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

Giovanni Peres, Fabio Reale, Gloria Spandre, Fabio Muleri, Valentin Martinez Pillet, Michele Pinchera, Sergio Fabiani, Paolo Romano, Vincenzo Carbone, Marco Stangalini, Fabio Manni, Roberto Piazzesi, Alex Feller, Fabio Cavallini, Fabio Giannattasio, Luca Giovannelli, Francesca Zuccarello, Alda Rubini, Stefano Scardigli, Pawel RudawyRonaldo Bellazzini, Gloria Spandre, Alessandro Mazzoni, Paolo Sandri, Francesca Pieralli, Valentin Martinez Pillet, Stuart M. Jefferies, Paolo Sandri, Fabio Manni, Alessandro Mazzoni, Paolo Sandri, Fabio Manni, Ermanno Pietropaolo, Paolo Sabatini, Johann Hirzberger, Alberto Bigazzi, Valentina Penza, Marianne Faurobert, Ilaria Ermolli, Gianna Cauzzi, Dario Del Moro, Szymon Gburek, Pawel Rudawy, Maria S. Madjarska, Paolo Sandri, Andrea Romoli, Klaus Galsgaard, Paolo Sandri, Giuseppe Consolini, Fabio Curti, Francesco Berrilli, Marco Velli, Luis Ramon Bellot Rubio, Alessandro Brez, Paolo Soffitta, Sami K. Solanki, Marco Romoli, Anna Maria Di Giorgio, Antonio Vecchio

Risultato della ricerca: Articlepeer review

10 Citazioni (Scopus)


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.
Lingua originaleEnglish
Numero di pagine15
RivistaJournal of Astronomical Telescopes, Instruments, and Systems
Stato di pubblicazionePublished - 2015

All Science Journal Classification (ASJC) codes

  • ???subjectarea.asjc.2500.2504???
  • ???subjectarea.asjc.2200.2207???
  • ???subjectarea.asjc.3100.3105???
  • ???subjectarea.asjc.3100.3103???
  • ???subjectarea.asjc.2200.2210???
  • ???subjectarea.asjc.1900.1912???


Entra nei temi di ricerca di 'ADAHELI+: exploring the fast, dynamic Sun in the x-ray, optical, and near-infrared'. Insieme formano una fingerprint unica.

Cita questo