This shows you the differences between two versions of the page.
| Next revision | Previous revision | ||
| results:2023_prominences_highlight [2024/11/14 13:02] – created etienne | results:2023_prominences_highlight [2024/12/18 14:41] (current) – removed etienne | ||
|---|---|---|---|
| Line 1: | Line 1: | ||
| - | ===== THEMIS prominences observations during the 2023 campaign ====== | ||
| - | Successful coordinated observations of filaments and prominences during run #2023/239 of Labrosse et al. | ||
| - | The IRIS spacecraft MgII UV line (left) and THEMIS-MTR2 Halpha and Helium D3 lines (right) are showing the same solar filament located in between NOAA 13449 and 13446. Both instruments are raster spectrographs. | ||
| - | |||
| - | ;#; | ||
| - | {{: | ||
| - | |||
| - | [Figure credit: B. Schmieder] | ||
| - | ;#; | ||
| - | |||
| - | ---- | ||
| - | |||
| - | < | ||
| - | <font size=" | ||
| - | © 2024 CNRS-THEMIS <br> | ||
| - | Terms of use: unless otherwise specified, all graphical (webcam records, movies, pictures) or non-graphical material (text) from this site is property of CNRS-THEMIS: | ||
| - | </ | ||