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The European Solar Telescope

MPS-Authors
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Gunár,  S.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Barczynski,  K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons92136

Beck,  C.
Department of Molecular Neurobiology, Max Planck Institute for Medical Research, Max Planck Society;

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Danilovic,  S.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Del Moro,  D.
Max Planck Institute for Solar System Research, Max Planck Society;

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Feller,  A.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Gafeira,  R.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
International Max Planck Research School for Solar System Science at the University of Göttingen, Max Planck Institute for Solar System Research, Max Planck Society;

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Grauf,  B.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Heinzel,  P.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Krishnappa,  N.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Manso Sainz,  R.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Matthews,  S.
Programming Logics, MPI for Informatics, Max Planck Society;

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Peter,  H.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Pleier,  O.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Riethmüller,  T. L.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Solanki,  S. K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Stangalini,  M.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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van Noort,  M.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Verma,  M.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Vögler,  A.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Zeman,  J.
High Magnetic Field Laboratory, Former Departments, Max Planck Institute for Solid State Research, Max Planck Society;

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Zeuner,  F.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
IMPRS for Solar System Science at the University of Göttingen, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Quintero Noda, C., Schlichenmaier, R., Bellot Rubio, L. R., Löfdahl, M. G., Khomenko, E., Jurčák, J., et al. (2022). The European Solar Telescope. Astronomy and Astrophysics, 666, A21. doi:10.1051/0004-6361/202243867.


Cite as: https://hdl.handle.net/21.11116/0000-000C-B25B-5
Abstract
The European Solar Telescope (EST) is a project aimed at studying the magnetic connectivity of the solar atmosphere, from the deep photosphere to the upper chromosphere. Its design combines the knowledge and expertise gathered by the European solar physics community during the construction and operation of state-of-the-art solar telescopes operating in visible and near-infrared wavelengths: the Swedish 1m Solar Telescope, the German Vacuum Tower Telescope and GREGOR, the French Télescope Héliographique pour l'Étude du Magnétisme et des Instabilités Solaires, and the Dutch Open Telescope. With its 4.2 m primary mirror and an open configuration, EST will become the most powerful European ground-based facility to study the Sun in the coming decades in the visible and near-infrared bands. EST uses the most innovative technological advances: the first adaptive secondary mirror ever used in a solar telescope, a complex multi-conjugate adaptive optics with deformable mirrors that form part of the optical design in a natural way, a polarimetrically compensated telescope design that eliminates the complex temporal variation and wavelength dependence of the telescope Mueller matrix, and an instrument suite containing several (etalon-based) tunable imaging spectropolarimeters and several integral field unit spectropolarimeters. This publication summarises some fundamental science questions that can be addressed with the telescope, together with a complete description of its major subsystems.