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  Bistability in Radiatively Heated Melt Ponds

Yang, R., Howland, C., Liu, H.-R., Verzicco, R., & Lohse, D. (2023). Bistability in Radiatively Heated Melt Ponds. Physical Review Letters, 131(23): 234002. doi:10.1103/PhysRevLett.131.234002.

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PhysRevLett.131.234002.pdf (Publisher version), 806KB
 
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 Creators:
Yang, R., Author
Howland, C.J., Author
Liu, H.-R., Author
Verzicco, R., Author
Lohse, Detlef1, Author           
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1Max Planck Institute for Dynamics and Self-Organization, Max Planck Society, ou_2063285              

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 Abstract: Melting and solidification processes, intertwined with convective flows, play a fundamental role in geophysical contexts. One of these processes is the formation of melt ponds on glaciers, ice shelves, and sea ice. It is driven by solar radiation and is of great significance for Earth’s heat balance, as it significantly lowers the albedo. Through direct numerical simulations and theoretical analysis, we unveil a bistability phenomenon in the melt pond dynamics. As solar radiation intensity and the melt pond’s initial depth vary, an abrupt transition occurs: this tipping point transforms the system from a stable fully frozen state to another stable equilibrium state, characterized by a distinct melt pond depth. The physics of this transition can be understood within a heat flux balance model, which exhibits excellent agreement with our numerical results. Together with the Grossmann-Lohse theory for internally heated convection, the model correctly predicts the bulk temperature and the flow strength within the melt ponds, offering insight into the coupling of phase transitions with adjacent turbulent flows and the interplay between convective melting and radiation-driven processes.

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Language(s): eng - English
 Dates: 2023-12-072023
 Publication Status: Issued
 Pages: -
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 Rev. Type: Peer
 Identifiers: DOI: 10.1103/PhysRevLett.131.234002
 Degree: -

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Project name : MultiMelt
Grant ID : 101094492
Funding program : Horizon 2020 (H2020)
Funding organization : European Commission (EC)

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Title: Physical Review Letters
  Abbreviation : Phys. Rev. Lett.
Source Genre: Journal
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Publ. Info: Woodbury, N.Y. : American Physical Society
Pages: - Volume / Issue: 131 (23) Sequence Number: 234002 Start / End Page: - Identifier: ISSN: 0031-9007
CoNE: https://pure.mpg.de/cone/journals/resource/954925433406_1