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Adalberto Perez
Adalberto Perez
PhD Candidate
Verified email at kth.se
Title
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Year
Exploring the ultimate regime of turbulent rayleigh–bénard convection through unprecedented spectral-element simulations
N Jansson, M Karp, A Perez, T Mukha, Y Ju, J Liu, S Páll, E Laure, ...
Proceedings of the International Conference for High Performance Computing …, 2023
102023
Understanding the impact of synchronous, asynchronous, and hybrid in-situ techniques in computational fluid dynamics applications
Y Ju, A Perez, S Markidis, P Schlatter, E Laure
2022 IEEE 18th International Conference on e-Science (e-Science), 295-305, 2022
102022
Appraisal of cavity hot-wire probes for wall-shear-stress measurements
A Perez, R Örlü, A Talamelli, P Schlatter
Experiments in Fluids 63 (9), 151, 2022
72022
In-situ techniques on GPU-accelerated data-intensive applications
Y Ju, M Li, A Perez, L Bellentani, N Jansson, S Markidis, P Schlatter, ...
2023 IEEE 19th International Conference on e-Science (e-Science), 1-10, 2023
32023
Generating synthetic turbulence with vector autoregression of proper orthogonal decomposition time coefficients
R Stanly, S Du, D Xavier, A Perez, T Mukha, S Markidis, S Rezaeiravesh, ...
Journal of Fluid Mechanics 1000, A83, 2024
12024
Dynamic Resource Management for In-Situ Techniques Using MPI-Sessions
Y Ju, D Huber, A Perez, P Ulbl, S Markidis, P Schlatter, M Schulz, ...
European MPI Users' Group Meeting, 105-120, 2024
12024
Towards spectral-element large-scale simulations of turbulent Rayleigh-Bénardconvection in round cells
M Karp, A Perez, N Jansson, T Mukha, R Samuel, J Schumacher, ...
Bulletin of the American Physical Society, 2023
2023
Are measurements of fluctuating wall-shear stress with flush-mounted cavity hot-wires possible?
R Örlü, A Perez, A Alvisi, A Talamelli, P Schlatter
APS Division of Fluid Dynamics Meeting Abstracts, E08. 015, 2020
2020
Compression of Turbulence Time Series Data Using Gaussian Process Regression
A Perez, S Rezaeiravesh, J Yu, E Laure, S Markidis, P Schlatter
Available at SSRN 4966490, 0
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