Solar magnetism eXplorer (SolmeX). Exploring the magnetic field in the upper atmosphere of our closest star
Autor: | N.-E. Raouafi, Sami K. Solanki, Bernd Inhester, Dominik Quantius, Andy Braukhane, Luca Teriaca, D. Moses, Oliver Romberg, V. Martínez Pillet, Hansjörg Dittus, John C. Raymond, Andreas Lagg, Silvano Fineschi, Andrzej Fludra, Véronique Bommier, Jean-Claude Vial, Douglas Griffin, S. Parenti, R. Manso Sainz, Werner Curdt, Francesco Berrilli, A. Pietarila, P. Rochus, J. Trujillo Bueno, Volker Maiwald, Steven Tomczyk, Markus Schlotterer, V. Andretta, Sarah A. Matthews, E. Landi Degl'Innocenti, Joseph M. Davila, Lucia Abbo, Achim Gandorfer, Alessandro Bemporad, F. Auchere, Udo H. Schuehle, Roberto Casini, Hardi Peter, Daniele Spadaro |
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Jazyk: | angličtina |
Rok vydání: | 2011 |
Předmět: |
ESA Cosmic Vision
Magnetism Solar eclipse Extreme ultraviolet lithography Astrophysics 01 natural sciences 7. Clean energy 010309 optics Atmosphere Settore FIS/05 - Astronomia e Astrofisica 0103 physical sciences Astrophysics::Solar and Stellar Astrophysics Space vehicles: instruments 010303 astronomy & astrophysics Physics Spacecraft business.industry Sun: atmosphere Magnetic fields Space vehicles: instruments Techniques: polarimetic ESA Cosmic Vision Sun: atmosphere - Magnetic fields - Space vehicles: instruments - Techniques: polarimetic - ESA Cosmic Vision - Concurrent Engineering Astrophysics::Instrumentation and Methods for Astrophysics Astronomy and Astrophysics Polarization (waves) Corona Magnetic field Techniques: polarimetic Space and Planetary Science Magnetic fields Physics::Space Physics Astrophysics::Earth and Planetary Astrophysics business Sun: atmosphere |
Popis: | The magnetic field plays a pivotal role in many fields of Astrophysics. This is especially true for the physics of the solar atmosphere. Measuring the magnetic field in the upper solar atmosphere is crucial to understand the nature of the underlying physical processes that drive the violent dynamics of the solar corona -- that can also affect life on Earth. SolmeX, a fully equipped solar space observatory for remote-sensing observations, will provide the first comprehensive measurements of the strength and direction of the magnetic field in the upper solar atmosphere. The mission consists of two spacecraft, one carrying the instruments, and another one in formation flight at a distance of about 200m carrying the occulter to provide an artificial total solar eclipse. This will ensure high-quality coronagraphic observations above the solar limb. Solmex integrates two spectro-polarimetric coronagraphs for off-limb observations, one in the EUV and one in the IR, and three instruments for observations on the disk. The latter comprises one imaging polarimeter in the EUV for coronal studies, a spectro-polarimeter in the EUV to investigate the low corona, and an imaging spectro-polarimeter in the UV for chromospheric studies. SOHO and other existing missions have investigated the emission of the upper atmosphere in detail (not considering polarization), and as this will be the case also for missions planned for the near future. Therefore it is timely that SolmeX provides the final piece of the observational quest by measuring the magnetic field in the upper atmosphere through polarimetric observations. |
Databáze: | OpenAIRE |
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