Help Privacy Policy Disclaimer
  Advanced SearchBrowse




Conference Paper

Scientific processing pipeline for ASPIICS coronagraph


Inhester,  Bernd
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available

Shestov, S. V., Bourgoignie, B., Nicula, B., Dolla, L., Jean, C., Verstringe, F., et al. (2020). Scientific processing pipeline for ASPIICS coronagraph. In Proceedings of Spie, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave. doi:10.1117/12.2560164.

Cite as: https://hdl.handle.net/21.11116/0000-0008-38AA-A
Here we describe scientific processing pipeline of ASPIICS. The ASPIICS coronagraph onboard the formation ying PROBA-3 mission will deliver unprecedented observations of the solar corona starting from 1:1Rꙩ 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.