in the newly-initiated group and 25 patients in the existing BOT group performed dose adjustment using 3-3-1 algorithm. HbA1c was significantly improved 4 weeks after the initiation from 8.5% ± 1.2% at baseline to 7.3% ± 0.7% at the final evaluation (p 0.01, vs. Baseline). The average daily insulin units increased throughout the study period from 10.1 ± 6.7 at baseline to 14.6 ± 8.9 units at the final evaluation. Weight didn’t significantly change throughout the study (p = 0.12). The incidents of hypoglycemia were 0.8/month during the insulin dose self-adjustment period and 0.4/month during the follow-up period. The 3-3-1 algorithm using insulin glargine provided a safe and simple dose adjustment and demonstrated its utility in patients who were newly introduced to insulin treatment as well as who were already on BOT.
基金supported by the National Natural Science Foundation of China(No.62071365)the Key Research and Development Program of Shaanxi Province(No.2017ZDCXL-GY-06-02).
文摘To improve the quality of the illumination distribution,one novel indoor visible light communication(VLC)system,which is jointly assisted by the angle-diversity transceivers and simultaneous transmission and reflection-intelligent reflecting surface(STAR-IRS),has been proposed in this work.A Harris Hawks optimizer algorithm(HHOA)-based two-stage alternating iteration algorithm(TSAIA)is presented to jointly optimize the magnitude and uniformity of the received optical power.Besides,to demonstrate the superiority of the proposed strategy,several benchmark schemes are simulated and compared.Results showed that compared to other optimization strategies,the TSAIA scheme is more capable of balancing the average value and variance of the received optical power,when the maximal ratio combining(MRC)strategy is adopted at the receiver.Moreover,as the number of the STAR-IRS elements increases,the optical power variance of the system optimized by TSAIA scheme would become smaller while the average optical power would get larger.This study will benefit the design of received optical power distribution for indoor VLC systems.
基金supported in part by the Natural Science Foundation of Xinjiang Uygur Autonomous Region (No.2023D01E20)the National Key R&D Program of China (No.2022YFA1603104)+3 种基金the National Natural Science Foundation of China (Nos.12288102,12273028 and 12033001)the Tianshan talents program (2023TSYCTD0013)the Major Science and Technology Program of Xinjiang Uygur Autonomous Region (No.2022A03013-1)the Urumqi Nanshan Astronomy and Deep Space Exploration Observation and Research Station of Xinjiang (XJYWZ2303)。
文摘The central compact object XMMU J173203.3-344518 in the supernova remnant HESS J1731-347 challenges conventional neutron star models due to its low mass M=0.77_(-0.17)^(+0.20)M■and high redshifted surface temperature T_(s)^(∞)=156_(-6)^(+6)e V (1.81_(-0.07)^(+0.07)×10^(6)K).We investigate the observational properties of XMMU J173203.3-344518 within a color-flavor-locked(CFL) phase strange star model.We construct a thermal evolution model of the CFL phase strange star,along with heating due to the viscous dissipation of r-mode oscillations.Employing one of th most widely used quark matter equations of state,we characterize the star properties by the strange quark mas(ms),effective bag constant (Beff),perturbative QCD correction (a4),and pairing gap (Δ).Our analysi demonstrates that the observed properties of XMMU J173203.3344518 can be explained by r-mode heating with CFL strange star,provided that the initial spin period is shorter than 18 ms.We constrain the r-mode saturation amplitude to 8×10^(-3)–1.4×10^(-2)and predict a current spin period of 6–9 ms for an initial period of 1 ms.Thi rapid rotation is consistent with the absence of detected pulsations.The r-mode instability window remains robus across a wide range of pairing gap values (5–200 MeV),providing a reliable framework for interpretation regardless of microscopic uncertainties.Our results support the identification of XMMU J173203.3344518 as rapidly rotating,low-mass CFL phase strange star,demonstrating the importance of r-mode heating in the therma evolution of compact objects with exotic dense matter.
