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| themis [2026/02/26 11:27] – etienne | themis [2026/03/31 14:51] (current) – etienne |
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| THEMIS is located at the [[https://www.iac.es/en/observatorios-de-canarias/teide-observatory | Teide Observatory]] of [[https://www.iac.es/en | IAC]], with a base office in La Laguna, in Tenerife, Canary Islands, Spain. | THEMIS is located at the [[https://www.iac.es/en/observatorios-de-canarias/teide-observatory | Teide Observatory]] of [[https://www.iac.es/en | IAC]], with a base office in La Laguna, in Tenerife, Canary Islands, Spain. |
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| | <color red > ** New ¡¡¡ [[observation:2026campaign#campaign_schedule | 2026 observing campaign schedule]] !!! ** \\ |
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| <html><b> February : The THEMIS team supports the call to French research personnel to <a href="https://atst.osups.universite-paris-saclay.fr/est-white-paper/" style="color:#FF0000;"> co-sign the white paper in support to the European Solar Telescope (EST) project (click here) </a></b></html> | [[science:results:Solo2026 | March : Participation of THEMIS at the "10th Solar Orbiter Scientific Workshop" in Berlin (FR).]] \\ |
| | February : The THEMIS team supports the call to French research personnel to [[https://atst.osups.universite-paris-saclay.fr/est-white-paper/| co-sign the white paper in support to the European Solar Telescope (EST) project]] \\ |
| /*[[https://atst.osups.universite-paris-saclay.fr/est-white-paper/ | February : The THEMIS team supports the call to French research personnel to co-sign the « White paper on the relevance of the European Solar Telescope (EST) for the French heliophysics community »]] */ | /*[[https://atst.osups.universite-paris-saclay.fr/est-white-paper/ | February : The THEMIS team supports the call to French research personnel to co-sign the « White paper on the relevance of the European Solar Telescope (EST) for the French heliophysics community »]] */ |
| | [[science:results:IBISNov25 | November : First screw of the Italian IBIS 2.0 Spectro-imager @ THEMIS.]] \\ |
| [[science:results:OFRAMEdays2026 | February : Participation of THEMIS at the "OFRAME space weather days 2026" conference in Grenoble (FR).]] \\ | |
| [[science:results:Jorgearrival | January : One year visit at THEMIS of PhD student Jorge Romero Castañeda (LPP) in the context of the ANR JET2SB project.]] \\ | |
| [[science:results:KISmeeting | January : Presentation of THEMIS and IBIS at the "Methods and techniques for high-resolution spectro-polarimetry" conference in Freiburg (GER).]] \\ | |
| ** [[science:results:IBISNov25 | November : First screw of the Italian IBIS 2.0 Spectro-imager @ THEMIS.]] ** \\ | |
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| == THEMIS image of the month: February 2026 == | == THEMIS image of the month: March 2026 == |
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| <columns 100% l 50> | <columns 100% l 50> |
| <html> <a href="https://www.themis.iac.es/lib/exe/fetch.php?media=science:gallery:schema:dataproducts_pola_level1.jpg"> | <html> <a href="https://www.themis.iac.es/lib/exe/fetch.php?media=science:gallery:protu:karki2026_fig4_sm.jpg"> |
| <img src="https://www.themis.iac.es/lib/exe/fetch.php?media=science:gallery:schema:dataproducts_pola_level1.jpg" | <img src="https://www.themis.iac.es/lib/exe/fetch.php?media=science:gallery:protu:karki2026_fig4_sm.jpg" |
| alt="THEMIS cable reel" style="width: 100%; height: auto;"></a></html> \\ | alt="THEMIS cable reel" style="width: 100%; height: auto;"></a></html> \\ |
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| <newcolumn 50%> | <newcolumn 50%> |
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| A summary figure of THEMIS level 1 [[observation:data | data products]]. These are the datasets that are directly generated during an observation with THEMIS. The full Sun and slitjaw images are context images that are mainly used by the observed to have basic information of the solar condition on the Sun and the location of the high resolution observations. They are not really meant for scientific use, as equivalent data of a better quality can be obtained by other instruments. The main scientific data are the [[observation:data#Broadband images (BBI)| broadband images]] to study the dynamics of the solar photosphere at high-cadence and high spatial resolution, and the [[observation:data#Spectral images]] from which physical properties such as composition, density, temperature, velocities and magnetic field of the emitting solar plasma can be derived. | |
| | Zoomed view of a solar filament observed on September 28th (top row) & 29th (bottom row) 2003, by GONG (left column) in Hα, and the slit-reconstructed images from the spectra in the Hα line center observed by THEMIS (middle column), and in the Mg II k line center (2796.4 Å) by IRIS (right column). The contours (blue) of the filament observed in GONG are overlaid on the THEMIS image, and the filament contours from THEMIS are overlaid in white over GONG and IRIS images to show the THEMIS FOV. Figure published in [[https://iopscience.iop.org/article/10.3847/1538-4357/ae40b6 | Garima Karki et al, ApJ, 999, 148, 2026.]] |
| </columns> | </columns> |
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