Future directions for whole atmosphere modeling: Developments in the context of space weather

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 road map for the important next steps needed to ensure further advances. These steps include a model verification strategy, analysis of the impact of nonhydrostatic dynamical cores, and a cost-benefit analysis of model chemistry for weather and climate applications.

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Copyright 2019 American Geophysical Union.


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Author Jackson, David R.
Fuller‐Rowell, Tim J.
Griffin, Dan J.
Griffith, Matthew J.
Kelly, Christopher W.
Marsh, Daniel R.
Walach, Maria‐Theresia
Publisher UCAR/NCAR - Library
Publication Date 2019-09-11T00:00:00
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Topic Category geoscientificInformation
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Metadata Date 2023-08-18T18:09:52.887274
Metadata Record Identifier edu.ucar.opensky::articles:22813
Metadata Language eng; USA
Suggested Citation Jackson, David R., Fuller‐Rowell, Tim J., Griffin, Dan J., Griffith, Matthew J., Kelly, Christopher W., Marsh, Daniel R., Walach, Maria‐Theresia. (2019). Future directions for whole atmosphere modeling: Developments in the context of space weather. UCAR/NCAR - Library. http://n2t.net/ark:/85065/d7bc42pb. Accessed 18 June 2025.

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