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–Pérot 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

ADAHELI+: Exploring the fast, dynamic Sun in the X-ray, optical, and near-infrared / Berrilli, F., Soffitta, P., Velli, M., Sabatini, P., Bigazzi, A., Bellazzini, R., Bellot Rubio, L.R., Brez, A., Carbone, V., Cauzzi, G., Cavallini, F., Consolini, G., Curti, F., Del Moro, D., Di Giorgio, A.M., Ermolli, I., Fabiani, S., Faurobert, M., Feller, A., Galsgaard, K., et al.. - In: JOURNAL OF ASTRONOMICAL TELESCOPES, INSTRUMENTS, AND SYSTEMS. - ISSN 2329-4124. - STAMPA. - 1:4(2015), p. 044006. [10.1117/1.JATIS.1.4.044006]

ADAHELI+: Exploring the fast, dynamic Sun in the X-ray, optical, and near-infrared

CURTI, Fabio;
2015

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–Pérot 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
2015
Fabry-Pérot; infrared spectroscopy; polarimetry; satellites; Sun; X-rays; Control and Systems Engineering; Electronic, Optical and Magnetic Materials; Instrumentation; Astronomy and Astrophysics; Mechanical Engineering; Space and Planetary Science
01 Pubblicazione su rivista::01a Articolo in rivista
ADAHELI+: Exploring the fast, dynamic Sun in the X-ray, optical, and near-infrared / Berrilli, F., Soffitta, P., Velli, M., Sabatini, P., Bigazzi, A., Bellazzini, R., Bellot Rubio, L.R., Brez, A., Carbone, V., Cauzzi, G., Cavallini, F., Consolini, G., Curti, F., Del Moro, D., Di Giorgio, A.M., Ermolli, I., Fabiani, S., Faurobert, M., Feller, A., Galsgaard, K., et al.. - In: JOURNAL OF ASTRONOMICAL TELESCOPES, INSTRUMENTS, AND SYSTEMS. - ISSN 2329-4124. - STAMPA. - 1:4(2015), p. 044006. [10.1117/1.JATIS.1.4.044006]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/944171
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