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MORGAN, H. DRUCKMÜLLER, M.
Originální název
Multi-Scale Gaussian Normalization for Solar Image Processing
Typ
článek v časopise ve Web of Science, Jimp
Jazyk
angličtina
Originální abstrakt
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.
Klíčová slova
Image processing; Corona
Autoři
MORGAN, H.; DRUCKMÜLLER, M.
Rok RIV
2014
Vydáno
1. 8. 2014
Nakladatel
Springer
ISSN
0038-0938
Periodikum
Solar Physics
Ročník
289
Číslo
8
Stát
Nizozemsko
Strany od
2945
Strany do
2955
Strany počet
11
URL
https://link.springer.com/article/10.1007%2Fs11207-014-0523-9
Plný text v Digitální knihovně
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" }