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Page in construction, the list is presently non-exhaustive ; Last Update March 2026.
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====== THEMIS publications list focusing on solar prominences/protuberances =====
- Karki G., Guo J., Schmieder B., Chandra R., Démoulin P., Poedts S., Gelly B.; //[[ https://ui.adsabs.harvard.edu/abs/2026ApJ...999..148K | Elongation of a Solar Filament and its Three-dimensional Numerical Reconstruction for Magnetic Structures ]]//; The Astrophysical Journal, 999, 148, (2026). DOI: 10.3847/1538-4357/ae40b6 \\
- Karki G., Schmieder B., Démoulin P., Devi P., Chandra R., Joshi R.; //[[ https://ui.adsabs.harvard.edu/abs/2025SoPh..300...98K | Counter-Streaming Velocities in a Quiescent Filament ]]//; Solar Physics, 300, 98, (2025). DOI: 10.1007/s11207-025-02509-w \\
- Karki G., Schmieder B., Devi P., Chandra R., Labrosse N., Joshi R., Gelly B.; //[[ https://ui.adsabs.harvard.edu/abs/2025ApJ...979..182K | Magnetic Reconnection between a Solar Jet and a Filament Channel ]]//; The Astrophysical Journal, 979, 182, (2025). DOI: 10.3847/1538-4357/ada28e \\
- Barczynski K., Schmieder B., Gelly B., Peat A. W., Labrosse N.; //[[ https://ui.adsabs.harvard.edu/abs/2023A&A...680A..63B | Two-horn quiescent prominence observed in Hα and Mg II h & k lines with THEMIS and IRIS]]//; Astronomy and Astrophysics, 680, A63, (2023). DOI:10.1051/0004-6361/202345970 \\
- 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 \\
- 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 \\
- Levens P. J., Labrosse N., Schmieder B., López Ariste A., Fletcher L.; //[[ https://ui.adsabs.harvard.edu/abs/2017A&A...607A..16L | Comparing UV/EUV line parameters and magnetic field in a quiescent prominence with tornadoes ]]//; Astronomy and Astrophysics, 607, A16, (2017). DOI: 10.1051/0004-6361/201730808 \\
- Levens P. J., Schmieder B., López Ariste A., Labrosse N., Dalmasse K., Gelly B.; //[[ https://ui.adsabs.harvard.edu/abs/2016ApJ...826..164L | Magnetic Field in Atypical Prominence Structures: Bubble, Tornado, and Eruption ]]//; The Astrophysical Journal, 826, 164, (2016). DOI: 10.3847/0004-637X/826/2/164 \\
- Schmieder B., Tian H., Kucera T., López Ariste A., Mein N., Mein P., Dalmasse K., Golub L.; //[[ https://ui.adsabs.harvard.edu/abs/2014A&A...569A..85S | Open questions on prominences from coordinated observations by IRIS, Hinode, SDO/AIA, THEMIS, and the Meudon/MSDP ]]//; Astronomy and Astrophysics, 569, A85, (2014). DOI: 10.1051/0004-6361/201423922 \\
- Schmieder B., Roudier T., Mein N., Mein P., Malherbe J. M., Chandra R.; //[[ https://ui.adsabs.harvard.edu/abs/2014A&A...564A.104S | Proper horizontal photospheric flows in a filament channel ]]//; Astronomy and Astrophysics, 564, A104, (2014). DOI: 10.1051/0004-6361/201322861 \\
- Schmieder B., Kucera T. A., Knizhnik K., Luna M., Lopez-Ariste A., Toot D.; //[[ https://ui.adsabs.harvard.edu/abs/2013ApJ...777..108S | Propagating Waves Transverse to the Magnetic Field in a Solar Prominence ]]//; The Astrophysical Journal, 777, 108, (2013). DOI: 10.1088/0004-637X/777/2/108 \\