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| THEMIS is an infrastructure at the forefront of contemporary research in the fields of solar physics, inner planetary physics as well as solar instrumentation. The [[science:objectives|complete description of its scientific objectives can be found on the dedicated webpage]]. In summary, its key scientific objectives are: | THEMIS is an infrastructure at the forefront of contemporary research in the fields of solar physics, inner planetary physics as well as solar instrumentation. The [[science:objectives|complete description of its scientific objectives can be found on the dedicated webpage]]. In summary, its key scientific objectives are: |
| * **Instrumental development in high-resolution spectropolarimetry & spectroscopy**:analyzing the electromagnetic spectrum and the polarization of the light to infer multiple properties of the observed celestial body | * **Instrumental development in high-resolution spectropolarimetry & spectroscopy**: analyzing the electromagnetic spectrum and the polarization of the light to infer multiple properties of the observed celestial body |
| * **Solar adaptive optics**: | * **Solar adaptive optics**: |
| * **Understand solar magnetism** : thanks to its spectropolarimetric capabilities, THEMIS performs magnetic field measurements of the visible light that has been polarized by the presence of magnetic field in the solar atmosphere | * **Understand solar magnetism** : thanks to its spectropolarimetric capabilities, THEMIS performs magnetic field measurements of the visible light that has been polarized by the presence of magnetic field in the solar atmosphere |
| * **Study of inner solar system objects**: THEMIS offers without equivalent ground-based observational capabilities of near-Sun objects such as Mercury and comets. THEMIS's high spectral resolution can allow detailed observations of the atmospheres of Mercury and measurement of chemical compositions via spectroscopy. | * **Study of inner solar system objects**: THEMIS offers without equivalent ground-based observational capabilities of near-Sun objects such as Mercury and comets. THEMIS's high spectral resolution can allow detailed observations of the atmospheres of Mercury and measurement of chemical compositions via spectroscopy. |
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| === Results === | ==== Outreach ==== |
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| **[[science:results| THEMIS news and highlights]]** \\ | **[[science:results| THEMIS news and highlights]]** \\ |
| [[science:results:gallery| Galleries of images and animations obtained with THEMIS]] | [[science:gallery| Galleries of images and animations obtained with THEMIS]]\\ |
| | [[science:resources | Media resources: ]] Posters, logos, ... |
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| === Scientific Publications === | ==== Scientific publications & communications ==== |
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| **[[science:publications| Lists of publications related to THEMIS]]** \\ | **[[science:publications| Lists of publications related to THEMIS]]** \\ |
| [[science:publications:technical| Technical publications related to THEMIS]] \\ | [[science:publications:technical| Technical publications related to THEMIS]] \\ |
| [[science:publications:solar| Solar physics publications with THEMIS]] | [[science:publications:solar| Solar physics publications with THEMIS]] \\ |
| [[science:publications:mercury| Hernian (Mercury) physics publications with THEMIS]] | [[science:publications:mercury| Hernian (Mercury) physics publications with THEMIS]] \\ |
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| | [[science:communications | Presentations & posters at scientific conferences]] |
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