cosmic ray neutron sensing in cropped field - ufzgabriele baroni ufz chs (leipzig, germany) 1 4th...

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4 th COSMOS workshop Leipzig (Germany) May 2014 Gabriele Baroni UFZ CHS (Leipzig, Germany) 1 4 th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped field: challenges and progress Gabriele Baroni (1) and Sascha E.Oswald (2) (1) UFZ CHS, Leipzig (Germany) (2) Inst. for Earth and Env.Sci., University of Potsdam (Germany)

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Page 1: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

1

4th COSMOS Workshop

Leipzig (Germany)

5-8 May 2014

Cosmic ray neutron sensing in cropped field:

challenges and progress

Gabriele Baroni(1) and Sascha E.Oswald(2)

(1) UFZ CHS, Leipzig (Germany)(2) Inst. for Earth and Env.Sci., University of Potsdam (Germany)

Page 2: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

2

Outline

�Motivation� Agricultural water management

�What are the challenges?� The role of biomass

�What is the progress?� Paper in prep.

Page 3: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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Uni Potsdam (Germany)

S.E.OswaldC.A.Rivera Villareyes

G.Baroni

Motivation

UFZ Leipzig (Germany)S.Zacharias and U.Wollschläger

Challenges Progress

� 2010 start

� Four Cosmic ray neutron probes

Page 4: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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Motivation

Is it possible to use the Cosmic-Ray neutron sensing for agricultural water

management? e.g. irrigation

� cropped field close to university

� Altitude 40 m a.s.l.� Relatively flat

� Area: ~ 30 ha

� sand >75%; clay <15%� Groundwater < 5 m

� 2 CRS

� 18 points FDR

Challenges Progress

Page 5: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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First results… But in a longer period…

Four months (full crop season)

Motivation Challenges Progress

Two weeks (~constant biomass)

Rivera Villareyes et al. (2011)Systematic deviation

Page 6: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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Motivation Challenges Progress

� Work conducted by Carlos

� Calibration approaches� C.R.Villareyes et al.,

2012

� Inverse modeling for effective soil parameters� C.R.Villareyes et al.,

2014 under review

� PhD Thesis� C.R.Villareyes, 2014

But in a longer period…

Four months (full crop season)

Systematic deviation

?

Page 7: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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( )pNfH p ,=

Neutron countsparametersH pool in the footprint

(30 ha 10-70 cm depth)

ChallengesMotivation Progress

Many sources of H

Page 8: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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By T.Franz

ChallengesMotivation Progress

Page 9: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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ChallengesMotivation Progress

(1) Static hydrogen pool can be intrinsic considered in the local calibration

(2) Measurements of all the H sources except the target (e.g. soil moisture)

� Two possible approaches

( )pNfHv

,=θ ( ) ∑−=k

iHpNfHv

1

In case more than one time-varying H pool?

( )( )tpNfHv

,=θ ( ) ( )tHpNfHk

iv ∑−=1

Page 10: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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The role of biomassHornbuckle et al. (2012)

( )( )tpNfHv

,=θ

ChallengesMotivation Progress

Page 11: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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(1)

(2)

� To develop an approach to correct the signal for multiple time-varying hydrogen pool (e.g., biomass)

( ) ( )tHpNfHk

iv ∑−=1

( )( )tpNfHv

,=θ

ChallengesMotivation Progress

Page 12: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

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� Correlation with height crop or LAI

ChallengesMotivation Progress

Page 13: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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� Even more complicate when we saw the results in Franz et al. (2013)

ChallengesMotivation Progress

harvesting

Page 14: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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(1)

(2)

� To develop an approach to correct the signal for multiple time-varying hydrogen pool (e.g., biomass)

� related also to below ground biomass

( ) ( )tHpNfHk

iv ∑−=1

( )( )tpNfHv

,=θ

ChallengesMotivation Progress

Page 15: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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biocCRSCRS θθθ ±=w

b

o

CRS aa

N

Na

ρρθ ⋅

−−

= 2

1

0

( ) 10⋅⋅−= zBWE CRScCRS θθ

The assumptions…

Desilet et al. (2010)

ProgressMotivation Challenges

(1) Static hydrogen pool can be intrinsic considered in the local calibration

In case more than one time-varying H pool

Page 16: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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sampling campaign θsam

snapshot in time

network θSoilNet

Installation??

biocCRSCRS θθθ ±=

samCRSc θθ = SoilNetCRSc θθ =

Can we do something more?

ProgressMotivation Challenges

Page 17: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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A scaling approach

2013 MaizeCosmic-Ray probe

FDR probes4 soil sampling campaigns

iiiCRSc cm +⋅= θθ

ProgressMotivation Challenges

Soil moisture in one position within the field

Page 18: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

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( ) 10)4(

⋅⋅−= zBWE samCRS θθ

ProgressMotivation Challenges

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Y = -0.7316x+0.1792

RMSE from 2.2% to 1.5%

ProgressMotivation Challenges

A scaling approach

iiiCRSc cm +⋅= θθ

Page 20: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

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Experimental site (Bornim)Data from 2011 in different crop conditions

ProgressMotivation Challenges

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Scaling approach in a longer term application

ProgressMotivation Challenges

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Gabriele BaroniUFZ CHS (Leipzig, Germany)

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Conclusions

� Application of Cosmic ray neutron sensing for soil moisture in cropped field� Challenges due to multiple time-varying hydrogen pools

� Scaling soil moisture� Practicable and reliable method to account for biomass

correction� Opportunity for upscale and downscale soil moisture � Attention: empirical approach!

� Paper in prep.

Page 23: Cosmic ray neutron sensing in cropped field - UFZGabriele Baroni UFZ CHS (Leipzig, Germany) 1 4th COSMOS Workshop Leipzig (Germany) 5-8 May 2014 Cosmic ray neutron sensing in cropped

4th COSMOS workshopLeipzig (Germany) May 2014

Gabriele BaroniUFZ CHS (Leipzig, Germany)

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Acknowledgment

University of Potsdam (Germany)

C.A.Rivera Villareyes, H.Esser, I.Hahn, T.Greiner, P.Bíró

UFZ Leipzig (Germany)S.Zacharias and U.Wollschläger

ATB Bornim (Germany)R.Gebbers

Thank you for the attentionQuestions and comments