Home > Research > Publications & Outputs > Future Directions for Whole Atmosphere Modelling

Research

Associated organisational unit

Electronic data

  • accepted_manuscript

    Rights statement: Accepted for publication in Space Weather. Copyright 2019 American Geophysical Union. Further reproduction or electronic distribution is not permitted This is the peer reviewed version of the following article: Jackson, D. R., Fuller‐Rowell, T. J., Griffin, D. J., Griffith, M. J., Kelly, C. W., Marsh, D. R., & Walach, M.‐T. ( 2019). Future Directions for Whole Atmosphere Modelling: Developments in the context of space weather. Space Weather, 17. https://doi.org/10.1029/2019SW002267 which has been published in final form at https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2019SW002267 This article may be used for non-commercial purposes in accordance With Wiley Terms and Conditions for self-archiving. © 2019 American Geophysical Union. All rights reserved.

    Accepted author manuscript, 4.17 MB, PDF document

    Available under license: CC BY-NC: Creative Commons Attribution-NonCommercial 4.0 International License

Links

Text available via DOI:

View graph of relations

Future Directions for Whole Atmosphere Modelling: Developments in the context of space weather

Research output: Contribution to Journal/Magazine › Comment/debate › peer-review

Published
  • David R. Jackson
  • T.J. Fuller-Rowell
  • D. J. Griffin
  • M. J. Griffith
  • C. W. Kelley
  • D. R. Marsh
  • Maria Walach
Close
More...
<mark>Journal publication date</mark>1/09/2019
<mark>Journal</mark>Space Weather
Issue number9
Volume17
Number of pages9
Pages (from-to)1342-1350
Publication StatusPublished
Early online date30/08/19
<mark>Original language</mark>English

Abstract

Coupled Sun‐to‐Earth models represent a key part of the future development of space weather forecasting. With respect to predicting the state of the thermosphere and ionosphere, there has been a recent paradigm shift; it is now clear that any self‐respecting model of this region needs to include some representation of forcing from the lower atmosphere, as well as solar and geomagnetic forcing. Here we assess existing modeling capability and set out a roadmap for the important next steps needed to ensure further advances. These steps include a model verification strategy, analysis of the impact of non‐hydrostatic dynamical cores, and a cost‐benefit analysis of model chemistry for weather and climate applications.

Bibliographic note

Add correct epub date when known Accepted for publication in Space Weather. Copyright 2019 American Geophysical Union. Further reproduction or electronic distribution is not permitted This is the peer reviewed version of the following article: Jackson, D. R., Fuller‐Rowell, T. J., Griffin, D. J., Griffith, M. J., Kelly, C. W., Marsh, D. R., & Walach, M.‐T. ( 2019). Future Directions for Whole Atmosphere Modelling: Developments in the context of space weather. Space Weather, 17. https://doi.org/10.1029/2019SW002267 which has been published in final form at https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2019SW002267 This article may be used for non-commercial purposes in accordance With Wiley Terms and Conditions for self-archiving. © 2019 American Geophysical Union. All rights reserved.

Related activities