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GIOVANNI PERES

ADAHELI+: exploring the fast, dynamic Sun in the x-ray, optical, and near-infrared

  • Authors: Berrilli, F.; Soffitta, P.; Velli, M.; Sabatini, P.; Bigazzi, A.; Bellazzini, R.; Bellot Rubio, L.; Brez, A.; Carbone, V.; Cauzzi, G.; Cavallini, F.; Consolini, G.; Curti, F.; Del Moro, D.; Di Giorgio, A.; Ermolli, I.; Fabiani, S.; Faurobert, M.; Feller, A.; Galsgaard, K.; Gburek, S.; Giannattasio, F.; Giovannelli, L.; Hirzberger, J.; Jefferies, S.; Madjarska, M.; Manni, F.; Mazzoni, A.; Muleri, F.; Penza, V.; Peres, G.; Piazzesi, R.; Pieralli, F.; Pietropaolo, E.; Pillet, V.; Pinchera, M.; Reale, F.; Romano, P.; Romoli, A.; Romoli, M.; Rubini, A.; Rudawy, P.; Sandri, P.; Scardigli, S.; Spandre, G.; Solanki, S.; Stangalini, M.; Vecchio, A.; Zuccarello, F.
  • Publication year: 2015
  • Type: Articolo in rivista (Articolo in rivista)
  • OA Link: http://hdl.handle.net/10447/226160

Abstract

Advanced Astronomy for Heliophysics Plus (ADAHELI+) is a project concept for a small solar and space weather mission with a budget compatible with an European Space Agency (ESA) S-class mission, including launch, and a fast development cycle. ADAHELI+ was submitted to the European Space Agency by a European-wide consortium of solar physics research institutes in response to the "Call for a small mission opportunity for a launch in 2017," of March 9, 2012. The ADAHELI+ project builds on the heritage of the former ADAHELI mission, which had successfully completed its phase-A study under the Italian Space Agency 2007 Small Mission Programme, thus proving the soundness and feasibility of its innovative low-budget design. ADAHELI+ is a solar space mission with two main instruments: ISODY+: an imager, based on Fabry-Perot interferometers, whose design is optimized to the acquisition of highest cadence, long-duration, multiline spectropolarimetric images in the visible/near-infrared region of the solar spectrum. XSPO: an x-ray polarimeter for solar flares in x-rays with energies in the 15 to 35 keV range. ADAHELI+ is capable of performing observations that cannot be addressed by other currently planned solar space missions, due to their limited telemetry, or by ground-based facilities, due to the problematic effect of the terrestrial atmosphere. (C) The Authors. Published by SPIE under a Creative Commons Attribution 3.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.