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1 Department of Surgery, Division of Cardiac and Thoracic Surgery, and 2 Center for Emerging Cardiovascular Technologies, Duke University Medical Center, Durham, North Carolina 27710
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ABSTRACT |
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Functional imaging computational fluid dynamics simulations of right ventricular (RV) inflow fields were obtained by comprehensive software using individual animal-specific dynamic imaging data input from three-dimensional (3-D) real-time echocardiography (RT3D) on a CRAY T-90 supercomputer. Chronically instrumented, lightly sedated awake dogs (n = 7) with normal wall motion (NWM) at control and normal or diastolic paradoxical septal motion (PSM) during RV volume overload were investigated. Up to the E-wave peak, instantaneous inflow streamlines extended from the tricuspid orifice to the RV endocardial surface in an expanding fanlike pattern. During the descending limb of the E-wave, large-scale (macroscopic or global) vortical motions ensued within the filling RV chamber. Both at control and during RV volume overload (with or without PSM), blood streams rolled up from regions near the walls toward the base. The extent and strength of the ring vortex surrounding the main stream were reduced with chamber dilatation. A hypothesis is proposed for a facilitatory role of the diastolic vortex for ventricular filling. The filling vortex supports filling by shunting inflow kinetic energy, which would otherwise contribute to an inflow-impeding convective pressure rise between inflow orifice and the large endocardial surface of the expanding chamber, into the rotational kinetic energy of the vortical motion that is destined to be dissipated as heat. The basic information presented should improve application and interpretation of noninvasive (Doppler color flow mapping, velocity-encoded cine magnetic resonance imaging, etc.) diastolic diagnostic studies and lead to improved understanding and recognition of subtle, flow-associated abnormalities in ventricular dilatation and remodeling.
ventricular function; diastole; cardiac mechanics; cardiac blood flow; endocardial mechanoreceptors
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INTRODUCTION |
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THE FLUID DYNAMICS of diastolic filling are essentially unexplored for the right ventricle (RV) (10, 11), although in the context of the left ventricle (LV), they have been shown to hold great importance for proper evaluations of diagnostic studies and in pathophysiological investigations of ventricular function (17, 18, 21, 22). The elegant, classic experimental in vitro findings on mechanical left heart models and their analytical interpretation reported by Bellhouse (1) have shown that ventricular dilatation, common in heart failure, induces a decrease in the diastolic filling vortex strength. The diastolic filling vortices of interest here are "global" or "macroscopic" in the sense that they occupy a sizeable region within the chamber. They are "large-scale" structures in contrast to "microscopic" high-frequency disturbances (eddies) within the turbulent regime downstream of a stenotic valve. Knowledge concerning diastolic RV flow field characteristics under normal conditions and changes induced by chamber dilatation should improve application and interpretation of noninvasive diagnostic studies (Doppler color flow mapping, velocity-encoded cine magnetic resonance imaging, etc.) under these conditions. They should also lead to better insights into factors limiting the accuracy of indicator dilution measurements in RV dilatation, and point toward new research areas on aspects of intracardiac flow that could be implicated in the pathophysiology of failure characterized by chamber dilatation and remodeling and their sequelae.
For these reasons, RV intraventricular diastolic filling flow patterns were investigated under normal conditions and during volume overload with or without paradoxic septal motion (PSM) as an extension of our previously published work (15). Functional imaging of the diastolic RV flow field involving computational fluid dynamic simulations in individual animals was carried out, utilizing three-dimensional (3-D) real-time echocardiography (RT3D) for dynamic RV chamber reconstructions, which were validated by simultaneous sonomicrometry, as described in a recent publication (15). The simulations yielded high spatial and temporal resolution data on the filling vortex and the evolution of the RV diastolic flow field throughout the E-wave, and quantitative visualizations elucidated its detailed dynamic characteristics in the hearts of lightly sedated, awake dogs under control conditions and in experimentally induced chamber dilatation.
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METHODS |
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Instrumentation and data acquisition.
Because of the complicated dynamic RV geometry, this investigation
required application of a recently developed functional imaging method
(15), which comprises real-time 3-D cardiac imaging and
computational fluid dynamics. Figure 1
summarizes the method.
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3-D real-time echocardiography and image segmentation. Real-time 3-D images of the RV were obtained using the RT3D ultrasound scanner (Volumetrics Medical Imaging; Durham, NC). Endocardial border detection involved proprietary software, which displayed one RV frame at a time. A two-dimensional "(2-D) Swath" algorithm (15) located the most likely position of the endocardial border. The individual points were converted into 3-D cartesian coordinates and stored in a file. Each file was a four-dimensional (4-D) matrix containing a sequence of 3-D RV chamber "volumes" ordered chronologically. Each "volume" was a succession of endocardial border layers from apex to base (Fig. 1, inset 1).
Reconstruction of endocardial border points. The data representing the extracted endocardial edges were in layered form and were further processed to generate the desired coordinates in 3-D. To obtain RV diastolic flow field simulations at a temporal resolution of 400 Hz, it was necessary to approximate the 3-D RV geometry at time instants between successive RT3D images. Under steady-state conditions, RV geometry was calculated at these instants as a quadratic weighted average of the dynamic geometry in contiguous RT3D frames. Representative RV reconstructions are depicted in Fig. 1, inset 2.
Dynamic RV chamber volume, using shell subtraction model (SSM) and sonomicrometric dimensions, and its time derivative or "inflow rate" were also calculated and compared with those obtained using RT3D data (cf. Fig. 1, inset 3). This allowed adjusting the instantaneous volume and velocity boundary conditions in the computational fluid dynamic (CFD) simulations of the flow field, as needed, according to a previously detailed scheme (15). The final set of endocardial border points served as input for mesh generation.Mesh generation and determination of boundary conditions. A combination of FIDAP (8, 9) and custom software (15) generated the mesh representing the 3-D domain for simulation of RV intraventricular diastolic flow (Fig. 1, inset 4). The instantaneous geometry defined the external nodal points of the mesh, to which were assigned boundary conditions, i.e., nodal velocity vectors describing direction and speed of instantaneous motion (Fig. 1, inset 4).
Computer simulations and flow visualization.
Simulations were carried out using the CRAY T-90 supercomputer running
FIDAP on the UNICOS operating system (Cray; Mendota Heights, MN) at the
North Carolina Supercomputing Center. They had to be completed through
consecutive runs, each advancing the solution by two to four 2.5-ms
time steps. It was assumed that blood is a Newtonian, incompressible
fluid with kinematic viscosity of 0.04 Stokes and mass density of 1.05 g/cm3 and that flow is governed by the Navier-Stokes
equations. The flow field was visualized using the FIDAP postprocessing
module, which extracts the field variables on any specified
visualization plane or "cut" within
the field (Fig. 1, inset 5; Figs. 2 and 3).
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RESULTS |
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Wall motion patterns. All seven lightly sedated, awake animals exhibited normal wall motion (NWM) at control; three also had normal and four exhibited diastolic PSM in volume overload with chamber dilatation. PSM and NWM differ qualitatively from each other in the direction of septal movement. In PSM, the septum moves toward the LV in diastole. The NWM condition exhibits the opposite scenario in which the septum functions as part of the LV and moves into the right ventricle.
RV diastolic flow field simulations.
The functional imaging simulations allowed examination of the dynamic
evolution of the RV diastolic flow field throughout the E-wave in
individual dog hearts under control and failure conditions
characterized by RV dilatation. By taking the time derivative of the
instantaneous RV volume calculated with the RT3D-based dynamic
reconstruction method, the RV diastolic filling rate could be
calculated. Representative plots of instantaneous RV volumetric filling
rate (dV/dt) and volume (V) are shown in Fig. 1,
insets 3a and b, respectively. Both control and
volume overload simulations extended throughout the E-wave (cf. arrows in Fig. 4). RV flow field information was
extracted from the databases obtained through the individual
simulations. Scientific visualization of each simulated RV flow field
disclosed the existence of large-scale vortical motions inside the
filling right ventricles of the individual dog hearts both at control
and under volume overload conditions.
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Intraventricular flow field. In the following sections, illustrative functional imaging visualizations from the individual simulations are considered together in the context of the filling process throughout the entire E-wave, for a comparison of the RV diastolic flow field characteristics in ventricular dilatation with PSM to those with NWM. We examine snapshots of the RV flow field at the following three informative points of the E-wave: early in the upstroke, at peak volumetric inflow, and late in the downstroke.
Early upstroke through the peak of the E-wave. Figure 2 illustrates typical RV flow fields developing during the early upstroke of the E-wave soon after the onset of filling (top) and at peak volumetric inflow rate (bottom). Figure 2, left, shows the flow fields applying at control with NWM and, right, the fields applying under conditions of RV dilatation with PSM in the same animal. The velocity fields are visualized on an RV coronal (frontal) plane. The arrows indicate both direction and magnitude of the flow velocity at each node within the plane. Such arrow maps are effective in revealing the spatial organization of flow within the entire flow field. Flow velocity is encoded in the length of an arrow, whereas its color is assigned according to the z component of the velocity vector. A negative z component (i.e., the blue-green region of the spectrum) maps flow toward the apex, whereas a positive one (red-orange region) represents a velocity pointing toward the RV base (see color scale inset in Fig. 2).
Figure 2, top, shows that the computed flow fields on an RV frontal plane were quite similar for both wall motion patterns. In both, the inflow velocities in the region of the tricuspid anulus and below have a balanced distribution, being directed approximately equally in each of the following directions: the anterior wall, the apex, and the posterior wall. Essentially all inflow velocity vectors are directed in a fan-like shape toward the chamber walls, which they meet perpendicularly satisfying the "no slip" condition. This pattern is consistent with the motion of intraventricular blood similar to displacement of a laminar telescoping fluid trunk peeling off successive layers that flare out laterally and meet the receding endocardium at right angles (cf. also Fig. 4). On the other hand, NWM and PSM exhibited dissimilar flow fields in the (median) sagittal plane: blood velocities were slanted toward the RV free wall in the NWM model and toward the septum in the PSM model, as previously described (15). The bottom panels in Fig. 2 pertain to peak volumetric inflow rate: the peak volumetric inflow velocity was 136 cm3/s for NWM and 216 cm3/s for PSM. Because of the higher inflow rates compared with the early inflow stage, stronger velocity fields are observed with both NWM and PSM. The magnitudes of the axial (z components) of the velocity vectors were predictably larger (dark blue) in PSM than NWM because of the much higher peak volumetric inflow rate in the volume overloaded (tricuspid regurgitation) condition. As earlier in the E-wave, NWM and PSM yield fundamentally similar fan-shaped flow velocity fields in the coronal (frontal) plane. The inflow velocity profiles in the region of the tricuspid orifice remain balanced. In a sagittal plane, with NWM the motion of the septum induced strong flow velocities toward the RV free wall, whereas with PSM the septal motion away from the RV free wall caused the individual velocity vectors to be slanted in the reverse direction, toward the septum and the left ventricle.Late downstroke of the E-wave. Figure 3, top, illustrates representative simulation plots of velocity vectors in the frontal plane. These results were obtained in the same dog as those in Fig. 2 but at instants close to the end of the E-wave. Figure 3, left, shows the flow field applying at control with NWM; the right shows the field applying under conditions of RV dilatation with PSM. The instantaneous volumetric inflow velocity was 39 cm3/s at control (NWM) and 71 cm3/s in the dilated chamber.
The most distinct feature of both flow fields at this later instant of the E-wave is the existence of large-scale vortical motions. In both the NWM and the PSM situations, streams roll up from regions near the apex toward the base. These streams are directed toward the plane of the inflow orifice, and some regurgitant flow was present under both control and volume overload conditions. In addition, the streams directed toward the inflow orifice interact with the incoming flow directed toward the apex. This interaction results in strong swirling motions, visualized nicely in Fig. 3. The extent of vortex formation appears to be stronger for the NWM case. Surprisingly, although the applying instantaneous volumetric inflow rate in NWM was much smaller than in PSM, higher (dark blue) velocity vector magnitudes are present within the control (NWM) flow field than in the dilated ventricle. The reason for this is discussed shortly. The formation of large-scale vortices results in a highly complex flow field. The general characteristics of the velocity field are better revealed using color mapping as is shown in Fig. 3, middle and bottom.Color mapping.
Figure 3, middle and bottom, shows color maps of
the velocity fields at the same instants as the corresponding velocity
plots of the top panels. Such mappings are familiar to
echocardiographers and suitable for revealing the global organization
of the flow. The regions with red and orange colors represent blood
flow toward the base of the right ventricle, whereas regions with blue
and green colors represent blood flow toward the apex. Comparison between NWM and PSM simulations showed that the vortical motion was
stronger in the former, with a high intensity in the region surrounding
the main incoming stream below the inflow orifice. This effectively
encroaches on the available central core area beyond the inflow orifice
that is available for flow toward the apex. The encroaching effect was
more pronounced in the simulations under control conditions than in the
dilated volume-overloaded ventricles (cf. Fig.
5). This is responsible for the higher
velocity vector magnitudes present within the normal flow field,
referred to in the preceding paragraph. As illustrated in the
representative case shown in Fig. 3, the vortical motion generated in
the dilated ventricles with PSM had a more even spatial distribution.
In addition, the space available for flow toward the apex, marked by
the blue, green, and yellow zones, was significantly greater for the
volume-overloaded situation.
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DISCUSSION |
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We have recently developed a comprehensive software environment that is able to model complex diastolic intracardiac flows in individual animal or human hearts (15). The integrated software system can accept data from RT3D and other digital imaging sources, such as computed tomography or magnetic resonance imaging, to generate dynamic geometric reconstructions of the cardiac chambers, which are then passed on to an automatic finite element mesh generator and a finite element solver. The flow fields of interest are then displayed using scientific visualization techniques. In the present investigation, simulations using this functional imaging system have yielded important information about the detailed diastolic RV flow fields of specific hearts in lightly sedated, awake dogs under control and volume overload conditions.
This research produced for the first time finite element 3-D simulations of diastolic blood flow into the RV chamber using in vivo, real-time 3-D dynamic RV geometric data. Completed, for the first time, were simulations of the evolution of the RV diastolic flow field throughout the entire E-wave in individual animal hearts under control and volume overload conditions associated with surgically induced experimental chronic tricuspid insufficiency. Simulations through the entire duration of the E-wave have allowed us to demonstrate the existence of large-scale 3-D vortical motions, which develop inside the RV chamber during diastole both at control and volume overload.
This study has also provided strong and important evidence regarding the impact of the applying chamber size and wall motion patterns on the development of the RV velocity field during diastole. The functional imaging approach can also be used to study the flow field in the left ventricle.
Reynolds number and distribution of nodal points.
The local Reynolds number, Re
D × v, of the RV
diastolic inflow field (6, 12) constitutes a very
important parameter in our computational fluid dynamic analysis. The
characteristic length, D, in Re is proportional to the
square root of flow cross-sectional area, whereas the velocity,
v, in a diverging flow field decreases linearly as the area
increases. Because the RV endocardial surface area is much larger than
the tricuspid orifice area (area of walls/area of orifice
10),
blood entering the chamber especially during the upstroke of the E-wave
(before the flow breaks down into the vortical pattern, see Fig. 4)
experiences powerful convective deceleration (6, 12). The
net effect of a rapidly decreasing velocity v and a slowly
increasing characteristic length D is a decrease in Re away
from the orifice along the streamlines of the blood flow. The drop in
Re is proportional to the square root of upstream to downstream flow
cross-sectional areas. The local Re is therefore highest near the
tricuspid orifice.
The RV diastolic vortex. In all simulations conducted in the seven dog hearts under control and volume overload conditions, development of large-scale vortical motions was observed during the downstroke of the E-wave. During this period, inflow velocity decreases and the pressure level rises within the flow field. As one moves away from the central stream toward the endocardial wall, convective pressure rise by the Bernoulli mechanism raises the pressure energy opposing ventricular inflow along any streamline. An adverse convective (11, 12) pressure gradient develops, and this is augmented by the local deceleration (11, 12) gradient during the downstroke of the E-wave. As is shown diagrammatically in Fig. 4, bottom left, the fanning streamlines are curved. This implies that the streaming blood is acted upon by a centripetal force and that the convective pressure gradient has a component normal to the concave streamlines also, which tends to drive the blood toward the base of the chamber (Fig. 4). Ultimately, the combined adverse pressure gradient forces arrest forward flow and deflect the direction of blood near the endocardial surface toward the base, leading to flow separation, roll up, and recirculating vortical motions within the chamber. Large-scale vortices form, as shown in Figs. 3 and 4.
Our RV simulation findings exemplified in the panels of Figs. 2 and 3 are corroborated by the adroit and elegant measurements of Rodevand et al. (17) who identified LV diastolic flow patterns in healthy human subjects with the use of high frame-rate 2-D color Doppler and color M-mode Doppler echocardiography. Intraventricular velocities were measured with pulsed Doppler at three levels in both posterolateral and anteroseptal parts of the left ventricle. During early transmitral flow acceleration, all intraventricular velocities were directed toward the apex. However, retrograde peripheral velocities representing diastolic vortex formation were documented after the peak of the E-wave. These LV findings, which are further discussed in a clinical survey of filling dynamics by Smiseth and Thompson (21), are thus seen to be in complete agreement with our RV functional imaging results in awake dogs. To look now at why a vortex display comes about, we invoke the Theory of Dissipative Structures, formulated by Ilya Prigogine (16). Because of the movement and exchange of energy, when the simple fanlike pattern breaks down, the flow is likely to reorganize itself in a more complex interactive form and achieves coherence in the vortical arrangement. Blood moves through the filling vortex and forms it at the same time. Energy moves likewise through the vortical structure and the latter embodies the energy, highly organized and in motion, as rotational kinetic energy of the vortex.Physiological significance. With the use of functional imaging (15), this study is the first to show the existence of vortical motion inside the right ventricle. The physiological repercussions of the vortical motion are most intriguing. Bellhouse (1), who conducted experimental studies on the LV diastolic vortex in the context of cardiac physiology in the early 1970s, proposed that vortical motion might assist in valve closure. Others (25) have suggested that the presence of LV diastolic vortical motions helps in the ensuing process of ejection, by conversion of vortex kinetic energy into kinetic energy of outflow after aortic valve opening. According to this view, vortices within the ventricle would act as energy-preserving flow structures (4). It is well known in fluid mechanics, however, that large vortices never unwind smoothly. Instead, they break up into smaller eddies, and this process is continued, until the vortices are reduced to micron-size eddies and at that level (Kolmogorov "microscale") they dissipate under the action of viscous forces (19). The process is known as the vortical cascade mechanism. This implies that vortices are essentially "traps" or "sinks of energy." Whatever kinetic energy is trapped in the recirculating motion of a vortex is bound to be converted to heat and lost from the motion and therefore cannot in fact aid ejection.
We propose a new hypothesis concerning the useful role played by the vortices in overall diastolic function. According to the hypothesis, the difference between the inflow orifice area (Ai) and the endocardial surface area (Aendo) is responsible for generating strong convective deceleration before transition to vortical flow in diastole (cf. Fig. 4). The diastolic intraventricular pressure gradient resulting from this convective deceleration, termed "convective deceleration load," adversely impacts diastolic inflow. This adverse impact is amplified in the presence of ventricular dilatation with attendant diastolic "ventriculoannular disproportion." The concept is analogous to the systolic one introduced in earlier studies (12). The key to the proposed useful physiological role of the vortices lies within their impounding of a certain amount of energy, and this becomes manifest as a decrease in the pressure energy of the inflowing blood. By shunting the inflow work and kinetic energy, which would otherwise contribute an inflow-impeding, pressure-rise between inflow orifice and the endocardial surface of the expanding chamber, into the kinetic energy of the vortical motion (Figs. 4 and 5) that is destined to be dissipated as heat, the diastolic vortex actually facilitates filling and the attainment of higher end-diastolic volume.Clinical impact of RV size and wall motion patterns. Using functional imaging, we have demonstrated that not just quantitative but qualitative important alterations in the intraventricular velocity field result from changes in applying RV dynamic geometry and wall motion patterns. As shown by the results presented, the impact of abnormal chamber dilatation and wall motion patterns on RV flow is manifested throughout the entire E-wave. In this study, we have been able to characterize extensively the resultant alterations of the diastolic flow field. Our functional imaging simulation findings are in agreement with the classic studies of Bellhouse (1), who reported reduced vortex strength and extent in dilated ventricles.
The reduced extent and strength of the diastolic vortex in RV chamber dilatation with diastolic PSM (cf. Fig. 5) may have notable clinical implications. Thus, in a meticulous clinical study (7), RV end-diastolic and end-systolic volume indexes in patients with dilated cardiomyopathy were significantly higher by thermodilution compared with MRI, and exclusion of patients with atrial fibrillation did not reduce the mean difference between both methods. Impaired indicator mixing associated with weakened vortical motions (Fig. 6) in the dilated cardiomyopathic ventricles could be responsible by introducing a strong violation of the underlying assumption of "perfect mixing" between injection and sampling sites.
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ACKNOWLEDGEMENTS |
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This work was supported in part by National Heart, Lung, and Blood Institute Grant R01-HL-50446 (to A. Pasipoularides), the North Carolina Supercomputing Center/Cray Research (to A. Pasipoularides), and the Duke/National Science Foundation Engineering Research Center for Emerging Cardiovascular Technologies (to A. Pasipoularides and M. Shu).
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FOOTNOTES |
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Address for reprint requests and other correspondence: D. D. Glower, Dept. of Surgery, PO Box 3851, Medical Center, Duke Univ., Durham, NC 27710.
The costs of publication of this article were defrayed in part by the payment of page charges. The article must therefore be hereby marked "advertisement" in accordance with 18 U.S.C. Section 1734 solely to indicate this fact.
First published December 19, 2002;10.1152/ajpheart.00804.2002
Received 13 September 2002; accepted in final form 13 December 2002.
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Q. Xi, D. Tcheranova, H. Parfenova, B. Horowitz, C. W. Leffler, and J. H. Jaggar Carbon monoxide activates KCa channels in newborn arteriole smooth muscle cells by increasing apparent Ca2+ sensitivity of {alpha}-subunits Am J Physiol Heart Circ Physiol, February 1, 2004; 286(2): H610 - H618. [Abstract] [Full Text] [PDF] |
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A. Pasipoularides, M. Shu, A. Shah, A. Tucconi, and D. D. Glower RV instantaneous intraventricular diastolic pressure and velocity distributions in normal and volume overload awake dog disease models Am J Physiol Heart Circ Physiol, November 1, 2003; 285(5): H1956 - H1965. [Abstract] [Full Text] [PDF] |
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