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
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