Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE): I. Coronal Heating
| Autor: | De Pontieu, Bart, Testa, Paola, Martinez-Sykora, Juan, Antolin, Patrick, Karampelas, Konstantinos, Hansteen, Viggo, Rempel, Matthias, Cheung, Mark C. M., Reale, Fabio, Danilovic, Sanja, Pagano, Paolo, Polito, Vanessa, De Moortel, Ineke, Nobrega-Siverio, Daniel, Van Doorsselaere, Tom, Petralia, Antonino, Asgari-Targhi, Mahboubeh, Boerner, Paul, Carlsson, Mats, Chintzoglou, Georgios, Daw, Adrian, DeLuca, Ed, Golub, Leon, Matsumoto, Takuma, Ugarte-Urra, Ignacio, McIntosh, Scott, team, the MUSE |
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| Přispěvatelé: | De Pontieu B., Testa P., Martinez-Sykora J., Antolin P., Karampelas K., Hansteen V., Rempel M., Cheung M.C.M., Reale F., Danilovic S., Pagano P., Polito V., De Moortel I., Nobrega-Siverio D., Van Doorsselaere T., Petralia A., Asgari-Targhi M., Boerner P., Carlsson M., Chintzoglou G., Daw A., Deluca E., Golub L., Matsumoto T., Ugarte-Urra I., McIntosh S.W., European Research Council, Science & Technology Facilities Council, University of St Andrews. Applied Mathematics, University of St Andrews. Office of the Principal |
| Jazyk: | angličtina |
| Rok vydání: | 2021 |
| Předmět: |
F300
FOS: Physical sciences F500 Astronomy & Astrophysics ACTIVE-REGION EVENTS FLOWS Solar coronal heating Theoretical models Solar instruments INTERFACE-REGION MAGNETIC RECONNECTION QB Astronomy TRANSITION REGION Instrumentation and Methods for Astrophysics (astro-ph.IM) Solar and Stellar Astrophysics (astro-ph.SR) QC QB MCC Science & Technology HOT PLASMA Astronomy and Astrophysics 3rd-DAS ALFVENIC WAVES SIMULATIONS QC Physics Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science Physical Sciences EUV IMAGING SPECTROMETER Astrophysics - Instrumentation and Methods for Astrophysics |
| ISSN: | 0004-637X |
| Popis: | The Multi-slit Solar Explorer (MUSE) is a proposed NASA MIDEX mission, currently in Phase A, composed of a multi-slit EUV spectrograph (in three narrow spectral bands centered around 171A, 284A, and 108A) and an EUV context imager (in two narrow passbands around 195A and 304A). MUSE will provide unprecedented spectral and imaging diagnostics of the solar corona at high spatial ( 46 pages, 22 figures, submitted to ApJ |
| Databáze: | OpenAIRE |
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