ESCAPE : a first step to high resolution solar coronagraphy in Antarctica

4th French-Chinese Meeting on Solar Physics Understanding Solar Activity: Advances and Challenges, 4th French-Chinese, Nice, France. International audience The Dome C high plateau is unique for coronagraphic observations: sky brightness is reduced, water vapour is low, seeing is excellent and contin...

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Published in:EAS Publications Series
Main Authors: Damé, Luc, Abe, L., Faurobert, M., Fineschi, S., Kuzin, S., Lamy, Philippe, Meftah, Mustapha, Vives, S.
Other Authors: HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Torino (OATo), Istituto Nazionale di Astrofisica (INAF), Laboratory for solar X-ray Astronomy of the Sun, P. N. Lebedev Physical Institute of the Russian Academy of Sciences Moscow (LPI RAS), Russian Academy of Sciences Moscow (RAS)-Russian Academy of Sciences Moscow (RAS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2012
Subjects:
Online Access:https://hal.archives-ouvertes.fr/hal-00717398
https://doi.org/10.1051/eas/1255050
id ftunivnantes:oai:HAL:hal-00717398v1
record_format openpolar
institution Open Polar
collection Université de Nantes: HAL-UNIV-NANTES
op_collection_id ftunivnantes
language English
topic [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
spellingShingle [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
Damé, Luc
Abe, L.
Faurobert, M.
Fineschi, S.
Kuzin, S.
Lamy, Philippe
Meftah, Mustapha
Vives, S.
ESCAPE : a first step to high resolution solar coronagraphy in Antarctica
topic_facet [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
description 4th French-Chinese Meeting on Solar Physics Understanding Solar Activity: Advances and Challenges, 4th French-Chinese, Nice, France. International audience The Dome C high plateau is unique for coronagraphic observations: sky brightness is reduced, water vapour is low, seeing is excellent and continuity of observations on several weeks is possible. ESCAPE (the Extreme Solar Coronagraphy Antarctic Program Experiment) will perform 2-dimensional spectroscopy of the forbidden line of FeXIV at 530.285 nm: precise line profile analysis will allow the diagnostic of the nature of waves by simultaneous measurements of velocities and intensities in the corona. ESCAPE is proposed to Institut Paul-Emile Victor (IPEV) for a campaign in 2012-2013 at Dome C/Concordia since all subsystems are available in particular thanks to an ESA STARTIGER 2010 R&D "Toward a New Generation of Formation Flying Coronagraph". Using state-of-the-art technologies developed for Space missions (a Three Mirrors Anastigmat telescope, the TMA, a 4 stages Liquid Crystal Tunable-filter Polarimeter, the LCTP) allows us to propose an automated Coronal Green Line full-field Polarimeter for unique observations (waves nature and intensity to address coronal heating) with the best possible performances on Earth and for preparing and testing the technologies for the next steps in Space. No other site would allow such coronagraphic performances (the sky brightness is a factor 2 to 4 better than in Hawaï) and with high spatial resolution (better than an arcsec is possible).
author2 HELIOS - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Joseph Louis LAGRANGE (LAGRANGE)
Université Nice Sophia Antipolis (1965 - 2019) (UNS)
COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur
COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)
INAF - Osservatorio Astrofisico di Torino (OATo)
Istituto Nazionale di Astrofisica (INAF)
Laboratory for solar X-ray Astronomy of the Sun
P. N. Lebedev Physical Institute of the Russian Academy of Sciences Moscow (LPI RAS)
Russian Academy of Sciences Moscow (RAS)-Russian Academy of Sciences Moscow (RAS)
Laboratoire d'Astrophysique de Marseille (LAM)
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Damé, Luc
Abe, L.
Faurobert, M.
Fineschi, S.
Kuzin, S.
Lamy, Philippe
Meftah, Mustapha
Vives, S.
author_facet Damé, Luc
Abe, L.
Faurobert, M.
Fineschi, S.
Kuzin, S.
Lamy, Philippe
Meftah, Mustapha
Vives, S.
author_sort Damé, Luc
title ESCAPE : a first step to high resolution solar coronagraphy in Antarctica
title_short ESCAPE : a first step to high resolution solar coronagraphy in Antarctica
title_full ESCAPE : a first step to high resolution solar coronagraphy in Antarctica
title_fullStr ESCAPE : a first step to high resolution solar coronagraphy in Antarctica
title_full_unstemmed ESCAPE : a first step to high resolution solar coronagraphy in Antarctica
title_sort escape : a first step to high resolution solar coronagraphy in antarctica
publisher HAL CCSD
publishDate 2012
url https://hal.archives-ouvertes.fr/hal-00717398
https://doi.org/10.1051/eas/1255050
long_lat ENVELOPE(136.500,136.500,-66.333,-66.333)
geographic Antarctic
Paul-Emile Victor
geographic_facet Antarctic
Paul-Emile Victor
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_source ISSN: 1633-4760
EISSN: 1638-1963
EAS Publications Series
https://hal.archives-ouvertes.fr/hal-00717398
EAS Publications Series, EDP Sciences, 2012, 55, pp.359-364. ⟨10.1051/eas/1255050⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1051/eas/1255050
hal-00717398
https://hal.archives-ouvertes.fr/hal-00717398
doi:10.1051/eas/1255050
op_doi https://doi.org/10.1051/eas/1255050
container_title EAS Publications Series
container_volume 55
container_start_page 359
op_container_end_page 364
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spelling ftunivnantes:oai:HAL:hal-00717398v1 2023-05-15T14:06:28+02:00 ESCAPE : a first step to high resolution solar coronagraphy in Antarctica Damé, Luc Abe, L. Faurobert, M. Fineschi, S. Kuzin, S. Lamy, Philippe Meftah, Mustapha Vives, S. HELIOS - LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Joseph Louis LAGRANGE (LAGRANGE) Université Nice Sophia Antipolis (1965 - 2019) (UNS) COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS) INAF - Osservatorio Astrofisico di Torino (OATo) Istituto Nazionale di Astrofisica (INAF) Laboratory for solar X-ray Astronomy of the Sun P. N. Lebedev Physical Institute of the Russian Academy of Sciences Moscow (LPI RAS) Russian Academy of Sciences Moscow (RAS)-Russian Academy of Sciences Moscow (RAS) Laboratoire d'Astrophysique de Marseille (LAM) Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS) 2012 https://hal.archives-ouvertes.fr/hal-00717398 https://doi.org/10.1051/eas/1255050 en eng HAL CCSD EDP Sciences info:eu-repo/semantics/altIdentifier/doi/10.1051/eas/1255050 hal-00717398 https://hal.archives-ouvertes.fr/hal-00717398 doi:10.1051/eas/1255050 ISSN: 1633-4760 EISSN: 1638-1963 EAS Publications Series https://hal.archives-ouvertes.fr/hal-00717398 EAS Publications Series, EDP Sciences, 2012, 55, pp.359-364. ⟨10.1051/eas/1255050⟩ [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] info:eu-repo/semantics/article Journal articles 2012 ftunivnantes https://doi.org/10.1051/eas/1255050 2022-08-09T23:04:03Z 4th French-Chinese Meeting on Solar Physics Understanding Solar Activity: Advances and Challenges, 4th French-Chinese, Nice, France. International audience The Dome C high plateau is unique for coronagraphic observations: sky brightness is reduced, water vapour is low, seeing is excellent and continuity of observations on several weeks is possible. ESCAPE (the Extreme Solar Coronagraphy Antarctic Program Experiment) will perform 2-dimensional spectroscopy of the forbidden line of FeXIV at 530.285 nm: precise line profile analysis will allow the diagnostic of the nature of waves by simultaneous measurements of velocities and intensities in the corona. ESCAPE is proposed to Institut Paul-Emile Victor (IPEV) for a campaign in 2012-2013 at Dome C/Concordia since all subsystems are available in particular thanks to an ESA STARTIGER 2010 R&D "Toward a New Generation of Formation Flying Coronagraph". Using state-of-the-art technologies developed for Space missions (a Three Mirrors Anastigmat telescope, the TMA, a 4 stages Liquid Crystal Tunable-filter Polarimeter, the LCTP) allows us to propose an automated Coronal Green Line full-field Polarimeter for unique observations (waves nature and intensity to address coronal heating) with the best possible performances on Earth and for preparing and testing the technologies for the next steps in Space. No other site would allow such coronagraphic performances (the sky brightness is a factor 2 to 4 better than in Hawaï) and with high spatial resolution (better than an arcsec is possible). Article in Journal/Newspaper Antarc* Antarctic Antarctica Université de Nantes: HAL-UNIV-NANTES Antarctic Paul-Emile Victor ENVELOPE(136.500,136.500,-66.333,-66.333) EAS Publications Series 55 359 364