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themis:technical [2024/12/02 18:22] etiennethemis:technical [2024/12/13 15:52] (current) etienne
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-===== THEMIS general technical description ===== +===== THEMIS technical description ===== 
-<html><font color="#ff0000" size="0.5"> Last Update December 2024</font></html>+<html><font color="#ff0000" size="0.5"> In construction ; Last Update December 2024</font></html>
  
 <columns 100% 60%> <columns 100% 60%>
  
-THEMIS is a versatile solar/planetary telescope that can be used in daylight for solar or bright objects observations, or at night for fainter objects.  +THEMIS is a versatile 90cm Ritchey-Chrétien telescope that can be used in daylight for solar or bright objects observations, or at night for fainter objects. THEMIS handle the (extremely) wide range of available light energy flux through a dedicated light distribution detailed below. \\
-THEMIS handle the (extremely) wide range of available light energy flux through a dedicated light distribution detailed below. \\+
  
 The figure opposite presents a diagram with diverse functional blocks of THEMIS systems. A more realistic cartoon (although simplified) of the light-path within THEMIS is presented hereafter. Below is a description of each of THEMIS functional blocks. \\ The figure opposite presents a diagram with diverse functional blocks of THEMIS systems. A more realistic cartoon (although simplified) of the light-path within THEMIS is presented hereafter. Below is a description of each of THEMIS functional blocks. \\
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 <html><font color="#0000ff"> Text in blue highlights a data product and shall redirect to the dedicated</font></html> [[observation:data|THEMIS data products webpage]]. <html><font color="#0000ff"> Text in blue highlights a data product and shall redirect to the dedicated</font></html> [[observation:data|THEMIS data products webpage]].
  
-=== 1Telescope Assembly ===+==== 1Telescope Assembly ====
 <html><font color="#ff0000" size="0.5"> Information on mirror and general description to be added</font></html> <html><font color="#ff0000" size="0.5"> Information on mirror and general description to be added</font></html>
 +
 +As a majority of large professional research telescopes, THEMIS is a Ritchey-Chrétien type telescope, with primary and secondary mirrors having hyperbolic shapes. This design allows to eliminate off-axis optical errors (e.g. comatic aberration) and thus offers wider field of view free of optical errors compared to traditional telescope.
 +
 +The 90cm primary mirror of THEMIS is made of ... and coated with...
 +The secondary mirror has a size of and is ...
 +
 +The telescope tube has a length of ...
 +While originally design to be vacuum sealed, the telescope tube is filled with Helium at 0.5 local atmospheric pressure. This enables optimum performance in order to reduce turbulence within the telescope tube and stress on the entrance plate (which would have been excessively important under vacuum conditions.  
 +
 +The THEMIS telescope is actively cooled by a water heat-exchanger system thanks to...
 +This allows to have typical working temperature of about 5-10°C on the different system 
 +
 +The entrance pupil of the THEMIS telescope tube...
 +
 +
 +Overall the weight of the THEMIS telescope assembly is about...
 +
  
 The telescope optical path has been modified in 2018 to allow for the simplification of the transfer optics F1 -> F2'. The secondary mirror has been refigured, together with a change of the exit window (now an exit lens with optical power and positive chromatic effects). The main resulting characteristics are a new f/16.58 F1 (quite close to the former version), and a new position (lower on) for this focus. \\  The telescope optical path has been modified in 2018 to allow for the simplification of the transfer optics F1 -> F2'. The secondary mirror has been refigured, together with a change of the exit window (now an exit lens with optical power and positive chromatic effects). The main resulting characteristics are a new f/16.58 F1 (quite close to the former version), and a new position (lower on) for this focus. \\ 
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 <html><font color="#ff9900"> No user option available here. </font></html> <html><font color="#ff9900"> No user option available here. </font></html>
  
-=== 1'Polarimetric analyser ===+==== 1'Polarimetric analyser ====
 <html><font color="#ff0000" size="0.5"> Information to be added</font></html> <html><font color="#ff0000" size="0.5"> Information to be added</font></html>
  
      
-=== 2Full-Sun or nighttime guider ===+==== 2Full-Sun guider ====
 <html><font color="#ff0000" size="0.5"> Status of Nighttime guider?</font></html>\\ <html><font color="#ff0000" size="0.5"> Status of Nighttime guider?</font></html>\\
    
-<html><font color="#ff9900"> Depending on the period of observations, two type of guiders are available, Full-Sun or nighttime guiders.</font></html> +/*<html><font color="#ff9900"> Depending on the period of observations, two type of guiders are available, Full-Sun or nighttime guiders.</font></html> 
    
-== Full-sun guider ==+== Full-sun guider ==*/
 A full-sun guider has been setup on the telescope outer ring of the heat protection, near the 1m entrance plate. It uses a 45/500 mm objective, an Herschel prism, a neutral filter, a green continuum 540nm photosphere filter, and a ZWO ASI 178 mono (2kx3k) CMOS camera. <html><font color="#0000ff"> The image from this camera is an available data product </font></html> [[observation:data#Full-sun  guider images| (cf. THEMIS data products)]]. A full-sun guider has been setup on the telescope outer ring of the heat protection, near the 1m entrance plate. It uses a 45/500 mm objective, an Herschel prism, a neutral filter, a green continuum 540nm photosphere filter, and a ZWO ASI 178 mono (2kx3k) CMOS camera. <html><font color="#0000ff"> The image from this camera is an available data product </font></html> [[observation:data#Full-sun  guider images| (cf. THEMIS data products)]].
  
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  \\  \\
  
-== nighttime guider ==+/*== nighttime guider ==
  
-<html><font color="#ff9900">A nighttime guider can be used for nighttime observations (although not mandatory).</font></html>. It is the historical/last full-sun guider. The guider images can be obtains thanks to the insertion of a small extra mirror in the light path above the M1 mirror. This creates a dark indentation over the telescope pupil, which cannot be allowed for solar AO operation : the pupil shall be as free as possible of any obscuration. A motor (EM19) is used to drive in or out this mirror and normal position for solar observation is now OUT.+<html><font color="#ff9900">A nighttime guider can be used for nighttime observations (although not mandatory).</font></html>. It is the historical/last full-sun guider. The guider images can be obtains thanks to the insertion of a small extra mirror in the light path above the M1 mirror. This creates a dark indentation over the telescope pupil, which cannot be allowed for solar AO operation : the pupil shall be as free as possible of any obscuration. A motor (EM19) is used to drive in or out this mirror and normal position for solar observation is now OUT.*/
      
  
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 === 4. Adaptive Optics correction === === 4. Adaptive Optics correction ===
 +
 +See the dedicated page about the [[themis:technical:tao|THEMIS adaptive optics]]
 +
  
 === 5. OBJ2 field scanning === === 5. OBJ2 field scanning ===
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 </columns> </columns>
  
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-<html> 
-<font size="0.5">  
-© 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: you are welcome in using any content provided that you properly cite its origin.</font> 
-</html> 
themis/technical.1733163728.txt.gz · Last modified: 2024/12/02 18:22 by etienne
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