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On the error analyses of polarization measurements of the white-light coronagraph aboard ASO-S
Feng, Li1; Li, Hui1; Inhester, Bernd2; Chen, Bo3; Ying, Bei-Li1; Lu, Lei1; Gan, Weiqun1
2019-04-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume19Issue:4Pages:10
Corresponding AuthorFeng, Li(lfeng@pmo.ac.cn)
AbstractThe Advanced Space-based Solar Observatory (ASO-S) mission aims to explore the two most spectacular eruptions on the Sun: solar flares and coronal mass ejections (CMEs), and their magnetism. For the study of CMEs, the payload Lyman-alpha Solar Telescope (LST) has been proposed. It includes a traditional white-light coronagraph and a Lyman-alpha coronagraph which opens a new window to CME observations. Polarization measurements taken by white-light coronagraphs are crucial for deriving fundamental physical parameters of CMEs. To make such measurements, there are two options for a Stokes polarimeter which have been applied by existing white-light coronagraphs for space missions. One uses a single or triple linear polarizer, the other involves both a half-wave plate and a linear polarizer. We find that the former option is subject to less uncertainty in the derived Stokes vector propagating from detector noise. The latter option involves two plates which are prone to internal reflections and may have a reduced transmission factor. Therefore, the former option is adopted as our Stokes polarimeter scheme for LST. Based on the parameters of the intended linear polarizer(s) colorPol provided by CODIXX and the half-wave plate 2-APW-L2-012C by Altechna, it is further shown that the imperfect maximum transmittance of the polarizer significantly increases the variance amplification of Stokes vector by at least about 50% when compared with the ideal case. The relative errors of Stokes vector caused by the imperfection of colorPol polarizer and the uncertainty due to the polarizer assembly in the telescope are estimated to be about 5%. Among the considered parameters, we find that the dominant error comes from the uncertainty in the maximum transmittance of the polarizer.
KeywordSun: corona Sun: coronal mass ejections (CMEs) techniques: polarimeter
DOI10.1088/1674-4527/19/4/59
WOS KeywordSOLAR
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000463893700011
PublisherNATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/24576
Collection中国科学院紫金山天文台
Corresponding AuthorFeng, Li
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Jiangsu, Peoples R China
2.Max Planck Inst Sonnensystemforsch, D-37077 Gottingen, Lower Saxony, Germany
3.Chinese Acad Sci, Changchun Inst Opt Fine Mech & Phys, Changchun 130033, Jilin, Peoples R China
Recommended Citation
GB/T 7714
Feng, Li,Li, Hui,Inhester, Bernd,et al. On the error analyses of polarization measurements of the white-light coronagraph aboard ASO-S[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2019,19(4):10.
APA Feng, Li.,Li, Hui.,Inhester, Bernd.,Chen, Bo.,Ying, Bei-Li.,...&Gan, Weiqun.(2019).On the error analyses of polarization measurements of the white-light coronagraph aboard ASO-S.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,19(4),10.
MLA Feng, Li,et al."On the error analyses of polarization measurements of the white-light coronagraph aboard ASO-S".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 19.4(2019):10.
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