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1.
PLoS One ; 11(10): e0162938, 2016.
Article in English | MEDLINE | ID: mdl-27727298

ABSTRACT

PURPOSE: Previous computational fluid dynamics (CFD) studies have demonstrated that the Chiari malformation is associated with abnormal cerebrospinal fluid (CSF) flow in the cervical part of the subarachnoid space (SAS), but the flow in the SAS of the posterior cranial fossa has received little attention. This study extends previous modelling efforts by including the cerebellomedullary cistern, pontine cistern, and 4th ventricle in addition to the cervical subarachnoid space. METHODS: The study included one healthy control, Con1, and two patients with Chiari I malformation, P1 and P2. Meshes were constructed by segmenting images obtained from T2-weighted turbo spin-echo sequences. CFD simulations were performed with a previously verified and validated code. Patient-specific flow conditions in the aqueduct and the cervical SAS were used. Two patients with the Chiari malformation and one control were modelled. RESULTS: The results demonstrated increased maximal flow velocities in the Chiari patients, ranging from factor 5 in P1 to 14.8 in P2, when compared to Con1 at the level of Foramen Magnum (FM). Maximal velocities in the cervical SAS varied by a factor 2.3, while the maximal flow in the aqueduct varied by a factor 3.5. The pressure drop from the pontine cistern to the cervical SAS was similar in Con1 and P1, but a factor two higher in P2. The pressure drop between the aqueduct and the cervical SAS varied by a factor 9.4 where P1 was the one with the lowest pressure jump and P2 and Con1 differed only by a factor 1.6. CONCLUSION: This pilot study demonstrates that including the posterior cranial fossa is feasible and suggests that previously found flow differences between Chiari I patients and healthy individuals in the cervical SAS may be present also in the SAS of the posterior cranial fossa.


Subject(s)
Arnold-Chiari Malformation/physiopathology , Cerebrospinal Fluid/physiology , Cranial Fossa, Posterior/physiology , Subarachnoid Space/physiology , Adult , Algorithms , Arnold-Chiari Malformation/cerebrospinal fluid , Arnold-Chiari Malformation/diagnostic imaging , Cranial Fossa, Posterior/diagnostic imaging , Female , Humans , Hydrodynamics , Magnetic Resonance Imaging , Middle Aged , Pilot Projects , Pressure , Subarachnoid Space/diagnostic imaging
2.
Article in English | MEDLINE | ID: mdl-26176823

ABSTRACT

Syringomyelia, fluid-filled cavities within the spinal cord, occurs frequently in association with a Chiari I malformation and produces some of its most severe neurological symptoms. The exact mechanism causing syringomyelia remains unknown. Since syringomyelia occurs frequently in association with obstructed cerebrospinal fluid (CSF) flow, it has been hypothesized that syrinx formation is mechanically driven. In this study we model the spinal cord tissue either as a poro-elastic medium or as a solid linear elastic medium, and simulate the propagation of pressure waves through an anatomically plausible 3D geometry, with boundary conditions based on in vivo CSF pressure measurements. Then various anatomic and tissue properties are modified, resulting in a total of 11 variations of the model that are compared. The results show that an open segment of the central canal and a stiff pia (relative to the cord) both increase the radial pressure gradients and enhance interstitial fluid flow in the central canal. The anterior median fissure, anisotropic permeability of the white matter, and Poisson ratio play minor roles.


Subject(s)
Cervical Cord/physiology , Gray Matter/physiology , Models, Biological , Pia Mater/physiology , Syringomyelia/pathology , White Matter/physiology , Animals , Arnold-Chiari Malformation/complications , Arnold-Chiari Malformation/pathology , Cerebrospinal Fluid Pressure , Cervical Vertebrae/physiology , Disease Models, Animal , Extracellular Fluid/physiology , Imaging, Three-Dimensional , Movement , Sheep , Syringomyelia/complications
3.
J Biomech ; 44(16): 2826-32, 2011 Nov 10.
Article in English | MEDLINE | ID: mdl-21924724

ABSTRACT

In experiments turbulence has previously been shown to occur in intracranial aneurysms. The effects of turbulence induced oscillatory wall stresses could be of great importance in understanding aneurysm rupture. To investigate the effects of turbulence on blood flow in an intracranial aneurysm, we performed a high resolution computational fluid dynamics (CFD) simulation in a patient specific middle cerebral artery (MCA) aneurysm using a realistic, pulsatile inflow velocity. The flow showed transition to turbulence just after peak systole, before relaminarization occurred during diastole. The turbulent structures greatly affected both the frequency of change of wall shear stress (WSS) direction and WSS magnitude, which reached a maximum value of 41.5Pa. The recorded frequencies were predominantly in the range of 1-500Hz. The current study confirms, through properly resolved CFD simulations that turbulence can occur in intracranial aneurysms.


Subject(s)
Blood Pressure , Computer Simulation , Intracranial Aneurysm/physiopathology , Models, Cardiovascular , Pulsatile Flow , Stress, Physiological , Blood Flow Velocity , Female , Humans , Hydrodynamics , Intracranial Aneurysm/pathology , Male
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