Modulated turbulent convection: a benchmark model for large scale natural flows driven by diurnal heating
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68081731%3A_____%2F24%3A00587692" target="_blank" >RIV/68081731:_____/24:00587692 - isvavai.cz</a>
Nalezeny alternativní kódy
RIV/00216208:11320/24:10494313
Výsledek na webu
<a href="https://www.nature.com/articles/s41598-024-66882-5" target="_blank" >https://www.nature.com/articles/s41598-024-66882-5</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1038/s41598-024-66882-5" target="_blank" >10.1038/s41598-024-66882-5</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Modulated turbulent convection: a benchmark model for large scale natural flows driven by diurnal heating
Popis výsledku v původním jazyce
Our life is strongly affected by turbulent convective flows, driven by time-dependent thermal forcing, especially diurnal heating of the Earth’s surface by the Sun. In a laboratory experiment, we investigate their analogues: We study complex and extraordinary properties of turbulent buoyancy driven flows generated due to periodic modulation of the temperature of the plates of a Rayleigh–Bénard cell, with amplitudes both smaller and larger than either the positive or negative mean temperature difference between the top and bottom. We probe the turbulent flow of our working fluid – cryogenic helium gas – using temperature sensors placed in the cell interior and embedded in its plates. We discuss spatial and temporal structure of the heat flow, generalize validity of Nusselt versus Rayleigh number scaling Nu ∝ Raγ with γ≈1/3 at very high Ra for modulated convection and argue that this system represents a benchmark model which helps us understand the energy budget of ocean currents or weather formation on Earth subject to diurnal Sun heating as well as similar natural flows on Earth-like planets.
Název v anglickém jazyce
Modulated turbulent convection: a benchmark model for large scale natural flows driven by diurnal heating
Popis výsledku anglicky
Our life is strongly affected by turbulent convective flows, driven by time-dependent thermal forcing, especially diurnal heating of the Earth’s surface by the Sun. In a laboratory experiment, we investigate their analogues: We study complex and extraordinary properties of turbulent buoyancy driven flows generated due to periodic modulation of the temperature of the plates of a Rayleigh–Bénard cell, with amplitudes both smaller and larger than either the positive or negative mean temperature difference between the top and bottom. We probe the turbulent flow of our working fluid – cryogenic helium gas – using temperature sensors placed in the cell interior and embedded in its plates. We discuss spatial and temporal structure of the heat flow, generalize validity of Nusselt versus Rayleigh number scaling Nu ∝ Raγ with γ≈1/3 at very high Ra for modulated convection and argue that this system represents a benchmark model which helps us understand the energy budget of ocean currents or weather formation on Earth subject to diurnal Sun heating as well as similar natural flows on Earth-like planets.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10305 - Fluids and plasma physics (including surface physics)
Návaznosti výsledku
Projekt
<a href="/cs/project/GC21-06012J" target="_blank" >GC21-06012J: Efekty narušení Oberbeck-Boussinesquovy aproximace v turbulentní konvekci za vysokých Rayleighových čísel v kryogenním héliu</a><br>
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2024
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Scientific Reports
ISSN
2045-2322
e-ISSN
2045-2322
Svazek periodika
14
Číslo periodika v rámci svazku
1
Stát vydavatele periodika
DE - Spolková republika Německo
Počet stran výsledku
9
Strana od-do
15987
Kód UT WoS článku
001270506400049
EID výsledku v databázi Scopus
2-s2.0-85198052955