Abstract

Objective To evaluate the left ventricular mechanical dyssynchrony in patients with chronic heart failure(CHF)by two dimensional speckle tracking imaging(2D-STI).Methods 37 CHF patients were enrolled in this study.According to left ventricular ejection fraction(LVEF),the patienst were classified into two subgroups:group A,LVEF≤ 35 %;group B,35 %<LVEF<50 %.35 healthy volunteers constituted the control group(group C).Standard 2D images were acquired in the 2-,3-and 4-apical views as well as the parasternal short-axis views at the level of the mitral valve and papillary muscles.The time to peak-systolic strain and strain rate were measured for each segment in the level of the mitral valve and papillary muscles in Qlab software.Dyssychrony parameters were defined as the standard deviation and the maximal time delay of the time to peak-systolic strain and strain rate for 12 segments.Parameters were compared among the three groups respectively.The correlation between dyssynchrony parameters and LVEF were analysed in CHF patients.The cut-off value of each parameter were derived from group C based on statistical principles.Dyssychrony rate of each parameter were calculated in group A and B,and compared within each group respectively.Results Compared with group C,all the dyssychrony parameters in group A were significant higher(P<0.05),and part of the parameters(Tsl-12SD,Tsl-12Dif,Tslr-12SD,Tslr-12Dif and Tsr-12SD)in group B were remarkable higher(P<0.05).Dyssychrony parameters in CHF patients correlated closely with LVEF(P<0.05).Significant differences among dyssychrony rates were noted in both group A and B(P<0.05),and Ts1-12SD showed the highest value in both subgroups.Conclusions 2D-STI is useful in quantifying left ventricular systolic dyssychrony in CHF patients,and the longitudinal parameters are more efficient to detect mechanical dyssychrony than the radial parameters and circumferential parameters. Key words: Echocardiography; Heart failure,congestive; Ventricular function,left; Speckle tracking imaging

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