Right Ventricular Longitudinal Strain in Acute Pulmonary Embolism and Right Ventricular Myocardial Infarction in Patients with McConnell’s Sign

Aim      To study the right ventricular (RV) myocardial longitudinal systolic strain in patient with RV myocardial infarction (MI), and pulmonary embolism (PE) with and without McConnell’ phenomenon.

Material and methods  This study included 53 patients with PE (mean age, 59.0±15.1 years; men, 58.5 %) and 30 patients with RVMI (mean age, 61.8±10.9 years; men, 90 %). Longitudinal strain of basal, medial and apical segments of the RV free wall (RVFW) and the interventricular septum (IVS) was determined in the mode of two-dimensional speckle tracking. Ratio of the IVS apical strain to the RVFW strain (apical ratio) was calculated. Systolic excursion of the RVFW apical segment (apical excursion) was measured in the anatomical M-mode from the apical four-chamber view.

Results The McConnell’s sign was observed in 23 (43.4 %) of 53 patients with PE and in 16 (53.3 %) of 30 patients with RVMI (p>0.05). Irrespective of the cause for the RV damage, patients with the McConnell’s sign had higher values of the apical ratio (1.69±0.50 vs. 0.95±0.22; p<0.001; cutoff point, 1.18) and apical excursion (7.9±1.7 vs. 2.6±1.4 mm; p<0.001; cutoff point, 5.0 mm). Apical excursion closely correlated with the value of apical ratio (r=0.65; p<0.001) but not with the RVFW apical segment strain (r= –0.07; p>0.05).

Conclusion      Incidence of the McConnell’s sign was similar in patients with PE and RVMI. McConnell’s sign is based on a passive systolic shift of the RVFW apical segment, which develops during contraction of the IVS apical segment. The greater the ratio of IVS apical segment to RBFW global strain the greater the amplitude of this shift. With the ratio value of 1.18 or more, the systolic shift of RVFW apical segment was >5 mm, which was visually perceived as the McConnell’s sign.

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