Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
Juno Jupiter image

Andrew Wells

Associate Professor of Physical Climate Science

Research theme

  • Climate physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Ice and Fluid Dynamics
Andrew.Wells@physics.ox.ac.uk
Telephone: 01865 (2)82425
Robert Hooke Building, room F60
  • About
  • Publications

Optimal and hysteretic fluxes in alloy solidification: Variational principles and chimney spacing

(2010)

Authors:

Andrew J Wells, JS Wettlaufer, Steven A Orszag
More details from the publisher

Maximal Potential Energy Transport: A Variational Principle for Solidification Problems

PHYSICAL REVIEW LETTERS 105:25 (2010) ARTN 254502

Authors:

AJ Wells, JS Wettlaufer, SA Orszag
More details from the publisher
More details

Variations in Ocean Surface Temperature due to Near-Surface Flow: Straining the Cool Skin Layer

JOURNAL OF PHYSICAL OCEANOGRAPHY 39:11 (2009) 2685-2710

Authors:

Andrew J Wells, Claudia Cenedese, J Thomas Farrar, Christopher J Zappa
More details from the publisher

A geophysical-scale model of vertical natural convection boundary layers

Journal of Fluid Mechanics 609 (2008) 111-137

Authors:

AJ Wells, MG Worster

Abstract:

A model is developed for turbulent natural convection in boundary layers formed next to isothermal vertical surfaces. A scaling analysis shows that the flow can be described by plume equations for an outer turbulent region coupled to a resolved near-wall laminar flow. On the laboratory scale, the inner layer is dominated by its own buoyancy and the Nusselt number scales as the one-third power of the Rayleigh number (Nu ∝ Raz1/3). This gives a constant heat flux, consistent with previous experimental and theoretical studies. On larger geophysical scales the buoyancy is strongest in the outer layer and the laminar layer is driven by the shear imposed on it. The predicted heat transfer correlation then has the Nusselt number proportional to the one-half power of Rayleigh number (Nu ∝ Raz1/2) so that a larger heat flux is predicted than might be expected from an extrapolation of laboratory-scale results. The criteria for transitions between flow regimes are consistent with a hierarchy of instabilities of the near-wall laminar flow, with a buoyancy-driven instability operating on the laboratory scale and a shear-driven instability operating on geophysical scales. © 2008 Cambridge University Press.
More details from the publisher
More details

A stochastic model for the turbulent ocean heat flux under Arctic sea ice

Physical Review E: Statistical, Nonlinear, and Soft Matter Physics American Physical Society

Authors:

Srikanth Toppaladoddi, Andrew Wells

Abstract:

The physics of planetary climate features a variety of complex systems that are challenging to model as they feature turbulent flows. A key example is the heat flux from the upper ocean to the underside of sea ice which provides a key contribution to the evolution of the Arctic sea ice cover. Here, we develop a model of the turbulent ice-ocean heat flux using coupled ordinary stochastic differential equations to model fluctuations in the vertical velocity and temperature in the Arctic mixed layer. All the parameters in the model are determined from observational data. A detailed comparison between the model results and measurements made during the Surface Heat Budget of the Arctic Ocean (SHEBA) project reveals that the model is able to capture the probability density functions (PDFs) of velocity, temperature and heat flux fluctuations. Furthermore, we show that the temperature in the upper layer of the Arctic ocean can be treated as a passive scalar during the whole year of SHEBA measurements. The stochastic model developed here provides a computationally inexpensive way to compute an observationally consistent PDF of this heat flux, and has implications for its parametrization in regional and global climate models.
Details from ORA
More details from the publisher
More details

Pagination

  • First page First
  • Previous page Prev
  • Page 1
  • Page 2
  • Page 3
  • Page 4
  • Page 5
  • Page 6
  • Page 7
  • Current page 8
  • Page 9
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet