WaLSA Team
This article has multiple issues. Please help improve it or discuss these issues on the talk page. (Learn how and when to remove these messages)
|
| Formation | 2018 |
|---|---|
| Fields | Astrophysics |
| Members | 41 (February 2024) |
| Website | walsa |
The Waves in the Lower Solar Atmosphere (WaLSA) team is an international consortium that is focused on investigating wave activity in the Sun's lower atmosphere. The purpose of the group is to understand how magnetohydrodynamic (MHD) waves generated within the Sun's interior and lower atmosphere affect the dynamics and heating of its outer layers.[1]
The WaLSA team's research has been supported by organizations including the Research Council of Norway through the Rosseland Centre for Solar Physics,[2] the Royal Society,[3] and the International Space Science Institute.[4]
Research
The WaLSA team's research focuses on understanding various wave modes propagating through solar structures.[5] They have investigated the coupling mechanisms between different wave modes[6] and measured energy carried by MHD waves.[7]
References
- ^ "Magnetic Waves Explain Mystery of Sun's Puzzling Outer Layer". 22 January 2021.
- ^ "WaLSA: Waves in the Lower Solar Atmosphere - RoCS – Rosseland Centre for Solar Physics".
- ^ Jess, D. B.; Keys, P. H.; Stangalini, M.; Jafarzadeh, S. (February 8, 2021). "High-resolution wave dynamics in the lower solar atmosphere". Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences. 379 (2190). arXiv:2011.13940. Bibcode:2021RSPTA.37900169J. doi:10.1098/rsta.2020.0169. PMC 7780137. PMID 33342388.
- ^ "WaLSA: Waves in the Lower Solar Atmosphere at High Resolution – ISSI Team led by P. H. Keys".
- ^ "First detection of the magnetic field in solar vortices". 8 December 2021.
- ^ Stangalini, M.; Verth, G.; Fedun, V.; Aldhafeeri, A. A.; Jess, D. B.; Jafarzadeh, S.; Keys, P. H.; Fleck, B.; Terradas, J.; Murabito, M.; Ermolli, I.; Soler, R.; Giorgi, F.; MacBride, C. D. (28 February 2022). "Large scale coherent magnetohydrodynamic oscillations in a sunspot". Nature Communications. 13 (1): 479. Bibcode:2022NatCo..13..479S. doi:10.1038/s41467-022-28136-8. PMC 8789893. PMID 35079009.
- ^ Tziotziou, K.; Scullion, E.; Shelyag, S.; Steiner, O.; Khomenko, E.; Tsiropoula, G.; Canivete Cuissa, J. R.; Wedemeyer, S.; Kontogiannis, I.; Yadav, N.; Kitiashvili, I. N.; Skirvin, S. J.; Dakanalis, I.; Kosovichev, A. G.; Fedun, V. (28 February 2022). "Vortex Motions in the Solar Atmosphere". Space Science Reviews. 219 (1): 1. doi:10.1007/s11214-022-00946-8. PMC 9823109. PMID 36627929.
Content Disclaimer
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.
- The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
- There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
- It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
- Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
- Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.