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observation:data [2026/02/26 11:11] – etienneobservation:data [2026/09/23 14:54] (current) – etienne
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- +<html><font color="#ff0000" size="2.5"> Page in construction ; Last Update September 2026</font></html>
-<html><font color="#ff0000" size="2.5"> Page in construction ; Last Update February 2026</font></html>+
  
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 ====== THEMIS data products and access  ====== ====== THEMIS data products and access  ======
  
-==== Data products summary ====+=== Summary ===
  
 Currently, THEMIS provides 4 types of level 1 data products :  Currently, THEMIS provides 4 types of level 1 data products : 
-  * Full-Sun guider images +  * [[# Full-Sun guider images]] 
-  * Broadband images (BBI) +  * [[# Broadband images (BBI)]] 
-  * Slit-jaw images  +  * [[# Slit-jaw context images | Slit-jaw images]]  
-  * MTR2 spectral images (with or without polarimetry)+  * [[# Spectral images | MTR2 spectral images (with or without polarimetry)]]
 Theses images are the direct outputs of the different cameras that equip THEMIS at different point of the optical path.  Their production is detailed on the **[[technical:description|THEMIS technical information page]]**, with informations about the possible options available to the users. Theses images are the direct outputs of the different cameras that equip THEMIS at different point of the optical path.  Their production is detailed on the **[[technical:description|THEMIS technical information page]]**, with informations about the possible options available to the users.
 +
 +THEMIS data are the property of property of CNRS-THEMIS under a [[https://creativecommons.org/licenses/by/4.0/" | Creative Commons CC-BY 4.0 license]]. The data are freely available, however there is unfortunately no catalogue nor webservers to directly access the data. ** Access to specific datasets can be done by contacting the THEMIS team: [[themis.team@themis.iac.es|themis.team@themis.iac.es]].**
  
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-Summary of THEMIS Level 1 data products, in polarimetric analysis mode. MTR2 spectral cameras permits simultaneous observations of different spectral bands (here Fe I @ 630,2 nm as an example). \\+
 <html> <a href="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:schema:dataproducts_pola_level1.jpg" style="width:90%; height: auto;"></a></html>  <html> <a href="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:schema:dataproducts_pola_level1.jpg" style="width:90%; height: auto;"></a></html> 
 +Summary of THEMIS Level 1 data products, in polarimetric analysis mode. \\ 
 +MTR2 spectral cameras permits simultaneous observations of different spectral bands (here Fe I @ 630,2 nm as an example). \\
  
 </columns>  </columns> 
  
-<columns 100% 60%>+<columns 100% 50%>
  
 ==== Data products examples ==== ==== Data products examples ====
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 The full-Sun guider images are mainly to provide context to the observations. They correspond to photospheric observations. They are broadband images taken in the green continuum, around 540 nm, with a bandpass of 10nm. They are not meant for pure scientific analysis. Images are provided as a .png files and have a size of 2000x3000 pixels². The full-Sun guider images are mainly to provide context to the observations. They correspond to photospheric observations. They are broadband images taken in the green continuum, around 540 nm, with a bandpass of 10nm. They are not meant for pure scientific analysis. Images are provided as a .png files and have a size of 2000x3000 pixels².
  
-<newcolumn *40%*>+<newcolumn *50%*>
  
-{{:call22:sun_094627_0000.png?200|}}+{{:call22:sun_094627_0000.png?200|}}\\ 
 +Example of a Full sun guider image
  
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 The images are 2000 x 2000 pixels, hence with pixel resolution of about 0.0275"/pixel. They are primarily provided as .fits files.     The images are 2000 x 2000 pixels, hence with pixel resolution of about 0.0275"/pixel. They are primarily provided as .fits files.    
    
-<newcolumn *40%*>+<newcolumn *50%*> 
 + 
 +<html> <a href="https://www.themis.iac.es/lib/exe/fetch.php?media=science:gallery:ar:z01_20220331_10521652_3.5s3k5ip100fr_decpsf.png"><img src="https://www.themis.iac.es/lib/exe/fetch.php?media=science:gallery:ar:z01_20220331_10521652_3.5s3k5ip100fr_decpsf.png" style="width:49%; height: auto;"></a> 
 +<a href="https://www.themis.iac.es/lib/exe/fetch.php?media=science:gallery:granulation:z01_20220608_12104256_3.5s3k5ip100fr_decpsf.png"><img src="https://www.themis.iac.es/lib/exe/fetch.php?media=science:gallery:granulation:z01_20220608_12104256_3.5s3k5ip100fr_decpsf.png" style="width:49%; height: auto;"></a> 
 +</html> \\ 
 +Examples of BBIs after Knox-Thompson image reconstruction. Right: solar active region. Left: solar granulation on the quiet Sun.
  
  
 </columns>  </columns> 
  
-<columns 100% 60%>+<columns 100% 50%>
  
 === Slit-jaw context images === === Slit-jaw context images ===
  
  
-<newcolumn *40%*>+<newcolumn *50%*>
  
 Planetary configuration (Mercury) \\ Planetary configuration (Mercury) \\
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-<columns 100% 60%>+<columns 100% 50%>
  
  
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 For non polarized observations, for each channel, at each time, the dataset consists 2D image, with a variable wavelength across the field of view in one direction, and the spatial direction along the slit in the other directions. Each channel is centered on a different wavelength across the line profile.  For non polarized observations, for each channel, at each time, the dataset consists 2D image, with a variable wavelength across the field of view in one direction, and the spatial direction along the slit in the other directions. Each channel is centered on a different wavelength across the line profile. 
  
-Datas examples :  +A few sample spectral datasets from the MTR2 spectrograph, along with some basic data manipulation tools will soon be available on the [[observation:data:MTRsampledata | dedicated webpage]].  
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 +<newcolumn *50%*> 
 <html> <video onloadedmetadata="this.muted = true" height="200" controls autoplay loop> <html> <video onloadedmetadata="this.muted = true" height="200" controls autoplay loop>
 <source src="/wdata/Call22/t003_b0101_sp_20190927_21431229_c3_2.mp4" type="video/mp4"> <source src="/wdata/Call22/t003_b0101_sp_20190927_21431229_c3_2.mp4" type="video/mp4">
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 NaD2 config with field scanning and AO NaD2 config with field scanning and AO
  
-<newcolumn 50%> +</columns>  
-<html> <video onloadedmetadata="this.muted = true" height="200" controls autoplay loop> + 
-<source src="/wdata/Call22/t003_b0101_sp_20190927_21431229_c3_2.mp4" type="video/mp4"> +<columns 100% 50%> 
-</video> </html>\\ + 
-NaD2 config with field scanning and AO +==== DATA access ==== 
-</columns>+ 
 +THEMIS data are the property of property of CNRS-THEMIS under a [[https://creativecommons.org/licenses/by/4.0/" | Creative Commons CC-BY 4.0 license]]. \\ 
 +The data are freely available, however there is unfortunately no extensive and complete catalogue nor webservers to directly access the data. Some historical heritage datasets can be retrieved form some archive  \\ 
 +** Access to specific datasets can be done by contacting the THEMIS team: [[themis.team@themis.iac.es|themis.team@themis.iac.es]].**
  
  
-==== DATA Access ==== 
 === THEMIS heritage data === === THEMIS heritage data ===
-The full archive until 2014 is stored  on DLT tapes at the telescope. We do have a functionnal tape reader but no usable software to run it.\\+The full archive until 2014 is stored  on DLT tapes at the telescope. We do have a functional tape reader but no usable software to run it.\\
 We maintain an **incomplete** archive of years 2009, 2010, 2012, 2013, 2014 on HDDs. Listing of what's available: We maintain an **incomplete** archive of years 2009, 2010, 2012, 2013, 2014 on HDDs. Listing of what's available:
   * [[http://www.themis.iac.es/wdata/WOldData/Y09-10.lst | 2009, 2010]]   * [[http://www.themis.iac.es/wdata/WOldData/Y09-10.lst | 2009, 2010]]
observation/data.1772104267.txt.gz · Last modified: by etienne
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