1.4k citations
- A. Pouquet2 profiles68 · h 62
- S. McIntosh60 · h 47
- T. Metcalfe2 profiles53 · h 54
- P. Mininni50 · h 47
- W. Chaplin2 profiles41 · h 81
- J. Christensen-Dalsgaard3 profiles39 · h 85
- P. Judge36 · h 35
- S. Mathur3 profiles36 · h 64
- R. Casini2 profiles35 · h 28
- Y. Elsworth2 profiles35 · h 64
- Yuhong Fan2 profiles35 · h 36
- H. Kjeldsen2 profiles34 · h 77
- NSF NCAR High Altitude ObservatoryUS515 papers
- Centre National de la Recherche ScientifiqueFR115 papers
- Instituto de Astrofísica de CanariasES105 papers
- University of Colorado BoulderUS101 papers
- Max Planck Institute for Solar System ResearchDE98 papers
- Lockheed Martin (United States)US70 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR66 papers
- National Solar ObservatoryUS63 papers
- Aarhus UniversityDK62 papers
- Center for Astrophysics Harvard & SmithsonianUS62 papers
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- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR59 papers
9 papers · 1 filter
Adapting Atmospheric Chemistry Components for Efficient GPU Accelerators
Christian Guzman Ruiz, Matthew Dawson, Mario C. Acosta +4
Atmospheric models demand a lot of computational power and solving the chemical processes is one of its most computationally intensive components. This work shows how to improve th…
Community Research Earth Digital Intelligence Twin (CREDIT)
John Schreck, Yingkai Sha, William Chapman +7
Recent advancements in artificial intelligence (AI) for numerical weather prediction (NWP) have significantly transformed atmospheric modeling. AI NWP models outperform traditional…
Intermittency assessed through a model of kurtosis-skewness relation in MHD in fast dynamo regimes
Yannick Ponty, Helene Politano, Annick Pouquet
Intermittency as it occurs in fast dynamos in the MHD framework is evaluated through the examination of relations between normalized moments at third order (skewness S) and fourth…
Observing the evolution of the Sun's global coronal magnetic field over eight months
Zihao Yang, Hui Tian, Steven Tomczyk +4
The magnetic field in the Sun's corona stores energy that can be released to heat the coronal plasma and drive solar eruptions. Measurements of the global coronal magnetic field ha…
On the intermittency of hot plasma loops in the solar corona
P. G. Judge, N. P. M. Kuin
A recent analysis has suggested that the heating of plasma loops in the solar corona depends not just on the Poynting flux but also on processes yet to be identified. This discover…
Improving ensemble extreme precipitation forecasts using generative artificial intelligence
Yingkai Sha, Ryan A. Sobash, David John Gagne
An ensemble post-processing method is developed to improve the probabilistic forecasts of extreme precipitation events across the conterminous United States (CONUS). The method com…