Concordia Station

Concordia Research Station, which opened in 2005, is a French–Italian research facility that was built 3,233 m (2.0 mi) above sea level at a location called Dome C on the Antarctic Plateau, Antarctica. It is located 1,100 km (680 mi) inland from the French research station at Dumont D'Urville, 1,100 km (680 mi) inland from Australia's Casey Station and 1,200 km (750 mi) inland from the Italian Zucchelli Station at Terra Nova Bay. Russia's Vostok Station is 560 km (350 mi) away. The Geographic South Pole is 1,670 km (1,040 mi) away. The facility is also located within Australia's claim on Antarctica, the Australian Antarctic Territory.

Concordia Station
Antarctic base
Concordia Research Station at Dome Circe, Charlie or Concordia.
Concordia Station
Location of Condordia Station in Antarctica
Coordinates: 75°05′59″S 123°19′56″E
Country Italy
 France
Location in AntarcticaDome C
Antarctic Plateau
Administered byNational Antarctic Research Program
IPEV
Established2005 (2005)
Elevation
3,233 m (10,607 ft)
Population
 (2017)
 • Total
  • Summer: 50
  • Winter: 13
TypeAll Year-round
PeriodAnnual
StatusOperational
WebsiteConcordia Institut Polaire Français
Concordia Skiway
The last take-off in February 2015
Summary
Airport typePrivate
OperatorNational Antarctic Research Program
IPEV
LocationAntarctic Plateau
Time zone(UTC+8)
Elevation AMSL10,725 ft / 3,269 m
Coordinates75°06′12″S 123°21′30″E
Map
Concordia Skiway
Location of airfield in Antarctica
Runways
Direction Length Surface
ft m
01/19 4,910 1,497 Ice[1]
The main part of the summer camp at Dome C (Concordia) Station in January 2005

Concordia Station is the third permanent, all-year research station on the Antarctic Plateau besides Vostok Station (Russian) and the Amundsen–Scott South Pole Station (U.S.) at the Geographic South Pole. It is jointly operated by scientists from France and Italy and regularly hosts ESA scientists.

Location of the "Concordia Station" relatively near the South Pole

History

In 1992, France decided to build a new station on the Antarctic Plateau. The program was later joined by Italy in 1993.

In 1995, Pr. Jean Vernin from University of Nice Sophia-Antipolis and Pr. Giorgio Dall'Oglio from University of Rome performed the first scientific experience towards a site qualification at Dome C.

In 1996, a French-Italian team established a summer camp at Dome C. The two main objectives of the camp were the provision of logistical support for the European Project for Ice Coring in Antarctica (EPICA) and the construction of a permanent research station.

The new all-year facility, Concordia Station, became operational in 2005. The first winterover began with a staff of 13 (eleven French and 2 Italians) in February 2005.

Access
Part of a traverse, which was bringing fuel, food, and other supplies from Dumont d'Urville to Dome C (January 2005)

Most of the cargo is moved to Dome C by traverse from Dumont d'Urville Station, covering 1,200 km in 7 to 12 days depending on weather conditions. Station personnel and light cargo arrive by air, using Twin Otter aircraft from DDU or Mario Zucchelli Station at 1200 km.

Environment

Dome C is situated on top of the Antarctic Plateau. No animals or plants live at a distance of more than a few tens of kilometers from the Southern Ocean. However, south polar skuas have been spotted overflying the station, 1,200 km away from their nearest food sources. It is believed that these birds have learned to cross the continent instead of circumnavigating it.

Human biology and medicine

Concordia Station shares many stressor characteristics similar to that of long-duration deep-space missions, in particular extreme isolation and confinement, and therefore serves as a useful analogue platform for research relevant to space medicine. During the winter, the crew are isolated from the outside world, having no transportation and limited communication[2] for 9 months and live a prolonged period in complete darkness, at an altitude almost equivalent to 4000m at the equator. This creates physiological and psychological strains on the crew. Concordia station is particularly useful for the study of chronic hypobaric hypoxia, stress secondary to confinement and isolation, circadian rhythm and sleep disruption, individual and group psychology, telemedicine, and astrobiology. Concordia station has been proposed as one of the real-life Earth-based analogues for long-duration deep-space missions.[3]

Glaciology

In the 1970s, Dome C was the site of ice core drilling by field teams of several nations. In the 1990s, Dome C was chosen for deep ice core drilling by the European Project for Ice Coring in Antarctica (EPICA). Drilling at Dome C began in 1996 and was completed on December 21, 2004, reaching a drilling depth of 3270.2 m, 5 m above bedrock. The age of the oldest recovered ice is estimated to be ca. 900,000 years.[4]

Astronomy

Concordia Station has been identified as a suitable location for extremely accurate astronomical observations. The transparency of the Antarctic atmosphere permits the observation of stars even when the sun is at an elevation angle of 38°. Other advantages include the very low infrared sky emission, the high percentage of cloud-free time and the low aerosol and dust content of the atmosphere.

The median seeing measured with a DIMM Differential Image Motion Monitor [5] placed on top of an 8.5 m high tower is 1.3 ± 0.8 arcseconds.

This is significantly worse than most major observatory sites, but similar to other observatories in Antarctica. However, Lawrence et al. consider other features of the site and conclude that "Dome C is the best ground-based site to develop a new astronomical observatory".[6] Note however that this was written before whole-atmospheric seeing measurements had been made at Dome C.

Thanks to the Single Star Scidar SSS, Vernin, Chadid and Aristidi et al. [7] and Giordano, Vernin and Chadid et al.[8] finally demonstrated that most of the optical turbulence is concentrated within the first 30 m atmospheric level at Dome C. The rest of the atmosphere is very quiet with a seeing of about 0.3-0.4 arcseconds, and the overall seeing is somewhat around 1.0 arcseconds.

Launched in 2007, PAIX the first robotic multi-color Antarctica Photometer [9] gives a new insight to cope with unresolved stellar enigma and stellar oscillation challenges and offers a great opportunity to benefit from an access to the best astronomical site on Earth –Dome C–. Indeed, Chadid, Vernin, Preston et al.[10] implement, for the first time from the ground, a new way to study the stellar oscillations, pulsations and their evolutionary properties with long uninterrupted and continuous precision observations over 150 days, and without the regular interruptions imposed by the Earth rotation. PAIX achieves astrophysical UBVRI bands time-series measurements of stellar physics fields, challenging photometry from Space.

Climate

The climate at Dome C where Concordia Station is located is frigid all year round, being one of the coldest places on Earth. It has a polar ice cap climate (Köppen EF), with maximums ranging from −24.8 °C (−12.6 °F) in December to −62 °C (−80 °F) in May, mean ranging from −30.4 °C (−22.7 °F) in December to −65.3 °C (−85.5 °F) in May and minimums ranging from −36.1 °C (−33.0 °F) in December to −68.7 °C (−91.7 °F) in May. The annual average air temperature is −54.5 °C (−66.1 °F). The station has never recorded a temperature above freezing; the warmest temperature recorded was −5.4 °C (22.3 °F) in January. Temperatures can fall below −80 °C (−112 °F) in winter, and the coldest recorded temperature was −84.6 °C (−120.3 °F) in August 2010; one of the coldest temperatures ever recorded on Earth.

Humidity is low and it is also very dry, with very little precipitation throughout the year.

Dome C does not experience the katabatic winds typical for the coastal regions of Antarctica because of its elevated location and its relative distance from the edges of the Antarctic Plateau. Typical wind speed in winter is 2.8 m/s.

Climate data for Concordia
Month Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec Year
Record high °C (°F) −5.4
(22.3)		 −12.9
(8.8)		 −31.0
(−23.8)		 −32.9
(−27.2)		 −28.5
(−19.3)		 −30.2
(−22.4)		 −25.4
(−13.7)		 −26.5
(−15.7)		 −30.3
(−22.5)		 −23.1
(−9.6)		 −17.0
(1.4)		 −9.4
(15.1)		 −5.4
(22.3)
Average high °C (°F) −24.9
(−12.8)		 −33.7
(−28.7)		 −48.7
(−55.7)		 −58.5
(−73.3)		 −62.0
(−79.6)		 −58.9
(−74.0)		 −58.4
(−73.1)		 −57.8
(−72.0)		 −54.1
(−65.4)		 −44.8
(−48.6)		 −32.5
(−26.5)		 −24.8
(−12.6)		 −46.6
(−51.9)
Daily mean °C (°F) −31.1
(−24.0)		 −40.6
(−41.1)		 −54.0
(−65.2)		 −61.9
(−79.4)		 −65.3
(−85.5)		 −62.3
(−80.1)		 −62.1
(−79.8)		 −61.7
(−79.1)		 −59.5
(−75.1)		 −52.2
(−62.0)		 −39.3
(−38.7)		 −30.4
(−22.7)		 −51.7
(−61.1)
Average low °C (°F) −37.5
(−35.5)		 −47.7
(−53.9)		 −59.4
(−74.9)		 −65.4
(−85.7)		 −68.7
(−91.7)		 −65.8
(−86.4)		 −66.0
(−86.8)		 −65.8
(−86.4)		 −65.2
(−85.4)		 −59.8
(−75.6)		 −46.2
(−51.2)		 −36.1
(−33.0)		 −57.0
(−70.5)
Record low °C (°F) −46.7
(−52.1)		 −60.0
(−76.0)		 −72.0
(−97.6)		 −75.9
(−104.6)		 −79.6
(−111.3)		 −77.3
(−107.1)		 −79.8
(−111.6)		 −84.6
(−120.3)		 −81.9
(−115.4)		 −74.0
(−101.2)		 −61.9
(−79.4)		 −45.9
(−50.6)		 −84.6
(−120.3)
Source: [11]

Winterovers

While the station has been in use for summer campaigns since December 1997, the first winterover (February to October) was only made in 2005. During this period, the station is inaccessible, requiring total autonomy.

First winter-over (DC01 – 2005)
Frozen face of wintering personnel (Christophe Mozer) during first Dome C winterover (2005)

The first winter began in mid-February 2005, with thirteen wintering (eleven French people and two Italians):

In September 2005 the highest temperature was −48 °C, with an average in August of −60.2 °C and a record of −78.6 °C on 1 September. At these temperatures, trips outside had to be performed with the utmost care. Those going outside travelled at least in pairs and were equipped with a radio, spare batteries and a full fleece suit, with only the eyes at times visible. Glaciologist Italian Emanuele Salvietti had to take snow samples every day one kilometre from the base. As he had to walk (because no vehicle operates at these temperatures), he built a full face mask, with only a pipe to breathe. The slightest mistake would lead to certain injury, as astronomer Agabi Karim explained: "Burns on the cheeks and eyelashes glued to the lens of the telescope," after exposure to the freezing cold.

Second winter-over (DC02 – 2006)

The second winter was conducted from February to November 2006 with a team of ten wintering (six French and four Italian):

  • Minh Ly Pham Minh: station leader, physician,  France
  • Michele Impara: computer science,  Italy
  • Loïc Le Bechec: chef,  France
  • Lucia Agnoletto: seismologist,  Italy
  • Eric Aristidi: astronomer,  France
  • Omar Cerri: glaciologist,  Italy
  • Shaun Deshommes: technical chief,  France
  • Elyseo D'Eramo: mechanic,  Italy
  • José Dos Santos: electrician,  France
  • Miguel Ravoux: plumber,  France

The record temperature for this winter was measured at −80 °C on 5 September 2006 at 2:37 ET was renewed several times.

Third winter-over (DC03 – 2007)

The third winter ran from February to November 2007 with a team of wintering composed of fourteen people (eight French and six Italian):

  • François Jeanneaux: engineer,  France
  • Jean-Pierre Pillisio: plumber,  France
  • Carlos Marsal: chef,  France
  • Maurizio Busetto: climatologist,  Italy
  • Yvan Levy: technical chief,  France
  • Nicolas Le Parc: electrician,  France
  • Christophe Choley: mechanic,  France
  • Federico Miliacca: computer and telecommunications,  Italy
  • Djamel Mékarnia: astronomer,  France
  • Runa Briguglio: astronomer,  Italy
  • Giuseppe Soriani: surgeon,  Italy
  • Pietro di Felice: station leader, engineer,  Italy
  • Benedict Cuisset: technical,  France
  • Alessandro Iacomino: glaciologist,  Italy

The average temperature was −65 °C and the minimum temperature recorded was −81.9 °C reached on September 5.

Fourth winter-over (DC04 – 2008)

The fourth winter took place from 31 January 2008 to 8 November 2008 with a team consisting of thirteen winter-overs (seven French and six Italian):

  • Erick Bondoux: astronomer,  France
  • Laurent Bonnardot: biomedical,  France
  • Zalpha Challita: astronomer,  France
  • Giorgio Deidda: chef,  Italy
  • Sébastien Denamur: mechanic,  France
  • Laurent Fromont: electrician,  France
  • Daniele Frosini: glaciologist,  Italy
  • Patrick LeRoy: technical chief,  France
  • Fabrizio Martinet: plumber,  Italy
  • Roberto Rainis: doctor,  Italy
  • Lucia Sabbatini: astrophysicist,  Italy
  • Riccardo Schioppo: climatologist,  Italy
  • Jean-François Vanacker: station leader, radio,  France

Fifth winter-over (DC05 – 2009)

The fifth wintering took place from February 2009 to November 2009 with a team of twelve people (eight French, three Italian and one British):

  • Massimiliano Faiella: technical chief,  Italy
  • Domenico Fasano: chef,  Italy
  • William Frinot: plumber,  France
  • Laura Genoni: glaciologist,  Italy
  • Caroline Jullian: atmospheric chemistry,  France
  • Alexander Leluc: mechanic,  France
  • Eric Lotz: station leader, physician,  France
  • Denis Petermann: astronomer,  France
  • Cyprien Pouzenc: astronomer,  France
  • Alex Salam: ESA biomedical research,  United Kingdom
  • Eric Tragin: electrician,  France
  • Jonathan Zaccaria: radio, computer, science support,  France

Sixth winter-over (DC06 – 2010)

This Wintering took place with a team of thirteen (six French, six Italian and one Czech):

  • Jean-François Vanacker: station leader,  France
  • Ales Rybka: ESA biomedical research,  Czech Republic
  • Karim Agabi: astronomer,  France
  • Alessandro Bambini: electrician,  Italy
  • Arthur Le Forestier: technical chief,  France
  • Boris Padovan: computer, telecommunications,  Italy
  • Christophe Rouy: mechanic,  France
  • Daniele Karlicek: glaciologist,  Italy
  • Giorgio Deidda: chef,  Italy
  • Jean-Marie Moysan: plumber,  France
  • Lorenzo Moggio: atmospheric chemistry,  Italy
  • Rosa Forgittoni: doctor,  Italy
  • Sylvain Lafont: glaciologist,  France

Seventh winter-over (DC07 – 2011)

The seventh wintering took place with a team of 14 people (seven French, six Italian and one British):

  • Andrea Cesana: station leader, doctor,  Italy
  • Eoin MacDonald: ESA biomedical research,  United Kingdom
  • Djamel Mekarnia: astronomer,  France
  • Eric Aristidi: astronomer,  France
  • Alessandro Giusto: electrician,  Italy
  • Sergeant Frederic: technical chief,  France
  • Paolo Perfetti: computer, telecommunications,  Italy
  • David Colin: mechanic,  France
  • Domenico Romano: astronomer, glaciologist,  Italy
  • Andrea Ballarini: chef,  Italy
  • Vivien Koutcheroff: plumber,  France
  • Ilann Bourgeois: atmospheric chemistry, glaciologist,  France
  • Pascal Robert: technician seismology, magnetism,  France
  • Angelo Galeandro: meteorologist,  Italy

Eighth winter-over (DC08 – 2012)

The eighth wintering took place with a team of 13 people (seven French, four Italian, one Russian and one British):

  • Erick Bondoux: station leader, electronic technician for science,  France
  • Alexander Kumar: Station physician and ESA biomedical research MD,  United Kingdom
  • Barbara Grolla: nurse anesthetist,  France
  • Guillaume Bouchez: astronomer,  France
  • Alessandro Bambini: electrotechnician,  Italy
  • Stephane Calvo: technical chief,  France
  • Roberto D'Amato: informatician, telecommunications,  Italy
  • Bruno Limouzy: mecanician,  France
  • Mattia Bonazza: glaciologist, atmospheric chemistry,  Italy
  • Giorgio Deidda: chef,  Italy
  • Gérard Guérin: plumber,  France
  • Sebastien Aubin: glaciologist, atmospheric chemistry,  France
  • Igor Petenko: atmospheric science and climate,  Russia.

Ninth winter-over (DC09 – 2013)

The ninth wintering took place with a team of 15 people (nine French, five Italian and one Greek):

  • Anne-Marie Courant: station leader, physician,  France
  • Evangelos Kaimakamis: ESA biomedical research,  Greece
  • Helene Faradji: astronomer,  France
  • Christophe Leroy Dos Santos: astronomer,  France
  • Yann Reinert: astronomer,  France
  • Jean Gabriel Coll: electrician,  France
  • Yannick Marin: technical chief,  France
  • Bruno Epifania: computer, telecommunications,  Italy
  • Simon Reuze: mechanic,  France
  • Elio Padoan: glaciologist, atmospheric chemistry,  Italy
  • Luigi Vailati: chef,  Italy
  • Olivier Delanoë: Plumber,  France
  • Albane Barbero: glaciologist, atmospheric chemistry, meteorological maintenance,  France
  • Antonio Litterio: electronic technician for science,  Italy
  • Simonetta Montaguti: atmospheric science and climate,  Italy

Tenth winter-over (DC10 – 2014)

The tenth wintering took place with a team of 13 people (six French, five Italian, one Russian and one Greek):[12]

  • Bruno Limouzy: Electrical motors,  France
  • Giorgio Deidda: Chef,  Italy
  • Tindari Ceraolo:physician,  Italy
  • Adrianos Golemis: ESA biomedical research,[13]  Greece
  • Pierre Pejoine: Mechanic,  France
  • Paride Legovini: Physicist,[14] Electronic technician for science,  Italy
  • Julien Ribet: Electrotechnician,  France
  • Tommaso Nicosia: Computer, telecommunications,  Italy
  • Daniele Tavagnacco: Astrophysicist,  Italy
  • Olivier Haye: Technical Chief, plumbing and heating,  France
  • Cecile Lenormant: Chemist,  France
  • Igor Petenko: Atmospheric science and climate,  Russia
  • Xavier Joffrin: Astronomy,  France.

During the 2014 Antarctic winter Concordia was an active amateur radio station: Paride Legovini operated from there on a weekly basis with call sign IA/IZ3SUS.[15] The HF radio equipment consists in a Rohde & Schwarz XK2100L transceiver with a 150W RF output and a delta loop antenna located a few hundreds of meters away from the station.[16]

The analemma (path that the sun follows in the sky if photographed at precisely the same time every week through the course of a year) was imaged for the first time ever in Antarctica by Adrianos Golemis during the 10th winterover mission at Concordia Station (2013–2014). The resulting composite exposure image was selected as NASA Astronomy Picture of the Day (APOD) on 23 September 2015.

Eleventh winter-over (DC11 – 2015)

The eleventh wintering is taking place from February 2015 to November 2015 with a team of 13 people (six French, five Italian, one British and one Swiss):[17]

  • Mario Salza: Station Leader, Information and Communications Technology (ICT),  Italy
  • Yannick Marin: Technical Manager and Electrical motors,  France
  • Antonietta Roveran: Physician,  Italy
  • Roxanne Jacob: Glaciology and Atmospheric Chemistry,  France
  • Luca Ficara: Chef,  Italy
  • Guillaume Poirot: Mechanic,  France
  • Giampietro Casasanta: Glaciology and Atmospheric Remote Sensing,  Italy
  • Benoit Laurent: Electronics for Science,  France
  • Markus Wildi: Astrophysics,   Switzerland
  • Benoit Joncheray: Plumbing and Heating Engineering Technician,  France
  • Lorenzo Moggio: Atmospheric Physics,  Italy
  • Beth Healey: ESA Biomedical Research,  United Kingdom
  • Rémi Puaud: Electrical Engineering Technician,  France

Twelfth winter-over (DC12 – 2016)

The twelfth winter began on February 10, 2016, with twelve overwintering (five Italian, six French, one Dutch):

  • Elvio Lazzarini: Physician,  Italy
  • Alessandro Fausto: Information and Communications Technology (ICT),  Italy
  • Luciano Milano: Electronics for Science,  Italy
  • Vitale Stanzione: Station Leader, Glaciology,  Italy
  • Bertrand Bonnefoy: Chef,  France
  • Floris van den Berg: ESA Biomedical Research MD,  the Netherlands
  • Georges Karakasidis: Electrician,  France
  • Henri van den Hove: Plumbing and Heating Engineering Technician,  France
  • Olivier Leloir: Technical Chief,  France
  • Gaetan Quere: Mechanic,  France
  • Simonetta Montaguti: Atmospheric Science and Climate,  Italy
  • Nicole Hueber: Glaciology and Atmospheric Chemistry,  France

Thirteenth winter-over (DC13 – 2017)

The thirteenth winter began on February 9, 2017, with thirteen overwintering (five French, seven Italian, one Belgian Canadian):

  • Simone Chicarella: Electronics for Science, Station Leader,  Italy
  • Andrea Tosti: Information and Communications Technology (ICT).  Italy
  • Didier L'Hôte: Technical Chief,  France
  • Aldo Clemenza: Medical Doctor,  Italy
  • Simone Marcolin: Chef,  Italy
  • Laura Caiazzo: Glaciology and Atmospheric Chemistry,  Italy
  • Sébastien Jullien-Palletier: Electrician,  France
  • Yuri de Prà: Astronomy,  Italy
  • Carole Dangoisse: ESA Biomedical Research MD,  Belgium  Canada
  • Alexis Robin: Plumbing and Heating Engineering Technician,  France
  • Pol Monfort: Mechanic,  France
  • Alfonso Ferrone: Atmospheric Science and Climate,  Italy
  • Paul Serre: Chemistry,  France

Fourteenth winter-over (DC14 – 2018)

The fourteenth winter began on February 6, 2018, with thirteen overwintering (five French, seven Italian, one Austrian):

  • Moreno Baricevic: Electronics for Science,  Italy
  • Remi Bras: Electrician,  France
  • Coline Bouchayeur: Glaciology and Atmospheric Chemistry,  France
  • Andre Bourre: Technical Chief,  France
  • Marco Buttu: Astronomy,  Italy
  • Filippo Cali' Quaglia: Atmospheric Science and Climate,  Italy
  • Florentin Camus: Plumbing and Heating Engineering Technician,  France
  • Mario Giorgioni: Information and Communications Technology (ICT),  Italy
  • Carmen Possnig: ESA Biomedical Research MD,  Austria
  • Jacques Rattel: Mechanic,  France
  • Alberto Razeto: Medical Doctor,  Italy
  • Marco Smerilli: Chef,  Italy
  • Cyprien Verseux: Glaciology and Atmospheric Chemistry, Station Leader,  France  Italy

Fifteenth winter-over (DC15 – 2019)

The fifteenth winter began on February 13, 2019, with thirteen overwintering (five French, six Italian, one Danish and one Australian):

  • Nadja Albertsen: ESA Biomedical Research MD,  Denmark
  • Damien Beloin: Mechanic,  France
  • Ivan Bruni: Astronomy,  Italy
  • Massimiliano Catricalà: Electronics for Science, Station Leader,  Italy
  • Giuditta Celli: Glaciology and Atmospheric Chemistry,  Italy
  • Meganne Louise Christian: Atmospheric Science and Climate,  Australia  Italy
  • Gianluca Ghiselli: Medical Doctor,  Italy
  • Daniele Giambruno: Chef,  Italy
  • Thibault Gillet: Electrician,  France
  • Bertrand Laine: Technical Chief,  France
  • Julien Le Goff: Plumbing and Heating Engineering Technician,  France
  • Alessandro Mancini: Information and Communications Technology (ICT),  Italy
  • Julien Moyé: Glaciology and Atmospheric Chemistry,  France

Sixteenth winter-over (DC16 – 2020)

The sixteenth winter began on February 7, 2020, with twelve overwintering (seven French, four Italian, one Dutch):

  • Camille Bréant: Glaciology and Atmospheric Chemistry,  France
  • Elisa Calmon: Chef,  France
  • Andrea Ceinini: Mechanic,  Italy
  • Loredana Faraldi: Medical Doctor,  Italy
  • Sylvain Guesnier: Chief of the power plant,  France
  • Luca Ianniello: Information and Communications Technology (ICT),  Italy
  • Vivien Koutcheroff: Plumbing and Technical Chief,  France
  • Wenceslas Marie Sainte: Electronics for Science,  France
  • Inès Ollivier: Glaciology and Atmospheric Chemistry,  France
  • Bastien Prat: Electrician,  France
  • Alberto Salvati: Atmospheric Science and Climate, Station Leader,  Italy
  • Stijn Thoolen: ESA Biomedical Research MD,  Netherlands

See also

References
  1. "AT03 Concordia Station". Airport Nav Finder. Retrieved 15 October 2018.
  2. Akshat, Rathi (14 August 2015). "What life is like in the most remote corner of the world". Quartz. Retrieved 12 November 2018.
  3. Salam, Alex (2009). "The coldest job on earth". BMJ: b2453. doi:10.1136/bmj.b2453.
  4. "In the Cornucopia of the European Project of Ice Coring in Antarctica: the oldest Antarctic ice core" (Press release). Alfred-Wegener-Institut. 13 January 2005. Archived from the original on 3 January 2006.
  5. Abdelkrim Agabi; Eric Aristidi; Max Azouit; Eric Fossat; Francois Martin; Tatiana Sadibekova; Jean Vernin; Aziz Ziad (2006). "First whole atmosphere night-time seeing measurements at Dome C, Antarctica". Proceedings of the Astronomical Society of the Pacific. 118 (840): 344–348. arXiv:astro-ph/0510418. Bibcode:2006PASP..118..344A. doi:10.1086/498728.
  6. Jon S. Lawrence; Michael C. B. Ashley; Andrei Tokovinin; Tony Travouillon (16 September 2004). "Exceptional astronomical seeing conditions above Dome C in Antarctica" (PDF). Nature. 431 (7006): 278–281. Bibcode:2004Natur.431..278L. doi:10.1038/nature02929. PMID 15372024. Archived from the original (PDF) on 25 March 2006. → FAQ by the authors Archived 15 February 2006 at the Wayback Machine
  7. {Vernin, J., Chadid, M., Aristidi, E., Trinquet, H. and van der Swaelmen, M.}, title = "{First single star scidar measurements at Dome C, Antarctica}", journal = {AP}, keywords = {atmospheric effects, site testing, turbulence, instrumentation: detectors, methods: data analysis, methods: observational}, year = 2009, month = jun, volume = 500, pages = {1271-1276}, doi = {10.1051/0004-6361/200811119}, adsurl = {http://cdsads.u-strasbg.fr/abs/2009A%26A...500.1271V}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} }
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