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.
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Research output: Contribution to Journal/Magazine › Comment/debate › peer-review
Research output: Contribution to Journal/Magazine › Comment/debate › peer-review
}
TY - JOUR
T1 - Future Directions for Whole Atmosphere Modelling
T2 - Developments in the context of space weather
AU - Jackson, David R.
AU - Fuller-Rowell, T.J.
AU - Griffin, D. J.
AU - Griffith, M. J.
AU - Kelley, C. W.
AU - Marsh, D. R.
AU - Walach, Maria
N1 - 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.
PY - 2019/9/1
Y1 - 2019/9/1
N2 - 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.
AB - 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.
U2 - 10.1029/2019SW002267
DO - 10.1029/2019SW002267
M3 - Comment/debate
VL - 17
SP - 1342
EP - 1350
JO - Space Weather
JF - Space Weather
SN - 1539-4956
IS - 9
ER -