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. (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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