Scientific processing pipeline for ASPIICS coronagraph

被引:0
|
作者
Shestov, Sergei [1 ,6 ]
Bourgoinie, Bram [1 ]
Nicula, Bogdan [1 ]
Dolla, Laurent [1 ]
Jean, Christopje [1 ]
Verstringe, Freek [1 ]
Katsiyannis, Athanassios C. [1 ]
Inhester, Bernd [2 ]
Maia, Dalmiro [3 ]
Ribeiro, Bruno [5 ]
Zhukov, Andrei [1 ,4 ]
机构
[1] Royal Observ Belgium, Solar Terr Ctr Excellence SIDC, Ave Circulaire 3, B-1180 Brussels, Belgium
[2] Max Planck Inst Solar Syst Res, Justus von Liebig Weg 3, D-37077 Gottingen, Germany
[3] Univ Porto, Fac Sci, Ctr Res Geospace Sci CICGE, P-4169007 Porto, Portugal
[4] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119991, Russia
[5] Inst Telecomunicacoes, Campus Univ Aveiro, Aveiro, Portugal
[6] Lebedev Phys Inst, Leninskii Pr T 53, Moscow 119991, Russia
关键词
ASPIICS; coronagraph; pipeline;
D O I
10.1117/12.2560164
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Here we describe scientific processing pipeline of ASPIICS. The ASPIICS coronagraph onboard the formation flying PROBA-3 mission will deliver unprecedented observations of the solar corona starting from 1:1R(circle dot) with low straylight. The Science Operations Center (SOC) of ASPIICS, to be installed at the Royal Observatory of Belgium, is responsible for delivering the raw and radiometrically calibrated data products to the science community. Among other processes, the SOC hosts the ASPIICS science data pipeline. The science processing of the ASPIICS data is required to account for the optical and detector effects correctly, convert the data into physical units, merge individual exposures into full field of view images, and calculate the polarized and spectral data products. The general architecture of the SOC is discussed and a particular attention is paid to the science data pipeline.
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页数:16
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