Artigo Revisado por pares

The spectrometer/telescope for imaging X-rays on board the ESA Solar Orbiter spacecraft

2013; Elsevier BV; Volume: 732; Linguagem: Inglês

10.1016/j.nima.2013.05.050

ISSN

1872-9576

Autores

Säm Krucker, A. O. Benz, G. J. Hurford, Nicolas Arnold, P. Orleański, Hans-Peter Gröbelbauer, D. Casadei, S. Kobler, L. Iseli, H. J. Wiehl, A. Csillaghy, L. Etesi, N. Hochmuth, M. Battaglia, Martin Bednarzik, R. Resanovic, O. Grimm, G. Viertel, V. Commichau, Andrew W. Howard, A. Meuris, O. Limousin, S. Brun, Nicole Vilmer, Konrad Skup, Rafał Graczyk, M. Stolarski, M. Michalska, Witold Nowosielski, Andrzej Cichocki, M. Mosdorf, Karol Seweryn, Agnieszka Białek, J. Sylwester, Mirosław Kowaliński, Tomasz Mrozek, P. Pоdgórski, G. Mann, Hakan Önel, H. Auraß, Svend‐Marian Bauer, Wilbert Bittner, Frank Dionies, J. Paschke, D. Plüschke, Emil Popow, J. Rendtel, A. Warmuth, M. Woche, Dieter Wolter, H. F. van Beek, F. Fárník, R. P. Lin,

Tópico(s)

Atmospheric Ozone and Climate

Resumo

Solar Orbiter is a Sun-observing mission led by the European Space Agency, addressing the interaction between the Sun and the heliosphere. It will carry ten instruments, among them the X-ray imaging spectrometer STIX. STIX will determine the intensity, spectrum, timing, and location of thermal and accelerated electrons near the Sun through their bremsstrahlung X-ray emission. This report gives a brief overview of the STIX scientific goals and covers in more detail the instrument design and challenges.

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