Construction of a computational non-planar curved tube model from MRI data

Author(s):  
T.A. Spirka ◽  
J.G. Myers ◽  
R.M. Setser ◽  
S.S. Halliburton ◽  
R.D. White ◽  
...  
Keyword(s):  
1993 ◽  
Vol 59 (560) ◽  
pp. 1079-1086
Author(s):  
Yutaka Komai ◽  
Gen Yamazaki ◽  
Shohei Onishi ◽  
Kazuo Tanishita

10.1114/1.113 ◽  
1998 ◽  
Vol 26 (6) ◽  
pp. 944-954 ◽  
Author(s):  
Aland Santamarina ◽  
Erlend Weydahl ◽  
John M. Siegel, Jr. ◽  
James E. Moore, Jr.

2020 ◽  
Author(s):  
Keyword(s):  

2021 ◽  
pp. 1-23
Author(s):  
A. Wischnewski ◽  
M. Euler ◽  
S. Gümüs ◽  
B. Lohmann

2000 ◽  
Vol 411 ◽  
pp. 1-38 ◽  
Author(s):  
C. ROSS ETHIER ◽  
SUJATA PRAKASH ◽  
DAVID A. STEINMAN ◽  
RICHARD L. LEASK ◽  
GREGORY G. COUCH ◽  
...  

Numerical and experimental techniques were used to study the physics of flow separation for steady internal flow in a 45° junction geometry, such as that observed between two pipes or between the downstream end of a bypass graft and an artery. The three-dimensional Navier–Stokes equations were solved using a validated finite element code, and complementary experiments were performed using the photochromic dye tracer technique. Inlet Reynolds numbers in the range 250 to 1650 were considered. An adaptive mesh refinement approach was adopted to ensure grid-independent solutions. Good agreement was observed between the numerical results and the experimentally measured velocity fields; however, the wall shear stress agreement was less satisfactory. Just distal to the ‘toe’ of the junction, axial flow separation was observed for all Reynolds numbers greater than 250. Further downstream (approximately 1.3 diameters from the toe), the axial flow again separated for Re [ges ] 450. The location and structure of axial flow separation in this geometry is controlled by secondary flows, which at sufficiently high Re create free stagnation points on the model symmetry plane. In fact, separation in this flow is best explained by a secondary flow boundary layer collision model, analogous to that proposed for flow in the entry region of a curved tube. Novel features of this flow include axial flow separation at modest Re (as compared to flow in a curved tube, where separation occurs only at much higher Re), and the existence and interaction of two distinct three-dimensional separation zones.


2015 ◽  
Vol 118 (12) ◽  
pp. 1525-1532 ◽  
Author(s):  
Winfried Möller ◽  
Gülnaz Celik ◽  
Sheng Feng ◽  
Peter Bartenstein ◽  
Gabriele Meyer ◽  
...  

Recent studies showed that nasal high flow (NHF) with or without supplemental oxygen can assist ventilation of patients with chronic respiratory and sleep disorders. The hypothesis of this study was to test whether NHF can clear dead space in two different models of the upper nasal airways. The first was a simple tube model consisting of a nozzle to simulate the nasal valve area, connected to a cylindrical tube to simulate the nasal cavity. The second was a more complex anatomically representative upper airway model, constructed from segmented CT-scan images of a healthy volunteer. After filling the models with tracer gases, NHF was delivered at rates of 15, 30, and 45 l/min. The tracer gas clearance was determined using dynamic infrared CO2 spectroscopy and 81mKr-gas radioactive gamma camera imaging. There was a similar tracer-gas clearance characteristic in the tube model and the upper airway model: clearance half-times were below 1.0 s and decreased with increasing NHF rates. For both models, the anterior compartments demonstrated faster clearance levels (half-times < 0.5 s) and the posterior sections showed slower clearance (half-times < 1.0 s). Both imaging methods showed similar flow-dependent tracer-gas clearance in the models. For the anatomically based model, there was complete tracer-gas removal from the nasal cavities within 1.0 s. The level of clearance in the nasal cavities increased by 1.8 ml/s for every 1.0 l/min increase in the rate of NHF. The study has demonstrated the fast-occurring clearance of nasal cavities by NHF therapy, which is capable of reducing of dead space rebreathing.


Solar Physics ◽  
1982 ◽  
Vol 76 (1) ◽  
pp. 21-28 ◽  
Author(s):  
Horst Balthasar ◽  
Manfred Sch�ssler ◽  
Hubertus W�hl
Keyword(s):  

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