2012
DOI: 10.1117/1.oe.51.10.107004
|View full text |Cite
|
Sign up to set email alerts
|

Illumination invariance and shadow compensation via spectro-polarimetry technique

Abstract: A major problem for obtaining target reflectance via hyperspectral imaging systems is the presence of illumination and shadow effects. These factors are common artefacts, especially when dealing with a hyperspectral imaging system that has sensors in the visible to near infrared region. This region is known to have highly scattered and diffuse radiance which can modify the energy recorded by the imaging system. Shadow effect will lower the target reflectance values due to the small radiant energy impinging on … Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
9
0

Year Published

2013
2013
2021
2021

Publication Types

Select...
5
1

Relationship

0
6

Authors

Journals

citations
Cited by 9 publications
(9 citation statements)
references
References 15 publications
0
9
0
Order By: Relevance
“…The illumination correction method implemented in the current ATCOR-4 model (Richter & Schläpfer, 2014) combines DEMs and an empirical model to quantify relative amounts of E dif and E dir at pixel level, which are used afterwards in the atmospheric correction. Ibrahim et al (2012) use an alternative concept called spectro-polarimetry to estimate relative amounts of E dif and E dir at pixel level, but this requires at least two observations with and without a polarizer, which is not practical for airborne observations. The ToA approach, as for example proposed by Laurent et al (2011a, b), provides a flexible framework to estimate and incorporate improved descriptive data and to account for illumination effects strictly following underlying physics.…”
Section: Strategies To Account For Illumination Effectsmentioning
confidence: 99%
“…The illumination correction method implemented in the current ATCOR-4 model (Richter & Schläpfer, 2014) combines DEMs and an empirical model to quantify relative amounts of E dif and E dir at pixel level, which are used afterwards in the atmospheric correction. Ibrahim et al (2012) use an alternative concept called spectro-polarimetry to estimate relative amounts of E dif and E dir at pixel level, but this requires at least two observations with and without a polarizer, which is not practical for airborne observations. The ToA approach, as for example proposed by Laurent et al (2011a, b), provides a flexible framework to estimate and incorporate improved descriptive data and to account for illumination effects strictly following underlying physics.…”
Section: Strategies To Account For Illumination Effectsmentioning
confidence: 99%
“…The comparison between the classical Harris algorithm [Eq. (11)] and the adapted one [Eq. (12)] is illustrated in Fig.…”
Section: Adapted Harris Corner Detectormentioning
confidence: 99%
“…In the last decades, thanks to its richness in information, the polarization concept has been strongly explored to analyze, interpret, or process several types of images. [8][9][10][11] This paper aims, by using the polarization imaging, to propose a generic solution for the catadioptric images processing. The proposed method provides an efficient model to define an accurate neighborhood around each pixel within the catadioptric plane.…”
Section: Introductionmentioning
confidence: 99%
“…Normalized technique are used to solve problems generated by different spectral profiles at the same material due to shading and shadow effects [11]. The most common technique is a normalized mean-centered normalization (Mean-Norm) method [12].…”
Section: Pervious Normalized Spectral Profile Spectral Methods 32mentioning
confidence: 99%