Contributo in atti di convegno, 2002, ENG, 10.1117/12.459804
Naletto, G., Da Deppo, V., Nicolosi, P. ,Zambolin, P., Barbieri, C. and Fornasier, S.
University of Padova (Italy), Dept. of Information Engineering, Padova, Italy; University of Padova (Italy), C.I.S.A.S., Padova, Italy; INFM, Unity of Padova (Italy), Padova, Italy; University of Padova (Italy), Department of Astronomy, Padova, Italy
Rosetta is one of the cornerstone missions of the European Space Agency for having a roundez-vous with the periodic comet P/Wirtanen in 2011. One of the imaging instruments on board the satellite is the Wide Angle Camera, a cooperation among several european institutes. This camera adopts an all reflecting, unvignetted unobstructed two mirror configuration which allows to cover a 12° × 12° Field of View with an F/5.6 aperture and an optical quality better than 80% geometrical ensquared energy inside approximately 20 arcsec. The flight model of this camera has been successfully integrated and tested in our laboratories and finally has been integrated on the satellite. In this paper we are going to describe the optical characteristics of the camera, and to summarize the results so far obtained with the preliminary calibration data. The analysis of the optical performance of this model shows a good agreement between theoretical performance and experimental results.
SPIE Astronomical Telescope, pp. 375–384, 22-23/08/2002
Aspherics, Calibration, Cameras, Galaxies, Image quality, Interplanetary flight, Mathematical models, Mirrors, Imaging instruments, Optical quality, Rosetta mission, Space instrumentation, Wide angle camera, Imaging systems
Naletto Giampiero, Nicolosi Piergiorgio, Da Deppo Vania
ID: 246354
Year: 2002
Type: Contributo in atti di convegno
Creation: 2013-08-01 19:13:03.000
Last update: 2020-08-30 21:33:28.000
CNR institutes
External IDs
CNR OAI-PMH: oai:it.cnr:prodotti:246354
DOI: 10.1117/12.459804
Scopus: 2-s2.0-0038781954
ISI Web of Science (WOS): 000182019200037