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Solar physics: Weather of the magnetic Sun

Stephane Mathis 1, 2, *
* Corresponding author
1 AIM (UMR_7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation
2 IRFU - Institut de Recherches sur les lois Fondamentales de l'Univers
Abstract : The Sun is a magnetically active rotating star. Simultaneous observations with the STEREO and SDO space missions reveal solar analogues of planetary Rossby waves that will help forecast space weather.
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Journal articles
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https://hal-cea.archives-ouvertes.fr/cea-01887617
Contributor : Bruno Savelli <>
Submitted on : Thursday, October 4, 2018 - 11:37:00 AM
Last modification on : Saturday, April 11, 2020 - 2:17:31 AM

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CEA | CNRS | UNIV-PARIS7 | IRFU-AIM | CEA-UPSAY | DSM-IRFU | INSU | USPC | UNIV-PARIS-SACLAY | CEA-DRF | UNIV-PARIS | UP-SCIENCES

Citation

Stephane Mathis. Solar physics: Weather of the magnetic Sun. Nature Astronomy, Nature Publishing Group, 2017, 1 (4), pp.0096. ⟨10.1038/s41550-017-0096⟩. ⟨cea-01887617⟩

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