PROBA-3 is a mission devoted to the in-orbit demonstration of precise formation flying techniques and technologies for future ESA missions. PROBA-3 will fly ASPIICS (Association de Satellites pour l'Imagerie et l'Interferométrie de la Couronne Solaire) as primary payload, which makes use of the formation flying technique to form a giant coronagraph capable of producing a nearly perfect eclipse allowing to observe the sun corona closer to the rim than ever before. The coronagraph is distributed over two satellites flying in formation (approx. 150m apart). The so called Coronagraph Satellite carries the camera and the so called Occulter Satellite carries the sun occulter disc. This paper is reviewing the design and evolution of the ASPIICS instrument as at the beginning of Phase C/D.

ASPIICS: an externally occulted coronagraph for PROBA-3: Design evolution / E. Renotte;E. C. Baston;A. Bemporad;G. Capobianco;I. Cernica;R. Darakchiev;F. Denis;R. Desselle;L. D. Vos;S. Fineschi;M. Focardi;T. Górski;R. Graczyk;J. Halain;A. Hermans;C. Jackson;C. Kintziger;J. Kosiec;N. Kranitis;F. Landini;V. Lédl;G. Massone;A. Mazzoli;R. Melich;D. Mollet;M. Mosdorf;G. Nicolini;B. Nicula;P. Orleański;M. Palau;M. Pancrazzi;A. Paschalis;R. Peresty;J. Plesseria;M. Rataj;M. Romoli;C. Thizy;M. Thomé;K. Tsinganos;R. Wodnicki;T. Walczak;A. Zhukov. - ELETTRONICO. - 9143:(2014), pp. 1-15. (Intervento presentato al convegno Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave tenutosi a Montreal (Canada) nel 22-27 June 2014) [10.1117/12.2056784].

ASPIICS: an externally occulted coronagraph for PROBA-3: Design evolution

CAPOBIANCO, GIADA;S. Fineschi;MAZZOLI, ANNA RITA;M. Pancrazzi;M. Romoli;
2014

Abstract

PROBA-3 is a mission devoted to the in-orbit demonstration of precise formation flying techniques and technologies for future ESA missions. PROBA-3 will fly ASPIICS (Association de Satellites pour l'Imagerie et l'Interferométrie de la Couronne Solaire) as primary payload, which makes use of the formation flying technique to form a giant coronagraph capable of producing a nearly perfect eclipse allowing to observe the sun corona closer to the rim than ever before. The coronagraph is distributed over two satellites flying in formation (approx. 150m apart). The so called Coronagraph Satellite carries the camera and the so called Occulter Satellite carries the sun occulter disc. This paper is reviewing the design and evolution of the ASPIICS instrument as at the beginning of Phase C/D.
2014
Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Montreal (Canada)
22-27 June 2014
E. Renotte;E. C. Baston;A. Bemporad;G. Capobianco;I. Cernica;R. Darakchiev;F. Denis;R. Desselle;L. D. Vos;S. Fineschi;M. Focardi;T. Górski...espandi
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/965262
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