Three‐dimensional propagation effects near the Mid‐Atlantic Bight

1997 ◽  
Vol 102 (5) ◽  
pp. 3143-3143
Author(s):  
Kevin B. Smith ◽  
Ching‐Sang Chiu ◽  
James H. Miller ◽  
James F. Lynch ◽  
Glen G. Gawarkiewicz
2011 ◽  
Vol 129 (6) ◽  
pp. EL260-EL266 ◽  
Author(s):  
Linus Y. S. Chiu ◽  
Ying-Tsong Lin ◽  
Chi-Fang Chen ◽  
Timothy F. Duda ◽  
Brian Calder

1987 ◽  
Vol 82 (S1) ◽  
pp. S44-S44 ◽  
Author(s):  
Ding Lee ◽  
Paul D. Scully‐Power ◽  
George Botseas ◽  
William L. Siegmann

2002 ◽  
Vol 112 (2) ◽  
pp. 373-376 ◽  
Author(s):  
Kevin B. Smith ◽  
Chris W. Miller ◽  
Anthony F. D’Agostino ◽  
Brian Sperry ◽  
James H. Miller ◽  
...  

2007 ◽  
Vol 121 (5) ◽  
pp. 3126-3126
Author(s):  
Kristy A. Moore ◽  
James H. Miller ◽  
Gopu R. Potty ◽  
James F. Lynch ◽  
Arthur Newhall

2019 ◽  
Vol 870 ◽  
pp. 1-4 ◽  
Author(s):  
R. J. Poole

Whereas the flow of simple single-phase Newtonian fluids tends to become more complex as the characteristic length scale in the problem (and hence the Reynolds number) increases, for complex elastic fluids such as dilute polymer solutions the opposite holds true. Thus small-scale, so-called ‘microfluidic’ flows of complex fluids can exhibit rich dynamics in situations where the ‘equivalent’ flow of Newtonian fluids remains linear and predictable. In the recent study of Qin et al. (J. Fluid Mech., vol. 864, 2019, R2) of the flow of a dilute polymeric fluid past a $50~\unicode[STIX]{x03BC}\text{m}$ cylinder (in a $100\times 60~\unicode[STIX]{x03BC}\text{m}$ channel), a novel 3-D holographic particle velocimetry technique reveals the underlying complexity of the flow, including inherent three-dimensionality and symmetry breaking as well as strong upstream propagation effects via elastic waves.


1966 ◽  
Vol 25 ◽  
pp. 227-229 ◽  
Author(s):  
D. Brouwer

The paper presents a summary of the results obtained by C. J. Cohen and E. C. Hubbard, who established by numerical integration that a resonance relation exists between the orbits of Neptune and Pluto. The problem may be explored further by approximating the motion of Pluto by that of a particle with negligible mass in the three-dimensional (circular) restricted problem. The mass of Pluto and the eccentricity of Neptune's orbit are ignored in this approximation. Significant features of the problem appear to be the presence of two critical arguments and the possibility that the orbit may be related to a periodic orbit of the third kind.


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