TY - JOUR
T1 - Turbulent Convection at Very High Rayleigh Numbers and the Weakly Nonlinear Theory
AU - Sreenivasan, Katepalli R.
AU - Niemela, Joseph J.
N1 - Publisher Copyright:
© 2023 by the authors.
PY - 2023/5
Y1 - 2023/5
N2 - To provide insights into the challenging problem of turbulent convection, Jack Herring used a greatly truncated version of the complete Boussinesq equations containing only one horizontal wavenumber. In light of later observations of a robust large-scale circulation sweeping through convecting enclosures at high Rayleigh numbers, it is perhaps not an implausible point of view from which to reexamine high-Rayleigh-number data. Here we compare past experimental data on convective heat transport at high Rayleigh numbers with predictions from Herring’s model and, in fact, find excellent agreement. The model has only one unknown parameter compared to the two free parameters present in the lowest-order least-squares power-law fit. We discuss why the underlying simplistic physical picture, meant to work at Rayleigh numbers slightly past the critical value of a few thousand, is consistent with the data when the single free parameter in it is revised, over some eleven decades of the Rayleigh number—stretching from about a million to about (Formula presented.).
AB - To provide insights into the challenging problem of turbulent convection, Jack Herring used a greatly truncated version of the complete Boussinesq equations containing only one horizontal wavenumber. In light of later observations of a robust large-scale circulation sweeping through convecting enclosures at high Rayleigh numbers, it is perhaps not an implausible point of view from which to reexamine high-Rayleigh-number data. Here we compare past experimental data on convective heat transport at high Rayleigh numbers with predictions from Herring’s model and, in fact, find excellent agreement. The model has only one unknown parameter compared to the two free parameters present in the lowest-order least-squares power-law fit. We discuss why the underlying simplistic physical picture, meant to work at Rayleigh numbers slightly past the critical value of a few thousand, is consistent with the data when the single free parameter in it is revised, over some eleven decades of the Rayleigh number—stretching from about a million to about (Formula presented.).
KW - heat transport
KW - high-Rayleigh-number asymptote
KW - turbulent convection
KW - ultimate state of convection
UR - http://www.scopus.com/inward/record.url?scp=85160671311&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85160671311&partnerID=8YFLogxK
U2 - 10.3390/atmos14050826
DO - 10.3390/atmos14050826
M3 - Article
AN - SCOPUS:85160671311
SN - 2073-4433
VL - 14
JO - Atmosphere
JF - Atmosphere
IS - 5
M1 - 826
ER -