Estimating the blood velocity vector using aperture domain data

Author(s):  
Shun-Li Wang ◽  
Meng-Lin Li ◽  
Pai-Chi Li
2019 ◽  
Vol 45 (7) ◽  
pp. 1691-1707 ◽  
Author(s):  
Anne E.C.M. Saris ◽  
Hendrik H.G. Hansen ◽  
Stein Fekkes ◽  
Jan Menssen ◽  
Maartje M. Nillesen ◽  
...  

2012 ◽  
pp. 211-221 ◽  
Author(s):  
Valentin A. Burov ◽  
Oleg V. Matveev ◽  
Semen N. Evtukhov ◽  
Olga D. Rumyantseva

2000 ◽  
Vol 39 (02) ◽  
pp. 175-178 ◽  
Author(s):  
K. Takehara ◽  
T. Yamamoto ◽  
R. Hashimoto ◽  
H. Nakamoto ◽  
F. Kajiya ◽  
...  

Abstract:We have evaluated rat glomerular microcirculation under in-vivo condition with an intravital videomicroscope. To measure erythrocyte velocities, a line segment was set along the glomerular capillaries in time-sequential videotaped images and then a spatiotemporal image was constructed along that segment. The angle of striped pattern in the spatio-temporal image which reflects the erythrocyte velocity, was estimated to compute erythrocyte velocity vector mapping. We found that erythrocyte velocities in rat glomeruli were significantly faster in diabetic rats than in control rats (p <0.05). In conclusion, we have succeeded in quantitatively evaluating the in-vivo renal microcirculation with our videomicroscope system and by spatiotemporal image analyzing method.


Author(s):  
Stefano Ricci ◽  
Alessandro Ramalli ◽  
Luca Bassi ◽  
Enrico Boni ◽  
Piero Tortoli

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1999 ◽  
Vol 45 (151) ◽  
pp. 533-538 ◽  
Author(s):  
Niels Reeh ◽  
Søren Nørvang Madsen ◽  
Johan Jakob Mohr

AbstractUntil now, an assumption of surface-parallel glacier flow has been used to express the vertical velocity component in terms of the horizontal velocity vector, permitting all three velocity components to be determined from synthetic aperture radar interferometry. We discuss this assumption, which neglects the influence of the local mass balance and a possible contribution to the vertical velocity arising if the glacier is not in steady state. We find that the mass-balance contribution to the vertical surface velocity is not always negligible as compared to the surface-slope contribution. Moreover, the vertical velocity contribution arising if the ice sheet is not in steady state can be significant. We apply the principle of mass conservation to derive an equation relating the vertical surface velocity to the horizontal velocity vector. This equation, valid for both steady-state and non-steady-state conditions, depends on the ice-thickness distribution. Replacing the surface-parallel-flow assumption with a correct relationship between the surface velocity components requires knowledge of additional quantities such as surface mass balance or ice thickness.


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