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Soil moisture impact on refectance of bare soils in the optical domain [0.4 – 15 μm]

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HAL Id: hal-02824027

https://hal.inrae.fr/hal-02824027

Submitted on 6 Jun 2020

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Soil moisture impact on refectance of bare soils in the optical domain [0.4 – 15 µm]

Audrey Lesaignoux, Sophie Fabre, Xavier Briottet, Albert Olioso

To cite this version:

Audrey Lesaignoux, Sophie Fabre, Xavier Briottet, Albert Olioso. Soil moisture impact on refectance of bare soils in the optical domain [0.4 – 15 µm]. 2. Workshop on Remote Sensing and Modeling of Surface Properties, Jun 2009, Toulouse, France. 16 p. �hal-02824027�

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Soil moisture impact on refectance of bare Soil moisture impact on refectance of bare

soils in the optical domain [0.4 – 15 µm]

soils in the optical domain [0.4 – 15 µm]

A. Lesaignoux1,3, S. Fabre1, X. Briottet1 and A. Olioso2

1 ONERA, Toulouse, France

2 INRA, Avignon, France

3 Université de Toulouse, France

22ndnd Workshop on Remote Sensing and Modeling of Surface Properties Workshop on Remote Sensing and Modeling of Surface Properties 9 - 11 June 2009 , Météo France, Toulouse, France9 - 11 June 2009 , Météo France, Toulouse, France

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Contents Contents

I.Context I.State of art

 Problem and approaches

 Spectral database related to soil moisture content

I.Laboratory measurements

 Description

 Method

 Analysis & Results:

 Spectra classifcation from dry samples

 Impact of soil moisture content on spectral refectance

 Empirical model

I. Conclusions and perspectives

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Context Context

Main objective

Development of a method estimating moisture of soils (bare soils and/or sparse Development of a method estimating moisture of soils (bare soils and/or sparse

vegetation) in the optical domain [0.4 – 15 µm] from hyperspectral data vegetation) in the optical domain [0.4 – 15 µm] from hyperspectral data

Applications

 Biomass estimation

 Vegetation cover health

 Traffcability: Defne link between soil characteristics (moisture, composition…) and a given vehicle with its passing number, to provide the information:

« GO » or « NO GO »

H yperspectral data [0.4 - 15 µm ]

G round spectral reflectance A tm ospheric

com pensation

Surface Soil M oisture extraction

M apping for several applications

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

State of art State of art

Problem and approaches Problem and approaches

Soil Moisture Content (SMC) Soil Moisture Content (SMC) of bare soils from spectra ? of bare soils from spectra ?

Spectra of sample’s bare soils at different moisture contents in the solar (left) and thermal domain (right) (Lab measurements)

Solar dom ain [0.4 - 2.5 µ m ]

Spe c tr a l ba nds e x plo ita tio n - A na ly tic a l m e tho ds

L iu e t a l. 2 0 0 2 L iu e t a l. 2 0 0 3 - Spe c tr a l inde x

B r y a nt e t a l. 2 0 0 3 K ha nna e t a l. 2 0 0 7 H a ubr o c k e t a l. 2 0 0 8

Spe c tr a l m o de ls - E x po ne ntia l

M ulle r 2 0 0 0 L o be ll e t a l. 2 0 0 2 - I nv e r s e g a us s ia n

« SM G M » m o de l W hiting e t a l. 2 0 0 3

G e o s ta tis tic a l m e tho ds - V N I R A m e tho d

B e n-D o r e t a l. 2 0 0 2 - G e o s ta tis tic a l a na ly s is

B r o c c a e t a l. 2 0 0 6 M e tho ds ba s e d o n s pe c tr a l

r e fle c ta nc e

T herm al dom ain [15 - 3 µ m ]

T r ia ng le m e tho d (Sa ndho lt e t a l. 2002)

I nde x (K im ur a e t

a l. 2007)

M e tho d o f the r m a l ine r tia (T r a m uto li e t a l.

2000)

[15 - 8 µ m ] e x plo ita tio n - C o r r e la tio n a na ly sis

X ia o e t a l. 2003 O g a w a e t a l. 2006 - Spe c tr a l r a tio

U r a i e t a l. 1997 M ir a e t a l. 2007 M e tho ds ba s e d o n s ur fa c e

te m pe r a tur e

M e tho d ba s e d o n s pe c tr a l e m iss iv ity

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

State of art State of art

Spectral database related to SMC Spectral database related to SMC

Approaches validation

Lab measurements of spectra of bare soils at different moisture contents Lab measurements of spectra of bare soils at different moisture contents

 Many data set in [0.4 – 2.5 µm] (Angstrom 1925, Liu et al. 2002, Lobell et al. 2002, Whiting et al. 2003, Khanna et al. 2007, Haubrock et al. 2008)

 Few data set in [8 – 15 µm] (VanBavel et al. 1976, Chen et al. 1989, Mira et al. 2007)

Synthesis

 Not enough information in the thermal domain

 No measurement covering at once solar and thermal domains

Necessity to build a database of spectral refectances of bare soils Necessity to build a database of spectral refectances of bare soils

in [0.4 – 15 µm] depending on SMC in [0.4 – 15 µm] depending on SMC

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Description Description

Samples description

 32 samples of bare soils

Collected over 8 locations in France (from South-West to South-East)

 Covering several ranges of composition and coloration

 Measurements (August 2008)

 [0.4 – 2.5 µm] : ASD FieldSpec Pro (bi-conical refectance)

 [3 – 15 µm] : Bruker Equinox 55 (directional-hemispherical refectance)

 Drying process from a lab oven

INSTRUMENT ACCURACY

ASD λ ± 1 nm

Bruker Error < 3%

Lab oven Residual moisture ~ 2 %

Different samples of bare soils

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Method (1/2) Method (1/2)

Spectral refectance measurement

Measurement of bi-conical refectance in solar domain (left) and direct-hemispherical refectance in thermal domain (right)

15°

Sample Mobile

Mirror

Detector

Integral sphere (infragold) Incident Beam

3.4 cm

Fourier Transform InfraRed spectrometer Bruker Sample

ASD Detector

3.4 cm 19.4 cm

6 cm 10°

Solar lamp

ASD spectrometer

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Method (2/2) Method (2/2)

Moisture content measurement

 Gravimetric method : Soil Moisture Content in %

Where mw : weight of the wet sample

mD : weight of the dry sample (after a 24 hours drying period at 60°C)

 Measurement protocol description

Measured spectra at several moisture contentsMeasured spectra at several moisture contents

 5 or 6 levels of SMC (%)

×100

=

W D W

m m SMC m

11. . Preparation of the measurements

tools and the samples (cleaning and saturing with

water)

2. Weighing 2.

with balance 3.

3. Brucker measurement

[3 – 15 µm]

5.

5. ASD measurement [0.4 – 2.5 µm]

7. Drying 7.

sample during 35 min at 60°C with lab oven

8. Return 8.

step 2 until the sample is

completely dry (~2%) 4. 4. Weighing

with balance

6. Weighing 6.

with balance

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Analysis & Results Analysis & Results

Measurement validation from literature

(Courault et al. 1988, Guyot et al. 1989, Liu et al. 2002, Whiting et al. 2003, Khanna et al. 2007, Haubrock et al. 2008, Salisbury et al.

1992, 1994)

Analysis

1.1. Informal soil spectra classifcation from dry samples (SMC ~ 2%)Informal soil spectra classifcation from dry samples (SMC ~ 2%) 2.2. Study of SMC impact on spectral refectanceStudy of SMC impact on spectral refectance

3.3. Empirical model of spectral refectance of bare soils related to SMC Empirical model of spectral refectance of bare soils related to SMC

 VIS: [0.4 – 0.8 µm] (VISible)

 NSWIR:[0.8 – 2.5 µm] (Near and ShortWave InfraRed)

 MWIR: [3 – 5 µm] (Medium Wavelength InfraRed)

 LWIR: [8 – 15 µm] (Long Wavelength InfraRed)

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Soil spectra classifcation (1/2) Soil spectra classifcation (1/2)

Carbonates Quartz H-C

Fe3+, Fe2+

Quartz Reststrahlen Carbonates Reststrahlen

Weak quartz Reststrahlen

Soil spectra behavior analysis from dry samples (SMC ~ 2%)

VISVIS

[0.4 – 0.8 µm]

[0.4 – 0.8 µm]

NSWIR NSWIR [0.8 – 2.5 µm]

[0.8 – 2.5 µm]

MWIRMWIR [3 – 5 µm]

[3 – 5 µm]

LWIRLWIR [8 – 15 µm]

[8 – 15 µm]

OH- H2O (OH-)

H2O (OH-)

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Soil spectra classifcation (2/2) Soil spectra classifcation (2/2)

Group 1 Group 1

Solar domain

Solar domain Thermal domainThermal domain

Example

Group 2 Group 2 Calcareous Calcareous

T3V

T1V

T1M

T1L

T2M

T3L

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Impact of SMC on spectral refectance (1/2) Impact of SMC on spectral refectance (1/2)

Solar domain: 0.4 - 2.5 µm

Spectral refectance at different moisture content in the VIS (left) and NSWIR (right) domain OH-

OH- OH-

For all samples between dry and saturated sample

VIS NSWIR

Mean of max spectra deviations 0.13±0.04 0.31±0.08 Mean of min spectra deviations 0.03±0.04 0.12±0.03

Fe3+, Fe2+

SMC

Min spectra deviation

Max spectra deviation ρ

λ Dry Saturated

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Impact of SMC on spectral refectance (2/2) Impact of SMC on spectral refectance (2/2)

Thermal domain: 3 - 15 µm

Spectral refectance at different moisture content in the MWIR (left) and LWIR (right) domain

Carbonates Quartz

SMC

Quartz Reststrahlen

Peaks detection is almost Peaks detection is almost

impossible if impossible if SMC is upper 20 % SMC is upper 20 %

For all samples between dry and saturated sample

MWIR LWIR

Mean of max spectra deviations 0.17±0.05 0.05±0.01 Mean of min spectra deviations -0.01±0.01 -0.03±0.01

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Empirical model (1/2) Empirical model (1/2)

Objective:

Determine an equation which simulate spectral refectance of bare soils at a SMC given, of which parameters are linked to SMC with empirical laws

From a soil’s composition (classifcation & chemical analysis) and a SMC we From a soil’s composition (classifcation & chemical analysis) and a SMC we could simulate spectral refectance in [0.4 – 15 µm] domain

could simulate spectral refectance in [0.4 – 15 µm] domain

Methodology in Solar domain

(Modifed Gaussian Model, Sunshine et al. 93)

LN(spectra)= Continuum(c

LN(spectra)= Continuum(c11,…,c,…,cnn)+)+ΣΣ Gaussians(g Gaussians(g11,…,g,…,gmm))

 Determine continuum with convex hull method to apply “Continuum removal” method

 Use 1st and 2nd derivative spectra (continuum removed spectrum) to determine extrema for initial parameters of Gaussians (gm ≡ centers, amplitudes, fwhm)

 Non linear Least-squares approximation of Gaussians and Least-squares approximation of Continuum (polynomial degree 4)

 Determine empirical laws link SMC with c and g (currently linear)

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

Lab measurements Lab measurements

Empirical model (2/2) Empirical model (2/2)

Preliminary results in Solar domain

 Less of absorption peaks at 1.8 µm and 2.2 µm

Difference level “seems” weak but error must be defne

Current works

 Improve algorithm to determination of Gaussian parameters

 Determine “non linear “ empirical laws between SMC and some parameters

?

?

MeasurementMeasurement ModelModel

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2nd Workshop on RSMSP, Météo France, Toulouse, 9-11 June 2009

[email protected] 16

 New database:

32 soils – 390 spectral signatures (informal spectra classifcation) Spectral refectances of bare soil related to SMC in [0.4 – 15 µm]

Spectral refectances of bare soil related to SMC in [0.4 – 15 µm]

 Impact of increase SMC on spectral refectance:

 Reduction of refectance level (mean of maximum refectance deviation < 0.3)

 Growth of depth and spreading absorption peaks at at 1.41.4 µm and µm and 1.91.9 µm µm

 Diminution of depth absorption peaks of minerals in NSWIR and MWIR

 Diminution of Reststrahlen bands of quartz and carbonates in LWIR

Empirical model:

 Improve algorithm to determination of Gaussian parameters

 Determine “non linear “ empirical laws between SMC and some parameters

 Develop algorithm for thermal domain

Perspectives:

 Use empirical model in direct simulations (processing chain)

 These lab measurements will be used to defne the inverse method to estimate

Conclusions and perspectives Conclusions and perspectives

Références

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