The Process of Data Formation for the Spectrometer/Telescope for Imaging X-rays (STIX) in Solar Orbiter

DOI10.1137/141001111zbMath1325.65188arXiv1412.6825OpenAlexW1486705190MaRDI QIDQ3192654

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Publication date: 13 October 2015

Published in: SIAM Journal on Imaging Sciences (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1412.6825

zbMATH Keywords

Fourier analysisspectroscopyMoiré patternhard X-ray imagingsolar flaring regionssolar orbiter clusterspectrometer/telescope for imaging X-rays

Mathematics Subject Classification ID

Numerical methods for trigonometric approximation and interpolation (65T40) Galactic and stellar dynamics (85A05)

Related Items (2)

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Uses Software

• PURIFY

Cites Work

• A Regularized Visibility-Based Approach to Astronomical Imaging Spectroscopy

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