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MR/3:
MR/3: 3D and Multichannel Data
MR/3 deals with the analysis of multi-channel data or 3D
data.
3D data can either be a real cube, or a set of images of the same observation,
but taken at different times.
Multi-channel data can be either 1D or 2D multi-channel:
1D multi-channel: a 1D signal is observed at several wavelength
or at different times. The result is an image.
2D multi-channel: a 2D signal (image) is observed at several wavelengths
or at different times. The result is a cube. A special case of multi-channel
images is color images. In this case, we have three channels.
Several color coordinate systems exist.
The most widely-used is the RGB system. Each pixel is identified by
three values R, G, and B corresponding to the three colors red, green,
and blue.
Applications in MR/3 are
- General tools: statistic, operations, noise simulation, conversion ....
- Cube and Wavelet transform
- 3D a trous wavelet transform and reconstruction.
- 3D bi-orthogonal wavelet transform and reconstruction.
- 3D Wavelet transform manipulation (band extraction, ...).
- 3D data filtering using the wavelet transform.
- Multi-channel Data
- 1D and 2D Wavelet Karhunen-Loeve transform (WT-KLT) and reconstruction.
- 1D and 2D multichannel data filtering using the WT-KLT.
- Independent Component Analysis.
- Color images
- RGB image compression.
- RGB image filtering.
- RGB image contrast enhancement.
- Multi-temporal images
- Images coaddition taking into account vertical and horizontal shifts.
- Images deconvolution taking into account vertical and horizontal shifts.
To read further:
- J.L. Starck and F. Murtagh,
Astronomical Image and Data Analysis , Springer, 2002.
(ISBN 3-540-42885-2.; 300-pp. monograph).
- J.L. Starck and P. Querre,
"Multispectral Image Restoration by the Wavelet-Karhunen-Loeve Transform",
Signal Processing , 81, 12, pp 2449-2459, 2001.
- J.-L. Starck, E. Pantin and F. Murtagh,
"Deconvolution in Astronomy: a Review" , Publication of
the Astronomical Society of the Pacific, Vol. 114, pp 1051--1069, 2002.
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