From European Southern Observatory [Observatoire européen austral][Europäische Südsternwarte] (EU): “New powerful laser based on ESO technology passes field test”
From European Southern Observatory [Observatoire européen austral][Europäische Südsternwarte] (EU)
31 August 2021
Domenico Bonaccini Calia
Physicist in the Laser and Photonics Group at ESO
Garching bei München, Germany
Email: dbonacci@eso.org
Juan Carlos Muñoz Mateos
ESO Media Officer
Garching bei München, Germany
Email: jmunoz@eso.org
A powerful experimental laser, based on ESO technology, passed a key test last month at the Allgäuer Volkssternwarte Ottobeuren – Startseite (DE). The adaptive-optics laser, developed in collaboration with industry, has important additional capabilities compared to existing systems. It will be part of the CaNaPy Laser Guide Star Adaptive Optics system set to be installed at the European Space Agency [Agence spatiale européenne][Europäische Weltraumorganisation](EU) Optical Ground Station in Tenerife, Spain, in the frame of the ESO–ESA Research & Development collaboration. The higher laser power, nearly three times higher than in current systems, opens the door for developments in laser satellite communication, as well as significant improvements in the sharpness of astronomical images taken with ground-based telescopes.
Astronomical adaptive optics refers to systems on ground-based telescopes that correct for the blurring effect brought about by turbulence in the Earth’s atmosphere — the same effect that causes stars seen from Earth to “twinkle”. To remove the distortions, these systems require a bright reference star close to the object of study. Because these stars are not always conveniently placed on the sky, astronomers use lasers to excite sodium atoms at 90 km altitude in the Earth’s atmosphere, creating artificial stars near the field of interest that can be used to map and correct the atmospheric turbulence.
The new experimental laser is based on the same ESO technology that is behind the Four Laser Guide Star Facility, successfully operating at ESO’s Very Large Telescope in Chile [below], as well as at most large astronomical observatories in the world. But while those lasers have a power of 22 Watts, this new laser has almost tripled the power at 63 Watts, a huge leap forward in astronomy laser technology that will, among other things, improve the sharpness of adaptive-optics images at visible wavelengths. As part of a collaborative R&D agreement with ESO, the Canadian company MPB Communications — one of ESO’s industry partners — has been able to scale up the power of their infrared “Raman fibre amplifier” source. This is the breakthrough that allows the ESO CaNaPy laser to achieve such a high power [1].
In addition, the German company TOPTICA Photonics AG, another of ESO’s industry partners, has developed and implemented in the CaNaPy laser a frequency chirping system for this new class of lasers, as part of a collaborative R&D agreement with ESO. Chirping consists in rapidly changing the frequency to which the laser is tuned. This increases the number of sodium atoms excited by the laser, making the artificial star brighter and thus improving the turbulence correction. TOPTICA has installed the chirping prototype on the 63 Watts laser and, with ESO, has commissioned on sky both the laser and its novel chirping system.
This new experimental CaNaPy laser is an example of astronomical technology developed in-house at ESO in partnership with industry and then transferred back to industrial usage including in new fields, thus finding applications beyond its original purpose and benefitting society as a whole. Once the CaNaPy facility instrument is installed at the ESA Optical Ground Station in Tenerife — a collaborative project between ESO [2] and ESA — it will provide both organisations, ESA and ESO, with opportunities to advance the use of laser guide star adaptive optics technologies not only for astronomy but also for satellite optical communication. Optical laser communication allows satellites to send and receive signals to and from Earth with ultra-fast bandwidth, a prospect that ESA is investigating. Optical laser signals can transmit much more information than radio signals, but they are equally affected by atmospheric turbulence. Laser guide star adaptive optics has thus the potential to greatly improve the optical links between satellites and ground stations.
Notes
[1] MPB Communications scaled up the power of their Raman fibre amplifier, which operates in the infrared at 1178 nm, from the 36 Watts level normally used in the commercial sodium guidestar lasers, to an unprecedented level of 100 Watts. This allows CaNaPy to achieve a continuous-wave power of 63 Watts while operating at 589 nm, in the visible.
[2] The collaboration includes several institutes in ESO member states: the INAF Italian National Institute for Astrophysics [Istituto Nazionale di Astrofisica] (IT), Durham University (UK), and the Institute of Astrophysics of the Canaries[Instituto de Astrofísica de Canarias] (ES).
See the full article here .
five-ways-keep-your-child-safe-school-shootings
Please help promote STEM in your local schools.
Visit ESO (EU) in Social Media-
European Southern Observatory [Observatoire européen austral][Europäische Südsternwarte] (EU) is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It is supported by 16 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world’s most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world’s largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is a major partner in ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre European Extremely Large Telescope, the E-ELT, which will become “the world’s biggest eye on the sky”.
European Southern Observatory(EU) La Silla HELIOS (HARPS Experiment for Light Integrated Over the Sun)
ESO 3.6m telescope & HARPS atCerro LaSilla, Chile, 600 km north of Santiago de Chile at an altitude of 2400 metres.
MPG Institute for Astronomy [Max-Planck-Institut für Astronomie](DE) 2.2 meter telescope at/European Southern Observatory(EU) Cerro La Silla, Chile, 600 km north of Santiago de Chile at an altitude of 2400 metres.
European Southern Observatory(EU)La Silla Observatory 600 km north of Santiago de Chile at an altitude of 2400 metres.
European Southern Observatory(EU) , Very Large Telescope at Cerro Paranal in the Atacama Desert •ANTU (UT1; The Sun ) •KUEYEN (UT2; The Moon ) •MELIPAL (UT3; The Southern Cross ), and •YEPUN (UT4; Venus – as evening star). Elevation 2,635 m (8,645 ft) from above Credit J.L. Dauvergne & G. Hüdepohl atacama photo.
European Southern Observatory/National Radio Astronomy Observatory(US)/National Astronomical Observatory of Japan(JP) ALMA Array in Chile in the Atacama at Chajnantor plateau, at 5,000 metres.
European Southern Observatory(EU)/MPG Institute for Radio Astronomy [MPG Institut für Radioastronomie](DE) ESO’s Atacama Pathfinder Experiment(CL) high on the Chajnantor plateau in Chile’s Atacama region, at an altitude of over 4,800 m (15,700 ft).
European Southern Observatory(EU) ExTrA telescopes at erro LaSilla at an altitude of 2400 metres.
A novel gamma ray telescope under construction on Mount Hopkins, Arizona. A large project known as the Čerenkov Telescope Array composed of hundreds of similar telescopes to be situated in the Canary Islands and Chile at, ESO Cerro Paranal site The telescope on Mount Hopkins will be fitted with a prototype high-speed camera, assembled at the. University of Wisconsin–Madison and capable of taking pictures at a billion frames per second. Credit: Vladimir Vassiliev.
European Space Agency [Agence spatiale européenne][Europäische Weltraumorganisation](EU), The new Test-Bed Telescope 2is housed inside the shiny white dome shown in this picture, at ESO’s LaSilla Facility in Chile. The telescope has now started operations and will assist its northern-hemisphere twin in protecting us from potentially hazardous, near-Earth objects.The domes of ESO’s 0.5 m and the Danish 0.5 m telescopes are visible in the background of this image.Part of the world-wide effort to scan and identify near-Earth objects, the European Space Agency’s Test-Bed Telescope 2 (TBT2), a technology demonstrator hosted at ESO’s La Silla Observatory in Chile, has now started operating. Working alongside its northern-hemisphere partner telescope, TBT2 will keep a close eye on the sky for asteroids that could pose a risk to Earth, testing hardware and software for a future telescope network.
European Space Agency [Agence spatiale européenne][Europäische Weltraumorganisation](EU) The open dome of The black telescope structure of the‘s Test-Bed Telescope 2 peers out of its open dome in front of the rolling desert landscape. The telescope is located at ESO’s La Silla Observatory, which sits at a 2400 metre altitude in the Chilean Atacama desert.
sciencesprings 
Reply