Lagrangian analysis of the formation and mass transport of compressible vortex rings generated by a shock tube

2020 ◽  
Author(s):  
Haiyan Lin ◽  
Yang Xiang ◽  
Hong Liu ◽  
Bin Zhang
Author(s):  
Naitoh Takashi ◽  
Okura Nobuyuki ◽  
Okude Muneshige ◽  
Sumitomo Osamu
Keyword(s):  

2021 ◽  
Vol 33 (9) ◽  
pp. 096105
Author(s):  
Sajag Poudel ◽  
Lakshmana Chandrala ◽  
Debopam Das ◽  
Ashoke De

2011 ◽  
Vol 77 (775) ◽  
pp. 557-567 ◽  
Author(s):  
Takashi NAITOH ◽  
Nobuyuki OKURA ◽  
Muneshige OKUDE ◽  
Yusuke UTSUMI

2020 ◽  
Vol 61 (3) ◽  
Author(s):  
Liang Qin ◽  
Yang Xiang ◽  
Haiyan Lin ◽  
Hong Liu
Keyword(s):  

2013 ◽  
Vol 45 (2) ◽  
pp. 025506 ◽  
Author(s):  
T Murugan ◽  
S De ◽  
C L Dora ◽  
D Das ◽  
P Prem Kumar

2014 ◽  
Vol 9 (3) ◽  
pp. JFST0060-JFST0060
Author(s):  
Takashi NAITOH ◽  
Nobuyuki OKURA ◽  
Osamu SUMITOMO
Keyword(s):  

Fluids ◽  
2021 ◽  
Vol 6 (12) ◽  
pp. 428
Author(s):  
Ghassan Maraouch ◽  
Lyes Kadem

The formation of vortex rings at valve leaflets during ventricular inflow has been a topic of interest for many years. It is generally accepted nowadays that the purpose of vortex rings is to conserve energy, reduce the workload on the heart, and minimize particle residence time. We investigated these claims by testing three different levels of annulus angle for the mitral valve: a healthy case, a slightly angled case (20°), and a highly angled case (46°). Circulation was determined to be reversed in the non-healthy case, with a dominant counterclockwise rotation instead of clockwise. Viscous energy dissipation was highest in the slightly angled case, followed by the healthy case and then the highly angled case. A Lagrangian analysis demonstrated that the healthy case resulted in the least amount of stasis, requiring eight cardiac cycles to evacuate 99% of initial ventricle volume compared to the 16 and 13 cardiac cycles required by the slightly angled and highly angled cases, respectively.


1979 ◽  
Vol 44 ◽  
pp. 349-355
Author(s):  
R.W. Milkey

The focus of discussion in Working Group 3 was on the Thermodynamic Properties as determined spectroscopically, including the observational techniques and the theoretical modeling of physical processes responsible for the emission spectrum. Recent advances in observational techniques and theoretical concepts make this discussion particularly timely. It is wise to remember that the determination of thermodynamic parameters is not an end in itself and that these are interesting chiefly for what they can tell us about the energetics and mass transport in prominences.


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