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themis [2025/03/18 14:54] etiennethemis [2025/04/10 06:35] (current) etienne
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-<color red > ** [[observation:2025campaign#2025 campaign schedule | Preliminary schedule of 2025 observing campaign]]  ** </color>+<color red > New: </color>  ** [[observation:2025campaign#2025 campaign schedule | Schedule of 2025 observing campaign]]  ** \\
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 **[[science| Scientific research with THEMIS]]** \\ **[[science| Scientific research with THEMIS]]** \\
 [[science:results| THEMIS scientific highlights and news]] \\ [[science:results| THEMIS scientific highlights and news]] \\
-[[science:results:gallery| THEMIS observations and media galleries]]+[[science:gallery| THEMIS observations and media galleries]]
  
  
-== THEMIS image of the month: March 2025 ==+== THEMIS image of the month: April 2025 ==
  
-<columns 70% l > +<columns 100% l > 
-<html> <a href="https://www.themis.iac.es/lib/exe/fetch.php?media=results:gallery:ar:noaa13981_c3flare_20250206_113010.jpg"> <img src="https://www.themis.iac.es/lib/exe/fetch.php?media=results:gallery:ar:noaa13981_c3flare_20250206_113010.jpg" alt="Themis NOAA 13981 during C3.3-class flare" style="width: 100%; height: auto;"></a></html> +<html> <a href="https://www.themis.iac.es/lib/exe/fetch.php?media=results:gallery:ar:activeregionbestof_6x2.jpg"> <img src="https://www.themis.iac.es/lib/exe/fetch.php?media=results:gallery:ar:activeregionbestof_6x2.jpg" alt="2022-2025 THEMIS sunspot best-of" style="width: 100%; height: auto;"></a></html> 
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-THEMIS observations of the east sunspot group of the active region NOAA 13981 on February 6th 2025. The left image is a Knox-Thompson reconstructed from red continuum broadband camera. The right panels are intensity maps reconstructed from spectral observations by the MTR2 spectrograph observing the Hα absorption lineTheses maps are reconstructed from a scan by the telescope of the active region. While these intensity images have lower spatial resolution, they provide a wealth of spectroscopic information. The region was observed during a flare, as can be noted by the typical ribbon-shape emission in the Hα line centre. This emission is absent from the continuum emission, indicating a chromospheric emission phenomena. Meanwhile, the red wing maps (Hα+1Å and Hα+0.5Å) display dark absorbing material above the location of the flare ribbons, signature of down-flowing dense material, a phenomena nicknamed "coronal rain"      +A selection of THEMIS sunspot observations obtained between 2022 and 2025 with the [[technical:description#broadband_imaging_bbi_filter_camera | BroadBand Imaging Camera]]Observations are performed using [[technical:tao|Themis Adaptive Optics]] and images are processed with Knox-Thompson image-reconstruction method. </columns>
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-[[results:gallery:imofmonth|Past images of the month]]+[[science:imofmonth|Past images of the month]]
  
  
themis.1742309687.txt.gz · Last modified: 2025/03/18 14:54 by etienne
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