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

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

Journal
JOURNAL OF ASTRONOMICAL TELESCOPES, INSTRUMENTS, AND SYSTEMS  
Date Issued
2015
Author(s)
BERRILLI, FRANCESCO
•
SOFFITTA, PAOLO  
•
VELLI, MARCO  
•
Sabatini, Paolo
•
Bigazzi, Alberto
•
Bellazzini, Ronaldo
•
Bellot Rubio, Luis Ramon
•
Brez, Alessandro
•
CARBONE, VINCENZO
•
CAUZZI, Gianna  
•
CAVALLINI, Fabio
•
CONSOLINI, Giuseppe  
•
Curti, Fabio
•
DEL MORO, DARIO
•
DI GIORGIO, Anna Maria  
•
ERMOLLI, Ilaria  
•
FABIANI, Sergio  
•
Faurobert, Marianne
•
Feller, Alex
•
Galsgaard, Klaus
•
Gburek, Szymon
•
Giannattasio, Fabio
•
GIOVANNELLI, LUCA  
•
Hirzberger, Johann
•
Jefferies, Stuart M.
•
Madjarska, Maria S.
•
Manni, Fabio
•
Mazzoni, Alessandro
•
MULERI, FABIO  
•
Penza, Valentina
•
Peres, Giovanni  
•
PIAZZESI, ROBERTO  
•
Pieralli, Francesca
•
PIETROPAOLO, ERMANNO  
•
Martinez Pillet, Valentin
•
Pinchera, Michele
•
Reale, Fabio  
•
ROMANO, Paolo  
•
Romoli, Andrea
•
ROMOLI, MARCO  
•
RUBINI, ALDA  
•
Rudawy, Pawel
•
Sandri, Paolo
•
Scardigli, Stefano
•
Spandre, Gloria
•
Solanki, Sami K.
•
STANGALINI, MARCO  
•
Vecchio, Antonio
•
Zuccarello, Francesca  
DOI
10.1117/1.JATIS.1.4.044006
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.
Volume
1
Issue
4
Start page
044006
Uri
http://hdl.handle.net/20.500.12386/24020
Url
https://www.spiedigitallibrary.org/journals/Journal-of-Astronomical-Telescopes-Instruments-and-Systems/volume-1/issue-04/044006/ADAHELI--exploring-the-fast-dynamic-Sun-in-thex-ray/10.1117/1.JATIS.1.4.044006.full?SSO=1
Issn Identifier
2329-4124
Ads BibCode
2015JATIS...1d4006B
Rights
open.access
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2015_JATIS_Berrilli.pdf

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Size

1.8 MB

Format

Adobe PDF

Checksum (MD5)

dc2e952b38a0d11b32369a322dde11ef

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