The Antarctica solar coronagraph - AntarctiCor- for the "Extreme Solar Coronagraphy Antarctic Program Experiment" -ESCAPE- comprises an internally-occulted coronagraph based on the externally-occulted ASPIICS coronagraph for the ESA formation-flying PROBA-3 mission. This paper describes the AntarctiCor design for ground-based observations from the DomeC Antarctica plateau of the polarized broad-band (591 nm ± 5 nm) K-corona and of the narrow-band (FWHM = 0.5 nm), polarized emission of the coronal green-line at 530.3 nm. The science goal of these observations is to map the topology and dynamics of the coronal magnetic field, addressing coronal heating and space weather questions.
AntarctiCor: Solar Coronagraph in Antarctica for the ESCAPE Project / Fineschi, S.; Capobianco, G.; Massone, G.; Susino, R.; Zangrilli, L.; Bemporad, A.; Liberatore, A.; Landini, F.; Romoli, M.; Damé, L.; Christille, J. M.; Sandri, P.; Marmonti, M.; Galy, C.. - STAMPA. - 42:(2019), pp. 1-5. (Intervento presentato al convegno SoHe2018) [10.1393/ncc/i2019-19026-9].
AntarctiCor: Solar Coronagraph in Antarctica for the ESCAPE Project
Landini, F.;Romoli, M.;
2019
Abstract
The Antarctica solar coronagraph - AntarctiCor- for the "Extreme Solar Coronagraphy Antarctic Program Experiment" -ESCAPE- comprises an internally-occulted coronagraph based on the externally-occulted ASPIICS coronagraph for the ESA formation-flying PROBA-3 mission. This paper describes the AntarctiCor design for ground-based observations from the DomeC Antarctica plateau of the polarized broad-band (591 nm ± 5 nm) K-corona and of the narrow-band (FWHM = 0.5 nm), polarized emission of the coronal green-line at 530.3 nm. The science goal of these observations is to map the topology and dynamics of the coronal magnetic field, addressing coronal heating and space weather questions.File | Dimensione | Formato | |
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