ADvanced Astronomy for HELIophysics (ADAHELI) is a Small Mission to study the structure and fast dynamics of the low solar atmosphere, performing Visible-NIR monochromatic and broad-band observations. The mission will achieve millimeter full disk observations as well. The ADAHELI Team has succesfully completed, in December 2008, the Phase A study awarded by the Italian Space Agency (ASI). The Interferometer for SOlar Dynamics (ISODY), on board the ADAHELI satellite, comprises a Gregorian telescope and its focal plane suite. The advanced design focal plane suite uses fast CMOS cameras for investigating photospheric and chromospheric fast dynamics and structure. ISODY is equipped with a pioneering focal plane suite composed of a spectral channel, based upon a tandem of Fabry-Perot interferometers operating in the visible-NIR spectral region, a broad band channel for high resolution imaging, and a correlation tracker used as an image stabilization system. ADAHELI's mission profile has been tailored to limit the spacecraft' s radial velocity in the Sunward direction, to not exceed ?4 km/s, during 95% of the yearly orbit, to allow a continuous use of the on-board interferometer.

The telescope and the double Fabry-Pérot interferometer for the ADAHELI solar space mission / V. Greco, F. Cavallini, F. Berrilli, M. Velli, L. Roselli, A Bigazzi, P. F. Moretti, M. Romoli, S. Orsini, P. Sabatini, V. Carbone, G. Consolini, M. P. Di Mauro, I Ermolli, E. Pietropaolo, P. Romano, P. Ventura, L. Valdettaro, S. M. White, F. Zuccarello, et al.. - STAMPA. - (2010), pp. 773142-773142-9. [10.1117/12.856617]

The telescope and the double Fabry-Pérot interferometer for the ADAHELI solar space mission.

VELLI, MARCO;ROMOLI, MARCO;LANDI, SIMONE;
2010

Abstract

ADvanced Astronomy for HELIophysics (ADAHELI) is a Small Mission to study the structure and fast dynamics of the low solar atmosphere, performing Visible-NIR monochromatic and broad-band observations. The mission will achieve millimeter full disk observations as well. The ADAHELI Team has succesfully completed, in December 2008, the Phase A study awarded by the Italian Space Agency (ASI). The Interferometer for SOlar Dynamics (ISODY), on board the ADAHELI satellite, comprises a Gregorian telescope and its focal plane suite. The advanced design focal plane suite uses fast CMOS cameras for investigating photospheric and chromospheric fast dynamics and structure. ISODY is equipped with a pioneering focal plane suite composed of a spectral channel, based upon a tandem of Fabry-Perot interferometers operating in the visible-NIR spectral region, a broad band channel for high resolution imaging, and a correlation tracker used as an image stabilization system. ADAHELI's mission profile has been tailored to limit the spacecraft' s radial velocity in the Sunward direction, to not exceed ?4 km/s, during 95% of the yearly orbit, to allow a continuous use of the on-board interferometer.
2010
Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave
773142
773142-9
V. Greco; F. Cavallini; F. Berrilli; M. Velli; L. Roselli; A Bigazzi; P. F. Moretti; M. Romoli; S. Orsini; P. Sabatini; V. Carbone; G. Consolini; M. P...espandi
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/939334
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