EGU24-16958, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-16958
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The Challenge of Non-Markovian Energy Balance Models in Climate

Nicholas Wynn Watkins1,2, Raphael Calel3, Sandra Chapman2,4,5, Aleksei Chechkin6,7,8, Rainer Klages9,10, and David Stainforth1,2
Nicholas Wynn Watkins et al.
  • 1CFSA, University of Warwick, Coventry, United Kingdom of Great Britain – England, Scotland, Wales (nickwatkins62@fastmail.com)
  • 2Grantham Research Institute on Climate Change and the Environment, LSE, UK
  • 3McCourt School of Public Policy, Georgetown University, USA
  • 4Department of Mathematics and Statistics, University of Tromsø, Norway.
  • 5International Space Science Institute, Bern, Switzerland
  • 6Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam-Golm, Germany
  • 7Faculty of Pure and Applied Mathematics, Hugo Steinhaus Center, Wrocław University of Science and Technology, Wyspianskiego 27, 50-370 Wrocław, Poland
  • 8Akhiezer Institute for Theoretical Physics National Science Center “Kharkiv Institute of Physics and Technology", 61108 Kharkiv, Ukraine
  • 9School of Mathematical Sciences, Centre for Complex Systems, Queen Mary University of London, Mile End Road, London E1 4NS, UK.
  • 10London Mathematical Laboratory, 8 Margravine Gardens, London W6 8RH, UK

Hasselmann’s paradigm, introduced in 1976 and recently honoured with the Nobel Prize, can, like many key innovations in the sciences of climate and complexity, be understood on several different levels, both technical and conceptual. It can be seen as a mathematical technique to add stochastic variability into pioneering energy balance models (EBMs) of Budyko and Sellers. On a more conceptual level, it used the mathematics  of Brownian motion to provide an  abstract superstructure linking slow climate variability to fast weather fluctuations, in a context broader than EBMs, leading Hasselmann to posit the need for negative feedback in climate modelling.

Hasselmann's paradigm itself has much still to offer us [e.g. Calel et al, Naure Communications, 2020], but naturally, since the 1970s a number of newer developments have built on his pioneering ideas. One important one has been the development of a rigorous mathematical hierarchy that embeds Hasselmann-type models in the more comprehensive Mori-Zwanzig (MZ) framework  (e.g.  Lucarini and Chekroun, Nature Reviews Physics, 2023). Another has been the interest in long range memory in stochastic EBMs, notably Lovejoy et al’s Fractional Energy Balance Equation [FEBE, discussed in this week’s Short Course SC5.15 ]. These have a memory with slower decay and thus longer range than the exponential form seen in Hasselmann’s EBM. My presentation [based on Watkins et al, in review at Chaos] attempts to build a bridge between MZ-based extensions of  Hasselmann, and the fractional derivative-based FEBE model.  I will argue that the Mori-Kubo overdamped Generalised Langevin Equation, as widely used in statistical mechanics, suggests the form of a relatively simple stochastic EBM with memory for the global temperature anomaly, and will discuss how this relates to FEBE.

How to cite: Watkins, N. W., Calel, R., Chapman, S., Chechkin, A., Klages, R., and Stainforth, D.: The Challenge of Non-Markovian Energy Balance Models in Climate, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-16958, https://doi.org/10.5194/egusphere-egu24-16958, 2024.

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