Cookies

We use cookies to ensure that we give you the best experience on our website. You can change your cookie settings at any time. Otherwise, we'll assume you're OK to continue.

Email and Telephone Directory

Staff Profile

Dr Anthony Yeates

Personal web page

Level 2 Course Director, Lecturer in the Department of Mathematical Sciences

Contact Dr Anthony Yeates

Research Groups

Department of Mathematical Sciences

  • Computational Applied Mathematics
  • Numerical Analysis

Research Interests

  • Computational modelling of the Sun's large-scale magnetic field
  • Solar dynamo models
  • Topology and reconnection of 3D magnetic fields

Selected Publications

Journal papers: academic

  • Yeates, A.R. (2014). Coronal Magnetic Field Evolution from 1996 to 2012: Continuous Non-potential Simulations. Solar Physics 289(2): 631-648.
  • Chian, A. C.-L., Rempel, E. L., Aulanier, G., Schmieder, B., Shadden, S. C., Welsch, B. T. & Yeates, A. R. (2014). Detection of coherent structures in photospheric turbulent flows. The Astrophysical Journal 786(1): 51.
  • Yeates, A. R., Bianchi, F., Welsh, B. T. & Bushby, P. J. (2014). The coronal energy input from magnetic braiding. Astronomy & Astrophysics 564: A131.
  • Yeates, A.R. & Munoz-Jaramillo, A. (2013). Kinematic active region formation in a three-dimensional solar dynamo model. Monthly Notices of the Royal Astronomical Society 436(4): 3366-3379.
  • Schrijver, C.J., Title, A.M., Yeates, A.R. & DeRosa, M.L. (2013). Pathways of Large-scale Magnetic Couplings Between Solar Coronal Events. The Astrophysical Journal 773(2): 93.
  • Yeates, A.R. & Hornig, G. (2013). Unique topological characterization of braided magnetic fields. Physics of Plasmas 20(1): 012102.
  • Yeates, A. R. & Mackay, D. H. (2012). Chirality of high-latitude filaments over Solar Cycle 23. The Astrophysical Journal Letters 753: L34.
  • Yeates, A. R., Hornig, G. & Welsch, B. T. (2012). Lagrangian coherent structures in photospheric flows and their implications for coronal magnetic structure. Astronomy & Astrophysics 539: A1.
  • Mackay, D. H. & Yeates, A. R. (2012). The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models. Living Reviews in Solar Physics 9: 6.
  • Yeates, AR & Hornig, G (2011). A Generalized Flux Function for Three-dimensional Magnetic Reconnection. Physics of Plasmas 18(10): 102118.
  • Yeates, A. R. & Hornig, G. (2011). Dynamical constraints from field line topology in magnetic flux tubes. Journal of Physics A. Mathematical and Theoretical 44: 265501.
  • Wilmot-Smith, A. L., Pontin, D. I., Yeates, A. R. & Hornig, G. (2011). Heating of Braided Coronal Loops. Astronomy & Astrophysics 536: A67.
  • Munoz-Jaramillo, A., Nandy, D., Martens, P. C. H. & Yeates, A. R. (2010). A double-ring algorithm for modeling solar active regions: Unifying kinematic dynamo models and surface flux-transport simulations. The Astrophysical Journal 720: L20.
  • Yeates, A. R., Mackay, D. H., van Ballegooijen, A. A. & Constable, J. A. (2010). A non-potential model for the Sun's open magnetic flux. Journal of Geophysical Research 115: A09112.
  • Yeates, A. R., Attrill, G. D. R., Nandy, D., Mackay, D. H., Martens, P. C. H. & van Ballegooijen, A. A. (2010). Comparison of a global magnetic evolution model with observations of coronal mass ejections. The Astrophysical Journal 709: 1238.
  • Yeates, A. R., Constable, J. A. & Martens, P. C. H. (2010). Solar cycle variation of magnetic flux ropes in a quasi-static coronal evolution model. Solar Physics 263: 121.
  • Yeates, A. R., Hornig, G. & Wilmot-Smith, A. L. (2010). Topological constraints on magnetic relaxation. Physical Review Letters 105(8): 085002.
  • Yeates, A. R. & Mackay, D. H. (2009). Initiation of coronal mass ejections in a global evolution model. The Astrophysical Journal 699(2): 1024.
  • Yeates, A. R. & Mackay, D. H. (2009). Modelling the global solar corona III: Origin of the hemispheric pattern of filaments. Solar Physics 254: 77.
  • Yeates, A. R., Mackay, D. H. & van Ballegooijen, A. A. (2008). Evolution and distribution of current helicity in full-Sun simulations. The Astrophysical Journal 680: L165.
  • Yeates, A. R., Nandy, D. & Mackay, D. H. (2008). Exploring the physical basis of solar cycle predictions: Flux transport dynamics and persistence of memory in advection versus diffusion-dominated solar convection zones. The Astrophysical Journal 673(1): 544-556.
  • Yeates, A. R., Mackay, D. H. & van Ballegooijen, A. A. (2008). Modelling the global solar corona II: Coronal evolution and filament chirality comparison. Solar Physics 247(1): 103-121.
  • Mackay, D. H., Gaizauskas, V. & Yeates, A. R. (2008). Where do solar filaments form? Consequences for theoretical models. Solar Physics 248: 51.
  • Yeates, A. R., Mackay, D. H. & van Ballegooijen, A. A. (2007). Modelling the global solar corona filament chirality observations and surface simulations. Solar Physics 245: 87.

Show all publications

Supervises