Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revisionPrevious revision
Next revision
Previous revision
themis:history [2024/12/05 12:41] etiennethemis:history [2024/12/16 16:23] (current) etienne
Line 3: Line 3:
 The Origins and Development of the THEMIS (Télescope Héliographique pour l’Étude du Magnétisme et des Instabilités Solaires) solar telescope encompass a rich history of international collaboration, scientific ambition, and technological innovation.  The Origins and Development of the THEMIS (Télescope Héliographique pour l’Étude du Magnétisme et des Instabilités Solaires) solar telescope encompass a rich history of international collaboration, scientific ambition, and technological innovation. 
  
-==== Scientific motivation, conceptualization (1970') ====+==== Scientific motivation, conceptualization (1970's) ====
  
 In the latter half of the 20th century, solar physicists recognized that the Sun's magnetic field plays a crucial role in various solar phenomena, including sunspots, solar flares, and coronal mass ejections. However, understanding the intricate details of the Sun's magnetic field required advanced observational tools capable of high-resolution measurements. In the latter half of the 20th century, solar physicists recognized that the Sun's magnetic field plays a crucial role in various solar phenomena, including sunspots, solar flares, and coronal mass ejections. However, understanding the intricate details of the Sun's magnetic field required advanced observational tools capable of high-resolution measurements.
Line 14: Line 14:
 was presented for the first time to the Institut National d’Astronomie et de Géophysique (predecessor of INSU) in 1975. was presented for the first time to the Institut National d’Astronomie et de Géophysique (predecessor of INSU) in 1975.
  
-=== Site selection (1970') ===+==== Site selection (1970's====
  
 The site selection for THEMIS was part of a larger project to search for optimal location for international solar observations. The The site selection for THEMIS was part of a larger project to search for optimal location for international solar observations. The
Line 22: Line 22:
  
  
-=== Telescope design & Instrumentation Development (1980') ===+==== Telescope design & Instrumentation Development (1980's====
  
 The design phase, directed by Jean Rayrole, focused on creating a telescope optimized for high-resolution spectropolarimetric observations. Key considerations included: The design phase, directed by Jean Rayrole, focused on creating a telescope optimized for high-resolution spectropolarimetric observations. Key considerations included:
Line 32: Line 32:
 High-precision spectropolarimeters were designed to analyze the polarization states of light across different wavelengths, providing detailed information about magnetic fields. In THEMIS design, three first light instruments have been developed: High-precision spectropolarimeters were designed to analyze the polarization states of light across different wavelengths, providing detailed information about magnetic fields. In THEMIS design, three first light instruments have been developed:
   * **a spectrograph, MTR**: XXXX    * **a spectrograph, MTR**: XXXX 
-  * **a spectro-imager, **: XXXX +  * **a spectro-imager, IPM**: the Italian Panoramic Monochromator ([[https://aas.aanda.org/articles/aas/abs/1998/06/ds6554/ds6554.html| Cavallini, A&A, 1998]]) performed solar bidimensional spectroscopy. On a square field $33''\times 33''$, this instrument allowed to obtain monochromatic images of the solar surface with high spectral resolution (R > 256 000 at 5500 Å), preserving all the spatial resolution delivered by the telescope (~0.2''). IPM consisted of a Fabry-Perot interferometer, used in telecentric mounting, in series with a Universal Birefringent Filter, used as an order sorter. 
   * **an imaging spectrometer, MSDP**: XXXX    * **an imaging spectrometer, MSDP**: XXXX 
  
-==== Construction====+==== Construction (1990's) ====
  
 Securing adequate funding was a critical step in the development of THEMIS. The project received financial backing from national science agencies of the participating countries, as well as from European Union research funds aimed at fostering international scientific collaborations. Each partner country committed a portion of the budget, covering aspects such as construction, instrumentation, and operational costs. Securing adequate funding was a critical step in the development of THEMIS. The project received financial backing from national science agencies of the participating countries, as well as from European Union research funds aimed at fostering international scientific collaborations. Each partner country committed a portion of the budget, covering aspects such as construction, instrumentation, and operational costs.
Line 42: Line 42:
   * France: The Institut National des Sciences de l'Univers (INSU), part of CNRS, took the lead in coordinating the project.   * France: The Institut National des Sciences de l'Univers (INSU), part of CNRS, took the lead in coordinating the project.
   * Italy: The Instituto Nazionale di Astrofisica (INAF), part of CNR contributed significant expertise in solar physics and instrumentation.   * Italy: The Instituto Nazionale di Astrofisica (INAF), part of CNR contributed significant expertise in solar physics and instrumentation.
-  * Spain: The Spanish National Research Council (CSIC) and other Spanish institutions, in particular the Instituto de Astrofísica de Canarias (IAC) provides the site and logistical support.  provided support, particularly in site selection and infrastructure development.+  * Spain: Consejo Superior de Investigaciones Científicas(CSIC) and other Spanish institutions, in particular the Instituto de Astrofísica de Canarias (IAC) provides the site and logistical support.  provided support, particularly in site selection and infrastructure development.
  
 An agreement was signed between the French CNRS and the Italian CNR. The construction cost of 87.5 million francs was covered with 80% financed by the CNRS and 20% by the CNR. The same funding distribution applies to the operation of the instrument. Observation time is allocated as follows: 60% for the French, 15% for the Italians, 20% for the Spanish, and 5% for "international time." A Franco-Italian steering committee then determined the general policies for the telescope's operation and development. An agreement was signed between the French CNRS and the Italian CNR. The construction cost of 87.5 million francs was covered with 80% financed by the CNRS and 20% by the CNR. The same funding distribution applies to the operation of the instrument. Observation time is allocated as follows: 60% for the French, 15% for the Italians, 20% for the Spanish, and 5% for "international time." A Franco-Italian steering committee then determined the general policies for the telescope's operation and development.
Line 48: Line 48:
 Construction began in the early 1990s, involving meticulous planning and execution to assemble the telescope's complex components. The primary mirror and optical components were manufactured with high precision to meet the stringent requirements for spectropolarimetric measurements. Integrating various subsystems, such as adaptive optics, control electronics, and data acquisition systems, was a challenging but essential task to ensure seamless operation. Construction began in the early 1990s, involving meticulous planning and execution to assemble the telescope's complex components. The primary mirror and optical components were manufactured with high precision to meet the stringent requirements for spectropolarimetric measurements. Integrating various subsystems, such as adaptive optics, control electronics, and data acquisition systems, was a challenging but essential task to ensure seamless operation.
  
-===Commissioning and early operations===+==== Commissioning, first light and first phase of exploitation (1996-XXX) ====
  
 Before full-scale operations commenced, extensive testing was conducted to verify the telescope's performance. Ensuring precise alignment of optical components was critical for achieving the desired resolution and polarimetric accuracy. Spectropolarimeters and other instruments underwent calibration processes to ensure accurate measurements. Before full-scale operations commenced, extensive testing was conducted to verify the telescope's performance. Ensuring precise alignment of optical components was critical for achieving the desired resolution and polarimetric accuracy. Spectropolarimeters and other instruments underwent calibration processes to ensure accurate measurements.
- 
-===First light and early scientific results=== 
  
 THEMIS received its first light on March 16, 1996, and was inaugurated that same year by the King and Queen of Spain, along with French and Italian authorities. THEMIS received its first light on March 16, 1996, and was inaugurated that same year by the King and Queen of Spain, along with French and Italian authorities.
  
-=== Evolution and enhancements ====+==== Evolution and redesign (2010's) ====
  
 +xxx
 Over the years, THEMIS has undergone several upgrades to enhance its capabilities: Over the years, THEMIS has undergone several upgrades to enhance its capabilities:
   * **[[themis:technical:tao|THEMIS Adaptive Optics]]**: Upgrades to adaptive optics systems to further reduce atmospheric distortions, allowing for sharper images.   * **[[themis:technical:tao|THEMIS Adaptive Optics]]**: Upgrades to adaptive optics systems to further reduce atmospheric distortions, allowing for sharper images.
Line 63: Line 62:
   * Planetary observations: XXXX   * Planetary observations: XXXX
  
-=== New life for the THEMIS telescope ==== + 
-xxxxx+ 
 +==== New life for the THEMIS telescope (2020's) ==== 
  
 Despite advancements in space-based solar observatories, THEMIS remains a valuable asset due to its unique capabilities and the ability to perform long-term, high-resolution observations from the ground. Despite advancements in space-based solar observatories, THEMIS remains a valuable asset due to its unique capabilities and the ability to perform long-term, high-resolution observations from the ground.
themis/history.1733402510.txt.gz · Last modified: 2024/12/05 12:41 by etienne
Recent changes RSS feed Debian Powered by PHP Valid XHTML 1.0 Valid CSS Driven by DokuWiki