Applicability of Taylor's hypothesis in thermally driven turbulence

In this paper, we show that, in the presence of large-scale circulation (LSC), Taylor’s hypothesis can be invoked to deduce the energy spectrum in thermal convection using real-space probes, a popular experimental tool. We perform numerical simulation of turbulent convection in a cube and observe th...

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Main Authors: Abhishek Kumar, Mahendra K. Verma
Format: Article
Language:English
Published: The Royal Society 2018-01-01
Series:Royal Society Open Science
Subjects:
Online Access:https://royalsocietypublishing.org/doi/pdf/10.1098/rsos.172152
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author Abhishek Kumar
Mahendra K. Verma
author_facet Abhishek Kumar
Mahendra K. Verma
author_sort Abhishek Kumar
collection DOAJ
description In this paper, we show that, in the presence of large-scale circulation (LSC), Taylor’s hypothesis can be invoked to deduce the energy spectrum in thermal convection using real-space probes, a popular experimental tool. We perform numerical simulation of turbulent convection in a cube and observe that the velocity field follows Kolmogorov’s spectrum (k−5/3). We also record the velocity time series using real-space probes near the lateral walls. The corresponding frequency spectrum exhibits Kolmogorov’s spectrum (f−5/3), thus validating Taylor’s hypothesis with the steady LSC playing the role of a mean velocity field. The aforementioned findings based on real-space probes provide valuable inputs for experimental measurements used for studying the spectrum of convective turbulence.
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spelling doaj.art-5a56516495404784a8ae09b7d0d9ba7d2022-12-21T19:21:20ZengThe Royal SocietyRoyal Society Open Science2054-57032018-01-015410.1098/rsos.172152172152Applicability of Taylor's hypothesis in thermally driven turbulenceAbhishek KumarMahendra K. VermaIn this paper, we show that, in the presence of large-scale circulation (LSC), Taylor’s hypothesis can be invoked to deduce the energy spectrum in thermal convection using real-space probes, a popular experimental tool. We perform numerical simulation of turbulent convection in a cube and observe that the velocity field follows Kolmogorov’s spectrum (k−5/3). We also record the velocity time series using real-space probes near the lateral walls. The corresponding frequency spectrum exhibits Kolmogorov’s spectrum (f−5/3), thus validating Taylor’s hypothesis with the steady LSC playing the role of a mean velocity field. The aforementioned findings based on real-space probes provide valuable inputs for experimental measurements used for studying the spectrum of convective turbulence.https://royalsocietypublishing.org/doi/pdf/10.1098/rsos.172152turbulenceturbulent convection
spellingShingle Abhishek Kumar
Mahendra K. Verma
Applicability of Taylor's hypothesis in thermally driven turbulence
Royal Society Open Science
turbulence
turbulent convection
title Applicability of Taylor's hypothesis in thermally driven turbulence
title_full Applicability of Taylor's hypothesis in thermally driven turbulence
title_fullStr Applicability of Taylor's hypothesis in thermally driven turbulence
title_full_unstemmed Applicability of Taylor's hypothesis in thermally driven turbulence
title_short Applicability of Taylor's hypothesis in thermally driven turbulence
title_sort applicability of taylor s hypothesis in thermally driven turbulence
topic turbulence
turbulent convection
url https://royalsocietypublishing.org/doi/pdf/10.1098/rsos.172152
work_keys_str_mv AT abhishekkumar applicabilityoftaylorshypothesisinthermallydriventurbulence
AT mahendrakverma applicabilityoftaylorshypothesisinthermallydriventurbulence