2018
DOI: 10.1364/ao.57.009239
|View full text |Cite
|
Sign up to set email alerts
|

Suppression of stray light based on energy information mining

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
11
0

Year Published

2019
2019
2022
2022

Publication Types

Select...
6

Relationship

0
6

Authors

Journals

citations
Cited by 20 publications
(11 citation statements)
references
References 19 publications
0
11
0
Order By: Relevance
“…In this section, we compared the proposed RMGM method with three other methods, including the classic method and the excellent method in recent years, which are suitable for eliminating the stray light non-uniform background noise in surveillance image. The compared methods are Top-Hat transformation (THT) method [31], mean iterative filtering (MIF) method [32], NSTS method [33]. These methods are used to perform stray light elimination experiments in the same real captured image datasets (600 images).…”
Section: Experiments and Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…In this section, we compared the proposed RMGM method with three other methods, including the classic method and the excellent method in recent years, which are suitable for eliminating the stray light non-uniform background noise in surveillance image. The compared methods are Top-Hat transformation (THT) method [31], mean iterative filtering (MIF) method [32], NSTS method [33]. These methods are used to perform stray light elimination experiments in the same real captured image datasets (600 images).…”
Section: Experiments and Discussionmentioning
confidence: 99%
“…Therefore, they are not suitable for eliminating this non-uniform noise in the surveillance image. For spatial-domain methods, such as average filtering and gradient based thresholding [29], morphology operation [30], [31], mean iterative filtering [32], and new star target segmentation (NSTS) method [33] etc. Although these methods can better eliminate the non-uniform background noise caused by stray light in the surveillance image.…”
Section: Introductionmentioning
confidence: 99%
“…A typical star image consists of dozens of bright star spots with a dark background [ 38 ]. The signal-to-noise ratio (SNR) is generally between 20 dB and 50 dB.…”
Section: Background and Basementioning
confidence: 99%
“…Fabricating a black surface which can absorb light in broadband range from all the incident angles find huge applications in the field of photovoltaic, energy harvesting devices, optoelectronic systems, stray light attenuation, and as a calibration source for spectroscopy and infrared cameras . A lot of efforts have been made to develop a perfect broadband absorbers using metamaterials, nanotexturing, and optical grading etc .…”
Section: Introductionmentioning
confidence: 99%