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| science:publications:solar [2025/04/14 11:02] – etienne | science:publications:solar [2026/02/10 16:04] (current) – etienne |
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| === Refereed publications === | === Refereed publications === |
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| == 2020s == | == 2020's == |
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| - Karki G., Schmieder B., Devi P., Chandra R., Labrosse N., Joshi R., Gelly B.; //[[ https://ui.adsabs.harvard.edu/abs/2024arXiv241209206K | Magnetic Reconnection between a Solar Jet and a Filament Channel]]//; arXiv e-prints, arXiv:2412.09206, (2024). DOI:10.48550/arXiv.2412.09206 \\ | - Karki G., Schmieder B., Devi P., Chandra R., Labrosse N., Joshi R., Gelly B.; //[[ https://ui.adsabs.harvard.edu/abs/2024arXiv241209206K | Magnetic Reconnection between a Solar Jet and a Filament Channel]]//; arXiv e-prints, arXiv:2412.09206, (2024). DOI:10.48550/arXiv.2412.09206 \\ |
| - Mackay D. H., Schmieder B., López Ariste A., Su Y.; //[[ https://ui.adsabs.harvard.edu/abs/2020A&A...637A...3M | Modelling and observations: Comparison of the magnetic field properties in a prominence]]//; Astronomy and Astrophysics, 637, A3, (2020). DOI:10.1051/0004-6361/201936656 \\ | - Mackay D. H., Schmieder B., López Ariste A., Su Y.; //[[ https://ui.adsabs.harvard.edu/abs/2020A&A...637A...3M | Modelling and observations: Comparison of the magnetic field properties in a prominence]]//; Astronomy and Astrophysics, 637, A3, (2020). DOI:10.1051/0004-6361/201936656 \\ |
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| == 2010s == | == 2010's == |
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| - Kalewicz T., Bommier V.; //[[ https://ui.adsabs.harvard.edu/abs/2019A&A...629A.138K | Magnetic field vector ambiguity resolution in a quiescent prominence observed on two consecutive days ]]//; Astronomy and Astrophysics, 629, A138, (2019). DOI: 10.1051/0004-6361/201935488 \\ | - Kalewicz T., Bommier V.; //[[ https://ui.adsabs.harvard.edu/abs/2019A&A...629A.138K | Magnetic field vector ambiguity resolution in a quiescent prominence observed on two consecutive days ]]//; Astronomy and Astrophysics, 629, A138, (2019). DOI: 10.1051/0004-6361/201935488 \\ |
