EGU23-15646, updated on 26 Feb 2023
https://doi.org/10.5194/egusphere-egu23-15646
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Characterization of Mediterranean large-scale atmospheric circulation based on Jenkinson-Collison Weather Type classification.

Juan Antonio Fernández-Granja1, Ana Casanueva2,3, Joaquín Bedia2,3, Swen Brands4, and Jesús Fernández1
Juan Antonio Fernández-Granja et al.
  • 1Meteorology Group, Instituto de Física de Cantabria (IFCA), Universidad de Cantabria-CSIC, 39005 Santander, Spain (juan.fernandez@unican.es)
  • 2Dept. of Applied Mathematics and Computer Science (MACC), Universidad de Cantabria, 39005 Santander, Spain
  • 3Grupo de Meteorología y Computación, Universidad de Cantabria, Unidad Asociada al CSIC, Santander, 39005, Spain.
  • 4MeteoGalicia, Consellería de Medio Ambiente, Territorio y Vivienda - Xunta de Galicia, Santiago de Compostela, Spain

The evaluation of new generations of global climate models (GCMs) with respect to their large-scale circulation features is crucial for model development and has recently been brought into focus by the downscaling community, interested in the suitability of GCMs for downscaling purposes. In such evaluation experiments, additional uncertainties emerge from differences among the reference datasets used for evaluation, typically reanalyses. In this context, weather typing techniques are a useful tool for the classification of the full diversity of data into a few recurrent patterns that can serve as objective characterizations of either global or regional atmospheric circulation. A well-known weather typing classification algorithm is the Jenkinson-Collison Weather Type (JC-WT, Jenkinson and Collison 1977) approach. Although the methodology was originally developed for the British Isles (Lamb, 1972), the JC-WT approach can in principle be applied to any mid-to-high latitude region (Jones et al, 2013). Fernandez-Granja et al (2023) extended the limits of applicability from 23.5º to 80º latitude on both hemispheres, but the suitability of the method is questionable for certain seasons over some areas of the globe, such as the Mediterranean region in summer.

In this study, we first explore the applicability of the JC classification over the Mediterranean by linking the JC-WTs with main northern hemisphere teleconnection indices and blocking conditions. Further, the diversity of JC-WTs and occurrence of the unclassified type are used to examine the suitability of the method. Results show that the application of the JC-WT classification is physically meaningful in large parts of the domain. Secondly, fundamental characteristics of the JC-WTs such as transition probabilities between consecutive types and persistence of the dominant JC-WTs (number of time-steps staying in the same type) obtained for five different reanalyses are compared. Important differences among reanalyses are found, especially in summer, which may bring additional uncertainties when the method is used in model evaluation experiments. 

References:

Fernández-Granja, J. A., Brands, S., Bedia, J., et al (2023) Exploring the limits of the Jenkinson–Collison weather types classification scheme: a global assessment based on various reanalyses. Climate Dynamics. DOI: 10.1007/s00382-022-06658-7

Jenkinson A., Collison F. (1977) An initial climatology of gales over the north sea. synoptic climatology branch memorandum. Meteorological Office, 62

Jones P.D., Harpham C., Briffa K.R. (2013) Lamb weather types derived from reanalysis products. International Journal of Climatology 33(5):1129–1139. DOI: 10.1002/joc.3498

Lamb H. (1972) British isles weather types and a register of daily sequence of circulation patterns 1861-1971. Meteorological Office, Geophysical Memoir 116:1–85

How to cite: Fernández-Granja, J. A., Casanueva, A., Bedia, J., Brands, S., and Fernández, J.: Characterization of Mediterranean large-scale atmospheric circulation based on Jenkinson-Collison Weather Type classification., EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-15646, https://doi.org/10.5194/egusphere-egu23-15646, 2023.