Results 11 to 20 of about 14,504 (190)
A Statistical Shape Modeling Approach for the Derivation of a Data-Driven Geometry-Aware Lumped Arterial Stenosis Model. [PDF]
Int J Numer Method Biomed EngA data‐driven workflow for constructing a geometry‐aware lumped arterial stenosis model: Statistical shape modeling extracts geometry‐specific shape modes from synthetically generated coronary lesion geometries. Large‐scale 3D CFD simulations over varying Reynolds numbers yield the geometries their viscous (Kv) and inertial (Kt) loss coefficients. Then,
Hilhorst PLJ +6 more
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The proposition of analytical expression HM�(vP/S) in microindentation pile-up deformation mode
Fracture and Structural Integrity, 2022 In this article, the characteristic curves of microindentation measured on Cu99 were analyzed on the basis of the analytical expression proposed by Habibi et al. (J. Mater. Res, 2021, 36 (15): 3074-3085). The ratio of applied load to square displacement,
D.-E. Semsoum� +3 more
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Cuspy and fractured black hole shadows in a toy model with axisymmetry
European Physical Journal C: Particles and Fields, 2022 Cuspy shadow was first reported for hairy rotating black holes, whose metrics deviate significantly from the Kerr one. The non-smooth edge of the shadow is attributed to a transition between different branches of unstable but bounded orbits, known as the
Wei-Liang Qian +4 more
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Center-Symmetrical Object Detection Based on Gabor Wavelets
IEEE Access, 2020 Symmetry is an important visual characteristic in the image and can be used to identify real-world objects based on their geometrically balanced structures.
Yi Zhang +3 more
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Preferred sunspot longitudes: non-axisymmetry and differential rotation [PDF]
Astronomy & Astrophysics, 2005 As recently found, the distribution of sunspots is non-axisymmetric and spot group formation implies the existence of two persistent active longitudes separated by 180 degrees. Here we quantitatively study the non-axisymmetry of sunspot occurrence. In a dynamic reference frame inferred from the differential rotation law, the raw sunspot data show a ...
Usoskin, I. G. +2 more
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PT-axisymmetry for extraordinary field confinement [PDF]
SPIE Proceedings, 2017 Optical Parity-Time (PT-) symmetric systems support unusual properties when the symmetric coupling between internal modes is broken. We propose a new class of quasiperiodic PT-axisymmetric systems which lead to a simultaneous extraordinary field enhancement and localization at the symmetry center.
Botey Cumella, Muriel +3 more
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Probing Non-Axisymmetry with Proper Motions [PDF]
Symposium - International Astronomical Union, 1995 The potential of the Milky Way is almost certainly not axisymmetric: the centre is believed to be dominated by a bar, and beyond the solar radius some non-axisymmetric feature of the potential appears to warp the disk. There are grounds for believing that the outer potential is mildly elliptical. Sub mas yr–1 proper motions of objects that lie near the
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Black ripples, flowers and dumbbells at large D
Journal of High Energy Physics, 2020 We explore the rich phase space of singly spinning (both neutral and charged) black hole solutions in the large D limit. We find several ‘bumpy’ branches which are connected to multiple (concentric) black rings, and black Saturns. Additionally, we obtain
David Licht, Raimon Luna, Ryotaku Suzuki
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Recipe for a Saturn‐Like Dynamo
AGU Advances, 2021 The Cassini Grand Finale orbits provided detailed observations of Saturn’s internal magnetic field. Unique characteristics of the observed field, such as its axisymmetry and power spectrum, provide constraints on dynamo processes deep in Saturn’s ...
C. Yan, S. Stanley
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Measuring non-axisymmetry in spiral galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 1997 We present a method for measuring small deviations from axisymmetry of the potential of a filled gas disk. The method is based on a higher order harmonic expansion of the full velocity field of the disk. This expansion is made by first fitting a tilted-ring model to the velocity field of the gas disk and subsequently expanding the velocity field along ...
Schoenmakers, R.H.M. +2 more
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