Copyright (c) 2022 Clemence Prevost, Pierre Chainais, Remy Boyer
Contact: clemence.prevost@univ-lille.fr
This software reproduces the results from the following:
@unpublished{prevost:hal-03617759,
TITLE = ,
AUTHOR = {Pr{\'e}vost, Cl{\'e}mence and Chainais, Pierre and Boyer, Remy},
URL = {https://hal.archives-ouvertes.fr/hal-03617759},
NOTE = {working paper or preprint},
YEAR = {2022},
MONTH = Mar,
KEYWORDS = {hyperspectral super-resolution ; data fusion ; low-rank tensor factorizations ; recovery ; least-squares problem},
PDF = {https://hal.archives-ouvertes.fr/hal-03617759/file/icip.pdf},
HAL_ID = {hal-03617759},
HAL_VERSION = {v1},
}
In order to run the demo files, you will need to:
Please quote the corresponding paper if you decide to use these codes.
## How it works
This software reproduces the figures and tables contained in the paper. You can play with the two datasets.
### Generate coupled tensor model
Real datasets are used. First, the HSI and MSI are generated following Wald’s protocol. Then, white Gaussian noise is added to the observations.
### Run algorithms
In fusion_isabella.m
and fusion_lockwood.m
, we showcase the performance of:
The metrics and computation time are then displayed in a table. Slices of the reference and reconstructions are plotted in a figure. The color scale is generated according to the image’s spectral support.
They are available in the /demos
folder.
The table below summarized what does what
Name | Content |
---|---|
fusion_isabella.m |
Simulations for Isabella Lake dataset |
fusion_lockwood.m |
Simulations for Lockwood dataset |
choice_ranks.m |
plots R-SNR as a function of the multilinear ranks |