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MORGAN, H. DRUCKMÜLLER, M.
Original Title
Multi-Scale Gaussian Normalization for Solar Image Processing
Type
journal article in Web of Science
Language
English
Original Abstract
Extreme ultra-violet images of the corona contain information over a wide range of spatial scales, and different structures such as active regions, quiet Sun, and filament channels contain information at very different brightness regimes. Processing of these images is important to reveal information, often hidden within the data, without introducing artefacts or bias. It is also important that any process be computationally efficient, particularly given the fine spatial and temporal resolution of Atmospheric Imaging Assembly on the Solar Dynamics Observatory (AIA/SDO), and consideration of future higher resolution observations. A very efficient process is described here, which is based on localised normalising of the data at many different spatial scales. The method reveals information at the finest scales whilst maintaining enough of the larger-scale information to provide context. It also intrinsically flattens noisy regions and can reveal structure in off-limb regions out to the edge of the field of view. We also applied the method successfully to a white-light coronagraph observation.
Keywords
Image processing; Corona
Authors
MORGAN, H.; DRUCKMÜLLER, M.
RIV year
2014
Released
1. 8. 2014
Publisher
Springer
ISBN
0038-0938
Periodical
Solar Physics
Year of study
289
Number
8
State
Kingdom of the Netherlands
Pages from
2945
Pages to
2955
Pages count
11
URL
https://link.springer.com/article/10.1007%2Fs11207-014-0523-9
Full text in the Digital Library
http://hdl.handle.net/11012/201728
BibTex
@article{BUT109713, author="Huw {Morgan} and Miloslav {Druckmüller}", title="Multi-Scale Gaussian Normalization for Solar Image Processing", journal="Solar Physics", year="2014", volume="289", number="8", pages="2945--2955", doi="10.1007/s11207-014-0523-9", issn="0038-0938", url="https://link.springer.com/article/10.1007%2Fs11207-014-0523-9" }