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Pemex (Mexico)

Mexico

1 paper here5 citations across 1
fields
  • astro-ph.SR1
ROR 040ek4035OpenAlex

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most citedTime-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT

5 citations

researchers with a paper here
  • A. Lani1 · h 13
  • B. Schmieder1 · h 5
  • D. Sorokina1 · h 2
  • Fan Zhang1 · h 1
  • Haopeng Wang1 · h 3
  • Hyun-jin Jeong1 · h 2
  • L. Linan1 · h 4
  • N. Mahdi1 · h 1
  • S. Poedts1 · h 5
  • T. Baratashvili1 · h 7
  • Yucong Li1 · h 2
collaborating institutions
  • Centre National de la Recherche ScientifiqueFR1 paper
  • KU LeuvenBE1 paper
  • Kyung Hee UniversityKR1 paper
  • LIRA - Laboratoire d'instrumentation et de recherche en astrophysiqueFR1 paper
  • Maria Curie-Skłodowska UniversityPL1 paper
  • National Space Science CenterCN1 paper
  • Observatoire de ParisFR1 paper
  • University of GlasgowGB1 paper
  • University of OsloNO1 paper
  • Von Karman Institute for Fluid DynamicsBE1 paper

1 paper

astro-ph.SR2026★ 5 cited

Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT

Haopeng Wang, Stefaan Poedts, Andrea Lani +8

Time-evolving MHD coronal models deliver more realistic results than traditional quasi-steady-state models. The fully implicit time-evolving coronal model COCONUT performs efficien…

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