Soil Science Society of America Journal 66:760-773 (2002)
© 2002 Soil Science Society of America
DIVISION S-1SOIL PHYSICS
Imaging Fluorescent Dye Concentrations on Soil Surfaces
Uncertainty of Concentration Estimates
Jan Vanderborght*,a,
Paul Gähwiller
,b,
Hannes Wydlerb,
Ute Schultzeb and
Hannes Flühlerb
a Laboratory of Soil and Water, Katholieke Universiteit Leuven, Vital Decosterstraat 102, B-3000 Leuven, Belgium
b Soil Physics, Inst. of Terrestrial Ecology, Swiss Federal Institute of Technology, ETHZ, Grabenstrasse 11a, CH-8952 Schlieren, Switzerland
* Corresponding author currently at, Inst. for Chemistry and Dynamics of the Geosphere, ICG-IV Agrospere, Research Center Jülich, D-52425 Jülich, Germany; (j.vanderborght{at}fz-juelich.de)
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ABSTRACT
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To investigate transport processes in soils, detailed information about the spatial distribution of solutes is required. We describe a method to obtain concentration maps of fluorescent tracers on cross sections of soil cores with a high spatial resolution. The fluorescence signal of two dye tracers, brilliant sulfaflavine (BF; 1H-Benz(de)isoquinoline-5-sulfonic acid, 2,3-dihydro-6-amino-1,3-dioxo-2-(p-tolyl)-, monosodium salt) and sulforhodamine B (SB; xanthylium, 3,6-bis(diethylamino)-9-(2,4-disulfophenyl)-, inner salt, sodium salt), was imaged on the exposed cross sections. The fluorescence signal was corrected for variable illumination light intensity and optical properties of the soil across the exposed surface. Correction factors for varying optical soil properties were derived from the image of the reflected excitation light at the exposed surface. Linear calibration relations related the corrected fluorescence image to the total tracer concentration (Ct) map, that is, mass of dye dissolved in the soil solution and sorbed to the soil particles per unit volume bulk soil. Corrections for varying optical properties of the soil surface were important to reduce the uncertainty of the concentration that was estimated from the fluorescence signal. For BF, the calibration relations were different for different soil materials and a soil specific calibration had to be used. Variations in background fluorescence were an important source of uncertainty of the BF concentration estimates but can be overcome by applying higher concentrations. For SB, variations in calibration relations and in the background fluorescence were considerably smaller, and so is the uncertainty of the estimated SB concentrations.
Abbreviations: BF, brilliant sulfaflavine CCD, charge-coupled device SB, sulforhodamine B TDR, time domain reflectometry
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INTRODUCTION
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LEACHING OF CHEMICALS in natural undisturbed soils remains an important research topic in soil science. This research is mainly fostered by concerns about the environmental impact of chemicals applied, stored, dumped, or accidentally spilled at or near the soil surface. To investigate leaching in soils, the movement of surface applied tracers was monitored. A general conclusion that can be drawn from leaching experiments is that the transport process in soils is very heterogeneous. However, what can be learned about the leaching process from a leaching experiment depends largely on the monitoring procedure. Commonly used procedures to monitor the leaching process are in situ extraction of soil solution using suction samplers or extraction of soil samples that were taken from the field. An alternative for soil solution samplers is the time domain reflectometry (TDR) technique that infers the concentration from the in situ measured bulk soil electrical conductivity (Vanclooster et al., 1993; Ward et al., 1994). A problem with monitoring solute concentrations in soils is that concentrations may vary across small horizontal distances. In addition, leaching may occur rapidly in only a small fraction of the total pore space, referred to as preferential flow. The probability of intercepting an active flow path with a given number of samplers is often insufficient (Roth et al., 1991). Even when bulk or volume averaged properties are measured in a relatively large sampling volume, for example, of TDR probes, active flow paths that comprise only a small fraction of the total bulk soil volume may go undetected through sampling volume (Vanderborght et al., 2000).
A characterization of the structure of these preferential flow regions and the interaction between the preferential flow and bypassed regions are essential to understand and predict solute leaching (Flühler et al., 1996). However, the spatial resolution that is obtained from soil sampling may be too coarse to identify preferential flow paths accurately (Ritsema and Dekker, 1996).
Nondestructive techniques such as x-ray computer tomography (Peyton et al., 1994), magnetic resonance imaging (Cislerova et al., 1999), electric resistance tomography (Binley et al., 1996), and single photon emission computed tomography (Perret et al., 2000) are currently being developed to monitor preferential flow and transport in soil cores. Application of these techniques is still confined to relatively small soil cores since a trade-off must be made between spatial resolution and object size.
Several authors used dye tracers to visualize preferential flow paths and identify transport processes (van Ommen et al., 1989; Ghodrati and Jury, 1990; Kung, 1990; Flury et al., 1994; Petersen et al., 1997; Vervoort et al., 1999). The structure of the preferential flow paths was, in most cases, characterized from binarized images of the stained patterns using a set of different parameters, for example, relative surface of stained area, number, size, or fractal dimension of stained objects (Hatano and Booltink, 1992; Baveye et al., 1998). To calibrate and validate transport models, dye concentrations rather than dye indicators are required (Forrer et al., 1999). One technique to determine dye concentration on soil surfaces is to quantify light absorption by the dye. Light absorption is quantified by analyzing color pictures of the soil surface. This technique was applied to determine concentration distributions in homogeneous media, for example, glass beads (Schincariol et al., 1993; Richard and Robin, 2000) and silica sand (Tidwell and Glass, 1994; Aeby et al., 1997). To determine concentration distributions in natural and heterogeneous soils, spatial variations in light absorption by the soil material need to be taken into account (Ewing and Horton, 1999; Forrer et al., 2000; Stadler et al., 2000).
Alternatively, dye concentrations can be derived from the intensity of light that is emitted by fluorescent dyes after excitation. Fluorescence of a dye is observed when photons are emitted from electronically excited states following the absorption of light of shorter wavelengths. Fluorescent dyes have been used to stain preferential flow paths in soils (Omoti and Wild, 1979; Jørgensen et al., 1998) and to monitor solute transport during breakthrough experiments (Trudgill, 1987). Recently, an in situ technique using fiber optic mini probes has been developed to monitor fluorescent dye concentrations with high temporal resolution in soils (Campbell et al., 1999; Garrido et al., 1999; Ghodrati, 1999). Using fluorescent dyes with different excitation spectra (fluorescence intensity as a function of the wavelength of the excitation light) and different emission spectra (intensity of the emitted light as a function of the wavelength) the fluorescence signal of the different dyes can be separated by filtering the excitation and emission light. This implies that different dyes can be determined independently and multitracing experiments can be carried out. Besides marking preferential flow paths, the fluorescence signal on soil surfaces can be quantitatively interpreted. In the field of environmental analysis, laser-induced fluorescence is used to determine contaminant concentrations in situ by measuring the emitted fluorescence on a soil surface (Löhmannsröben and Roch, 2000). The quantitative interpretation of the fluorescence signal from dyes on a soil surface is similar to the interpretation of fluorescence from contaminants (Löhmannsröben and Schober, 1999).
In this paper, we discuss a procedure that was introduced by Aeby et al. (2001) to derive tracer concentrations maps from a fluorescence image of an exposed soil surface. This procedure corrects variations in the fluorescence signal that are not caused by variations in dye concentration. We evaluate the effects or importance of different correction steps and discuss the uncertainty on the estimated concentrations. Finally, we propose some changes to the procedure of Aeby et al. (2001) that reduce the uncertainty of the estimated concentrations. Fluorescent tracers were applied to undisturbed soil cores during a leaching experiment. This leaching experiment was carried out to investigate transport of fluorescent tracers in undisturbed soil. Breakthrough data, fluorescent tracer distributions on horizontal surfaces at several depths in the soil cores, and the relation between soil structure and solute leaching are discussed in an accompanying paper (Vanderborght et al., 2002).
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EXPERIMENTAL SETUP
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Tracer Application
During a leaching experiment, dye tracers were applied to undisturbed soil cores (107-mm i.d., 110-mm length) that were taken at three different depths in a loamy Stagni-Humic Cambisol under forest (Unterehrendingen, Switzerland). Physical and chemical properties of this soil and of a loamy Eutric Regosol (Bekkevoort, Belgium) are listed in Table 1. Calibration relationships were also determined for the Bekkevoort soil (see below). The soil cores were taken by pushing stainless steel cylinders gently into the soil. In the lab, the samples were pushed out of the steel cylinders and cast with a resin (Araldite CW 2418-1 and hardener HR 5162, Novartis, Switzerland). The samples were saturated with water, put on fritted glass plates in sample holders and placed in a small Plexiglas container with four horizontally installed nozzles that created a mist of fine water droplets (Kasteel, 1997). By turning the nozzles periodically on and off, a quasi steady state water flux was established at the surface of the soil cores. The flow rate that was generated in the Plexiglas container ranged from 33 to 51 mm d-1 depending on the location in the container. Once a steady flow rate was achieved in the soil cores, 1 mL of a tracer cocktail [2 g L-1 BF (Sigma Chemical Co., St. Louis, MO), 0.2 g L-1 SB (FLUKA Chemie AG, Buchs, Switzerland) and 10 g L-1 CaCl2·2H2O] was applied every 30 min to approximate a step input of tracer solution with concentration C0. C0 was calculated from the amount and concentration of the applied tracer cocktail and the flux of solute free water at the soil surface. The salt CaCl2·2H2O was added to investigate the effect of sorption to soil particles on dye leaching by comparing dye leaching with leaching of Cl- that is not retarded by sorption (Vanderborght et al., 2002). Depending on the location of the soil core in the container, the following C0 were applied: 0.2 to 0.32 g L-1 BF, 0.02 to 0.032 g L-1 SB, and 1 to 1.6 g L-1 CaCl2·2H2O.
The chemical properties of the two fluorescent dyes, BF and SB, are listed in Table 2. In this paper, dye concentrations are expressed as mass formulated dye powder per volume. The high fluorescence of the two dyes, which is pH independent in the range of pH 3 to 9 (Aeby et al., 2001; Smart and Laidlaw, 1977), makes the dyes suitable for transport studies in soils. Since the excitation and emission spectra are well separated, the excitation and emission light of the dyes can be filtered so that the fluorescence signal of only one dye can be measured without interference by the other dye. The infiltration of the tracer solution was stopped 72 h after the start of the tracer application in a first set of cores and 96 h after the start of the tracer application in the second set. After stopping the infiltration, the cores were drained by gravity and horizontally sliced at 100 mm, 95 mm, and then down to 15 mm by 10-mm increments above the bottom surface of the cores. From each horizontal slice five pictures (see below) were taken to determine the concentration patterns of the two dyes. To minimize tracer accumulation at the soil surface due to evaporation, images were taken immediately after slicing. We tested the role of evaporation in the context of measuring dye tracer concentrations on field soil profiles (Forrer et al., 2000) and observed that during a period of 5 to 9 d the evaporative accumulation of the dye tracer in the evaporating surface layer was minor.
Image Acquisition
Figure 1
outlines the different components of the equipment. The light generated by a 1-kW xenon light source (KiloArc, Photon Technology Int., South Brunswick, NJ) is guided to a liquid light guide and selectively filtered for the appropriate excitation spectrum of each dye by a set of filters, dichroic mirrors, and lenses. The window of high optical transmission ranges from 400 to 445 nm for the BF excitation filter set and from 535 to 545 nm for the SB excitation filter set. The excitation filter set must be exchanged when measuring another dye. Detailed information about the characteristics of the optical components and the ranges of high optical transmission of the filter combinations is given by Aeby (1998) and Aeby et al. (2001). The light guide (series 380, Lumatech, Munich, Germany) brings the light into a darkened room where the soil cores were positioned on a vertically adjustable table under the camera. The end of the light guide was placed next to the camera to avoid large shadows on the picture. For every horizontal slice, the height of the table was adjusted so that the upper surface of the soil cores remained in focus (focus distance was 0.785 m). Because of the relatively weak fluorescence of the dyes on the soil surfaces and corresponding long exposure times, the sensitivity of the camera must be large, whereas the noise should remain as small as possible. Hence, a slow-scan cooled charge-coupled device (CCD) camera (Antares TE4 EEV CCD05-30 MPP, AstroCam Ltd., Cambridge, UK) with a high-speed normal lens (Noct-Nikkor 58 mm f/1.2, Nikkon Corp., Japan), a 1248- by 1152-pixel image size, and a 16-bit digitization was used. For a focus distance of 0.785 m, the spatial resolution was 0.233 mm. The CCD chip was cooled to -30°C to minimize thermal noise. The accumulated signal for each pixel was sent pixel by pixel to the controller (slow-scan) to reduce readout noise. The camera is controlled and the images are captured from the controller and stored by the PixCel software (AstroCam Ltd, Cambridge, UK).
From each horizontal cross section, five pictures were taken: two fluorescence images, A(x), one for each dye (exposure time: 90 and 180 s for BF and SB, respectively), two reflection images, R(x), (exposure time: 1 s and 600 ms for BF and SB, respectively), and one image of a flat cardboard that was placed on top of the soil cores, F(x). The fluorescence images were taken with the dye-specific emission light filter in front of the camera, which transmits the emitted light by the fluorescent dye but filters the excitation light that is reflected at the soil surface. The window of high optical transmission ranges from 470 to 560 nm for the BF emission filter set and from 575 to 635 nm for the SB emission filter. The reflection images were taken without emission filter and record the reflection of the excitation light at the soil surface. To determine the bias to the measured signal, images were taken with the protection cap on the camera lens (dark images) using the same exposure times. The average value of the dark image was subtracted and A(x), R(x), and F(x) refer from here forward to images of which the bias was removed.
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METHODS
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For a dye solution, the fluorescence intensity, If, is a function of the intensity of incident light, I0, and the concentration C:
 | [1] |
where
f is the fluorescence efficiency,
is the light absorption efficiency of the dye according to the Beer Lambert law, and d is the thickness of the absorbing layer. For 2.303
Cd < 0.05, Eq. [1] can be linearized:
 | [2] |
For fluorescence measurements on soil surfaces, the product Cd can be interpreted as the dye mass that is illuminated per unit area. Due to scattering and absorption of incident light at the soil surface, the excitation light intensity at the soil surface, I0, is different from the intensity of incident light. Even for a uniform intensity of incident light, the excitation light intensity may vary over the soil surface due to variations in soil properties over the soil surface. The procedure that we use to derive dye concentration maps from fluorescence measurements on soil surfaces consists of three steps. Figure 2
gives an overview of the different steps: correction for variable incident light intensity (Step I), correction for variations in soil surface properties that influence the local excitation light intensity and that are linked to variations in light reflection at the soil surface (Step II), and application of calibration relations (Step III).

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Fig. 2. Outline of the image processing steps to derive dye concentrations from the fluorescence image. Left-hand side panels are images of the fluorescence signal of brilliant sulfaflavine (BF) on horizontal cross sections of four soil cores from the Unterehrendingen soil (upper and lower cores in the panel are taken from the topsoil and subsoil, respectively): A(x) is the raw fluorescence signal; Aff(x) is the flat field corrected fluorescence signal; Affr(x) is the background subtracted fluorescence signal corrected for variations in soil surface reflection; and Ct(x) is the total concentration pattern. Right-hand side panels represent correction factors <F(x)>/F(x) for inhomogeneous illumination (flat field correction); correction factors R0/Rff(x) for variations in excitation light reflection at the soil surface; and calibration relations between corrected fluorescence and total dye concentration, Ct.
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Corrections for Inhomogeneous Illumination (Step I)
Since the point-like light source was relatively close to the surface, the light intensity was higher in the center of the image. The fluorescence image matrix, A(x), is corrected for this variation in illumination using the flat field image, F(x):
 | [3] |
where Aff(x) is the flat field corrected fluorescence image and <F(x)> is the mean value of the flat field.
Corrections for Spatial Variations of Soil Surface Properties (Step II)
The fluorescence signal that is recorded by the camera depends, in addition to the concentration of the fluorescent dye at the soil surface, on soil surface properties that influence the local excitation light intensity. Two different causes for spatial variability of the excitation light intensity over the soil surface can be distinguished. First, geometrical irregularities of the soil surface at different scales, that is, surface roughness due to irregular particle shapes, irregular arrangement of particles, and depressions at a larger scale, lead to differences in local excitation light incidence. Rougher soil surfaces contain more shadowed regions where the local excitation light intensity is lower than the intensity of the incident light. Second, variations in the chemical and physical composition of the soil surface (mineralogy, organic carbon content, and water content) lead to differences in local light absorption and, hence, differences in local excitation and emission light intensities. Variations in soil surface roughness are seen as gradations of darkness, whereas variations in chemical and physical composition of the soil surface are seen as gradations of soil color.
Assuming a chemically and physically homogeneous soil surface, the effect of spatial variability of soil surface roughness on the fluorescence signal can be corrected as:
 | [4] |
where A
ffr(x) is the fluorescence image corrected for variations in soil roughness, R0 is a reference reflection, and Rff(x) [= R(x) <F(x)>/F(x)] is the flat-field corrected reflection image (the index (1) discriminates the different correction procedures for variations in optical properties of the soil surface). This correction term follows directly from the linear relations between the local excitation light intensity, the fluorescence signal, and the reflection signal, Rff(x).
Assuming a constant surface roughness, correction factors for variations in chemical and physical composition of the soil surface can also be derived from the reflection image, Rff(x). Assuming that most of the excited dye molecules are at or close to the surface and directly exposed to incident light, the excitation light intensity is the sum of direct excitation light incidence and the diffuse reflected excitation light at the soil surface (Aeby et al., 2001). In the same vein, the emitted light intensity is the sum of the directly emitted light and the reflected emitted light at the exposed soil surface. This assumption leads to the following correction for spatial variations in light absorption that result from variations in chemical and physical composition of the soil surface:
 | [5] |
where fex0 and fem0 are the reference diffuse reflectance at the excitation and emission wave lengths, respectively, and fex(x) and fem(x) are the diffuse reflectance of the exposed soil surface at location x, which depend on the chemical and physical composition of the soil surface at this location. Because of the random orientation of soil particles, the light reflection from a macroscopically flat surface is diffuse, that is, the light is reflected in all directions with the same intensity. The diffuse reflectance is the ratio of the intensity of the reflected light from a macroscopically flat surface to the intensity of the incident light. It is measured using diffuse reflectance spectroscopy by comparing the light reflection from a soil sample with the reflection from a white reference standard (BaSO4), which is placed at exactly the same position with respect to the light source and detector as the soil sample and which reflects >98% of the incident light at every wavelength of the visible spectrum. The diffuse reflectance is closely related to the light reflection that is measured using the image acquisition setup. At a certain point it can be derived from the reflection image as:
 | [6a] |
and
 | [6b] |
where R0 is the reflection of a reference surface with diffuse reflectance fex0 and fem0.
There are two problems related to the application of this correction. First, the correction factor for variations in surface roughness is different from the correction factor for variations in chemical and physical composition of the surface. But, the reflection image, Rff(x), reflects variations in surface roughness as well as variations in chemical and physical composition of the surface. Since the roughness and chemical and physical composition vary independently across the soil surface, it is impossible to distinguish them based on the reflection image, Rff(x). Therefore, Aeby et al. (2001) suggested using an averaged correction term, which they defined as the arithmetic average of Eq. [4] and [5]. Second, for rough soil surfaces, it might be questioned whether most of the dye molecules are directly exposed to the incident light. As an alternative working hypothesis, we postulate that most dye molecules are excited by scattered or diffuse reflected light from randomly oriented microscopic surfaces. The intensity of this local scattered light depends on the local light absorption by the soil minerals and the roughness of the surface. It is proportional to the local intensity of the reflected light that is recorded by the camera in the reflection image. If it is assumed that dye molecules are excited by the scattered light rather than by direct incident light, then the intensity of the scattered excitation light and the fluorescence signal are proportional. In the same vein, the local fluorescence light and the local diffuse reflected excitation light that are recorded by the camera are proportional. As a consequence, variations in both soil surface roughness and chemical and physical composition of the surface could be linked to variations in local light reflection and corrected for by the following correction:
 | [7] |
Notice that this equation is identical to the correction for variations in soil roughness assuming a chemically and physically homogeneous soil surface (Eq. [4]). Löhmannsröben and Schober (1999) used and experimentally verified an identical correction of laser-induced fluorescence of diesel in soils with differing light absorption and reflection. Since the light absorption by a certain compound depends on the wavelength, reflection images, Rff(x), have to determined at the excitation light frequency.
It is evident that also fluorescent dye molecules absorb excitation light and influence the reflection image. However, correction factors were determined assuming that variations in the reflection image result only from variations in soil surface properties. Therefore, the correction factors can only be used when light absorption by fluorescent dye molecules is negligible compared with the light absorption by the soil surface. In addition to dye molecules, other chemical substances at the soil surface, such as organic matter, may emit a background fluorescence signal. This background fluorescence signal, Abg, may be negatively correlated, due to low fluorescence efficiency, to the reflection image. For a constant background or a background signal that is negatively correlated to the reflection image, Eq. [7] generates a noise on the corrected image. The background fluorescence is derived from the average fluorescence signal in selected regions on the surfaces in which apparently no dye was present. The standard deviation of the background fluorescence within the nonstained regions,
Abg, defines the minimal dye fluorescence that can be discriminated from the background signal. Twice the standard deviation of the fluorescence signal in nonstained regions can be interpreted as a detection limit of the dye fluorescence. Background subtracted fluorescence signals (Aff(x) - Abg) that are larger than 2
Abg or detection limit, come with a probability >95% from dye molecules. To avoid the introduction of noise, an average value of the background signal is subtracted from the original fluorescence signal and all values of the background subtracted fluorescence [Aff(x) - Abg] that are smaller than 2
Abg are set equal to zero before the fluorescence image is multiplied by the correction factor:
 | [8a] |
 | [8b] |
It should be noticed that for the calculation of A
ffr(x) or A
ffr(x), a flat field image F(x) is not required since replacing Aff(x) and Rff(x) in Eq. [4] and [7] by A(x) and R(x), respectively, would lead to exactly the same results. However, a flat field image is required to determine the background signal Abg and its standard deviation
Abg and calculate A
ffr(x) and A
ffr(x).
Calibration Procedure (Step III)
The corrected and background subtracted fluorescence signal, Affr(x), is related to the concentration pattern using a calibration relation. For relatively low concentrations, a linear relation can be assumed (Eq. [2]). The definition of the concentration units depends on how the concentrations are determined or preset in the calibration experiment. The calibration relation can be determined in different ways. In a first procedure, soil material could be sampled and the tracer extracted to determine the local concentration at number of points on a soil surface of which the fluorescence signal was recorded. Using the extraction procedure, the concentration is most naturally defined in terms of the extracted tracer mass per mass of dry soil material. However, two problems arise with this extraction calibration procedure. First, the fluorescence signal is defined by the number of dye molecules per surface area. Thus, the local soil bulk density must be known to link the fluorescence signal to the mass of dye per mass of dry soil. Second, the fluorescence signal depends on the concentration at the soil surface whereas the concentration in the soil extract represents the average concentration in the sampled soil volume. Since local concentrations vary a lot with a short distance, this may lead to a discrepancy between the concentration in the extract of the sampled soil volume and the concentration at the soil surface. Therefore, we used an alternative procedure and prepared a soil paste mixing preset amounts of dry soil and tracer solution with known concentration. A sample container with known volume was filled with the soil paste and weighted so that the total dye concentration, Ct, that is, dye mass per volume bulk soil, in the soil samples could be calculated. The total concentration Ct comprises the mass of dye dissolved in the soil solution and sorbed to soil particles. It should be noted that a unique calibration relation between fluorescence signal and total dye concentration for soil materials with different dye adsorption isotherms (for the same total dye concentration a different fraction of dye mass is adsorbed to soil particles) implies that fluorescence of dye molecules is not influenced by adsorption to soil particles. A calibration relation was established between Ct in the prepared soil samples and the fluorescence signal from these samples. To prepare the samples, we took nonstained soil material from the 0- to 0.1-m and from the 0.5- to 0.6-m soil layers of the Unterehrendingen soil. In addition, we also used nonstained soil material from the 0- to 0.1-m and the 0.5- to 0.6-m soil layers of the Bekkevoort soil (Eutric Regosol) in order to evaluate the variability of the calibration relationships between different soil materials. The properties of the different soil layers of the Unterehrendingen and Bekkevoort soils are listed in Table 1. The soil material was dried for 24 h at 70°C, ground, and sieved with a 0.5-mm sieve. For the Unterehrendingen soil, we mixed 12 g of the dried and sieved soil with 3.6 mL dye solution. For the Bekkevoort soil, a mixture of 12 g soil and 3.6 mL dye solution was too liquefied and therefore we mixed 12 g soil with only 2.4 mL dye solution for this soil. Dye solutions of 10, 20, 40 (50 for the 0.5- to 0.6-m layer in Unterehrendingen), 100, and 200 mg L-1 SB and 50, 100, 200, 500, 1000, 2000 (Unterehrendingen), and 5000 (Unterehrendingen, 0.5- to 0.6-m soil layer) mg L-1 BF were used to create a calibration series of soil pastes. Small Polystyrole-cylinders of 6.49-mL volume were filled with soil paste and sealed to prevent evaporation that would alter the dye distribution within the sample and the optical properties of the soil surface. Water flow within the sample towards the soil surface accumulates dyes at the soil surface and dry surfaces are brighter than wet ones (Gimmi et al., 1999). The resulting volumetric water content,
, in the samples with the Unterehrendingen and Bekkevoort soil, was, respectively, 0.44 and 0.34. The total dye concentrations, Ct, in the calibration samples ranged for SB from
3 to 70 mg L-1 bulk soil (Bekkevoort) and from
4 to 90 mg L-1 bulk soil (Unterehrendingen), and for BF from
15 to 350 mg L-1 bulk soil (Bekkevoort) and from
20 to 2000 mg L-1 bulk soil (Unterehrendingen). Exact Ct were calculated for each calibration sample knowing the weight and volume of the sample, the ratio of dye solution and dry soil of the soil paste, and the dye concentration in the dye solution.
The fluorescence and reflection images of the calibration samples were recorded under the same illumination conditions as the horizontal cross sections of the Unterehrendingen soil cores and corrected for variations in illumination light intensity (Eq. [3]). Averages of the fluorescence and reflection across the surface of a calibration sample were used in the correction equations for variations in optical properties between samples from different soil layers (Eq. [4][7]) and in the calibration relations. The reference reflection, R0, is defined as the average reflection of the samples from the four different soil layers. However, since the spectrum of the excitation light is relatively wide, and since the diffuse reflectance of the soil cannot be measured at the emission wavelength using the image acquisition setup, the diffuse reflectances of a certain soil material at the excitation and emission wave lengths, fex and fem, were measured using diffuse reflectance spectroscopy. The reference diffuse reflectances, fex0 and fem0, were defined as the average reflectances of the different soil materials, consistent with the definition of R0. Differences in optical properties of the surfaces of calibration samples and soil cores lead to a different light reflection and fluorescence signal for the same total concentration Ct. Equation [5] or Eq. [7] corrects these differences so that, in principle, the factors that determine the optical properties (water content, surface roughness, and soil material) need not to be identical in the calibration samples and soil cores.
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RESULTS AND DISCUSSION
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In this section we discuss the importance of different steps in the image analysis procedure (Fig. 2) to derive concentration patterns from a fluorescence image and the uncertainty of the derived concentration pattern. The importance of a certain step is evaluated in terms of the changes that it makes to the original image. Although the derivation of concentrations from the fluorescence signal using calibration relations is the last step in the procedure, we start with discussing this step, since it was decided based on the calibration experiments which correction factor was used to correct for variations in soil surface properties.
Calibration Relations
In Fig. 3
, the fluorescence of the calibration samples is plotted vs. the total dye concentration in the samples, Ct. Calibration relationships are shown for fluorescence signals that are, Affr, and that are not, Aff, corrected for differences in light reflection between soil samples with different soil material. Either Eq. [5]
or Eq. [7]
were used to correct for differences in light reflection. In order to facilitate the interpretation of the double logarithmic plots, the background fluorescence signal (fluorescence signal for Ct = 0 mg L-1), which was determined for each soil material and correction procedure, was subtracted. The relative reflection coefficient, Rff/R0 and the diffuse reflectance, fex and fem, of the soil material in the calibration samples at the excitation and emission wavelengths are listed in Table 3, together with the correction factors derived from Eq. [5] and [7]. Notice in Table 3 that the correction factors derived from Eq. [5] are close to 1, whereas Eq. [7] leads to larger corrections of the fluorescence signal. Except for BF in the Unterehrendingen soil, the darker color of the top soil layer due to its higher organic carbon content is reflected in larger correction factors. The correction factors are also larger for the Bekkevoort soil that appears to be darker than the Unterehrendingen soil.
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Table 3. Soil diffuse reflectances at the excitation, fex, and emission, fem, light wavelength and fluorescence signal correction factors calculated from Eq. [5] and Eq. [7] using the relative reflection of the excitation light at the soil surface measured by the image acquisition setup, R0/Rff, for different soil layers.
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Since the slopes of the calibration plots in Fig. 3, in which both coordinate axes are logarithmically scaled, are close to 1, it can be concluded that the relation between fluorescence signal and total concentration is nearly linear in the considered concentration ranges (202000 mg L-1 BF and 390 mg L-1 SB). For the lower end of the concentration ranges, the variability of the fluorescence signal is quite large, which suggests that the lowest concentrations are close to the detection limit of the method. For the Unterehrendingen subsoil (0.5- to 0.6-m layer), samples with concentrations <100 mg L-1 cannot be separated on the basis of the fluorescence signal so that the detection limit of BF in this layer is
100 mg L-1. The y-intercepts of the calibration relations in the double log10 plots correspond to the slope of the calibration relation in a linear plot. The slopes, a, of the linear calibration relations, Ct = aA
ffr or Ct = aAff(x), were estimated from the y-intercept of a linear regression between the loge transformed concentration and fluorescence whereby the slope was fixed and put equal to 1:
 | [9] |
where n is the number of calibration points. The obtained slopes for the different soil materials and different fluorescence corrections are listed in Table 4. For BF, the slopes of the calibration relations are quite different for the different soil types and correcting the fluorescence for differences in light reflection resulted in an even larger spreading of the slopes. Therefore, differences in the fluorescence cannot be explained by differences in local excitation light intensities due to differences in optical properties of the soil surfaces. The different calibration relationships between fluorescence signal and total BF concentration for the two layers from the Unterehrendingen soil can neither be explained by assuming that only dissolved BF molecules contribute to the fluorescence signal. For the same total BF concentration, the fluorescence signal is a factor 3.3 higher in the 0- to 0.1-m layer than in the 0.5- to 0.6-m layer, whereas the concentration in the liquid phase is only a factor 1.3 higher. This factor was calculated from the water content, bulk density of the calibration samples, and the linear distribution coefficient, Kd, between liquid and solid phase concentrations (see Fig. 1 in Vanderborght et al., 2002). This suggests that the chemical composition of the soil solution and the sorption mechanisms of BF to soil particles, which may differ for different soil materials, influence the fluorescence of BF on soil surfaces. The large differences in the calibration relations between the different soil materials imply that a soil-specific calibration is required to derive the absolute concentrations from the fluorescence signal. In a given soil material, relative concentration distributions can be inferred directly from the fluorescence signal. However, to interpret the fluorescence signal of BF on a vertical soil surface with different soil layers and corresponding different calibration relations, a soil type or depth dependent calibration relation must be used.
For SB, the variability of the calibration slopes is smaller and is reduced by correcting the fluorescence signal for variations in light reflection at the soil surfaces. Especially for the Unterehrendingen soil, the differences in the calibration relations are nearly completely corrected by Eq. [7]. For the Unterehrendingen soil, large differences in SB adsorption to soil from the 0- to 0.1-m and from the 0.5- to 0.6-m layer was observed in batch adsorption experiments with considerably more dye adsorption in the 0.5- to 0.6-m layer (Vanderborght et al., 2002). The similar calibration relations for the two soil layers between fluorescence signal and total dye concentration (sorbed and dissolved dye mass) suggest that SB fluorescence is relatively independent of dye sorption to soil particles.
The differences in light reflection between the calibration samples were mainly due to differences in chemical and physical composition of the soil surfaces since nearly flat surfaces were obtained by pushing the soil paste to the Polystyrene container surface. However, unlike Eq. [5], Eq. [7] also corrects for variations in surface roughness. Therefore, we use Eq. [7] from this point forward to correct Aff(x) for variations in light absorption and roughness of the soil surface.
Correction for Variations in Soil Surface Properties
In Fig. 4
, a noncorrected fluorescence image, Aff(x), and three differently corrected images for variations in light reflection at the soil surface, A
ffr(x), A
ffr(x), and 
ffr(x), are shown. 
ffr(x) is calculated using Eq. [8] but on the basis of the median filtered (9- by 9-pixel median filter) fluorescence and reflection images. Not subtracting the background before the correction led to a considerable introduction of noise A
ffr(x), Fig. 4b] that nearly completely blurred the signal in the original fluorescence image. In Fig. 5
, the background fluorescence, detection limit (which was defined as twice the standard deviation of the background fluorescence in nonstained regions), and the typical signal of the dye fluorescence are graphically presented. The typical signal merely represents a typical background subtracted fluorescence signal in stained regions on the soil surfaces. The total dye concentrations, Ct, that correspond with this background, detection, and typical dye signal and that are derived using the calibration relations are listed in Table 5. For BF, the background is as large as the dye signal and the detection limit is
20 and 30% of the typical dye signal for the 0- to 0.1-m and 0.5- to 0.6-m layer, respectively. To increase the signal to detection limit ratio, higher BF concentrations should be applied. For SB, the background is smaller compared with the typical dye signal and the detection limit is
5% of the typical dye signal. It should also be noted that the variability of the background fluorescence in nonstained regions of the soil core surfaces and the calibration plots (Fig. 3) point at similar absolute values of the detection limit.

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Fig. 5. Illustration of the background fluorescence signal, detection limit, and typical dye fluorescence signal.
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Table 5. Dye concentrations corresponding to the background fluorescence signal, the detection limit, and the typical dye fluorescence signal.
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The corrected image A
ffr(x) (Fig. 4c) contains dark features that alternate with strongly illuminated regions and give the impression of shadows on an illuminated rough surface. These shadowlike features point at an artifact that results from small shifts of the reflection against the fluorescence images. When the two figures are slightly shifted, shadows in the reflection image, which correspond to large correction factors, are shifted to regions in the fluorescence image with a high signal, and the fluorescence signal is amplified dramatically. Small shifts of the two images were unavoidable since the camera could not be fixed completely when the emission light filter was screwed on the camera. To evaluate the uncertainty due to small shifts of the images, the reflection image was shifted from 3 to +3 pixels along both coordinate axes. For each shift, 49 in total, the corrected fluorescence was computed and a set of corrected fluorescence values was obtained for each pixel. The coefficient of variation of this set of corrected fluorescences amounted 20% and is a measure of the uncertainty or the noise that results from small image shifts. This noise was considerably reduced in 
ffr(x) (Fig. 4d) by applying a 9- by 9-pixel median filter to the reflection and fluorescence image before the correction. The noise reduction by the median filter is at the expense of the image resolution. Since the image has a pixel size of 0.233 by 0.233 mm, the resolution of the median filtered image is 2.1 by 2.1 mm.
In Fig. 6
, the range of correction factors that is used to correct the fluorescence image for variations in soil surface roughness and light absorption are shown for the different soil layers and the two dyes. The range is represented by the minimum and maximum correction factors and an interval around the mean correction factor. This interval is defined as:
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where
is the standard deviation of the loge transformed correction factors, and R0/Rmean is the average correction factor for a soil surface. For lognormally distributed variables, this interval represents the range in which 90% of the correction factors are found. In general, this interval ranges from 0.65 to 1.5 R0/Rmean.

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Fig. 6. Range of correction factors for variations in excitation light reflection at the surface of soil cores from the 0- to 0.1-m, 0.2- to 0.3-m, and the 0.5- to 0.6-m layer of the Unterehrendingen soil for the excitation light wavelengths of brilliant sulfaflavine (BF) and sulforhodamine B (SB). Horizontal bars mark the interval that is defined in Eq. [10] and that contains 90% of the correction factors.
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Dye Mass Recoveries
Table 6 lists mass recoveries of the dyes in the soil cores. The mass recovery was calculated from the average total dye concentration on the horizontal cross sections and is expressed as a percentage of the expected mass in the soil cores (i.e., the difference between the infiltrated and leached dye mass from the soil cores). The mass between the top (100 mm above the bottom of the soil core) and the bottom (15 mm above the bottom of the core) cross sections was calculated using the trapezoidal rule. The masses in the top (between 110 and 100 mm) and bottom slices (between 15 and 0 mm) were calculated by extrapolating the average concentration from the top and bottom sections, respectively. For some soil cores, the image of the 100-mm section was missing and the mass in the top slice was calculated by extrapolating the concentration from the 95-mm section. For SB, the mass recovery in soil cores taken from the topsoil (0- to 0.3-m layer) is fairly close to 100%, whereas only half of the expected mass is found back in the cores from the subsoil (0.5- to 0.6-m layer). The mass recoveries of BF deviate more from 100% than those of SB, which might be explained by the larger uncertainty of the BF concentration estimates. However, deviations between the calculated and expected mass recoveries also result from the extrapolation of concentrations in the top slice of the soil cores. In the subsoil layer, preferential flow through the cores occurred. The tracer solution was funneled into preferential flow paths within the top slice of the soil core so that only a fraction of the total cross section was stained in the 100-mm slice (see Fig. 7 and 8 in Vanderborght et al., 2002). Therefore, the dye mass is likely to be underestimated in the top slice of the soil core so that the low mass recoveries are the result of an incomplete description of the concentration profile near the input surface.
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Table 6. Mass recoveries (percentage of expected dye mass in the soil cores). Mass recoveries of cores missing the 100-mm section are given between parentheses.
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SUMMARY AND CONCLUSIONS
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In order to interpret the fluorescence signal of dyes on a soil surface in terms of dye concentrations, we need (i) corrections for variations in soil surface properties that influence the local excitation light intensity and (ii) a calibration relation. Figure 7
summarizes the effect of this correction and calibration on the interpretation of the original fluorescence. The range of factors, normalized to one, with which the original fluorescence signal is multiplied to obtain a concentration estimate, is shown. This range can also be interpreted as an uncertainty range around the concentration estimates when the fluorescence signal is not corrected for variations in soil surface properties and when no soil specific calibration relation is used to link the corrected fluorescence signal to the dye concentration. It is compared with the uncertainty of the estimated concentrations due to pixelwise shifts of the reflection image against the fluorescence image and the detection limit that results from fluctuations in the background fluorescence signal. For BF, a soil specific calibration is very important for the interpretation of the fluorescence signal, which is apparently influenced by other soil properties than those that influence the local excitation light intensity at the soil surface. At this moment, we do not know the reason for the variations of the calibration relation. A more extensive study on the calibration relationships in a larger set of different soils is required. It is not unlikely that the underlying causes for this calibration variability vary across a soil surface. Therefore, the difference in calibration relations for different soil materials brings about an uncertainty of the concentration estimates. Also, the detection limit of BF was relatively high compared with the typical fluorescence signal of the dye in the stained regions. For SB, the calibration relation is less soil type dependent and the detection limit compared with the typical dye signal is smaller than for BF. Therefore, the uncertainty of concentration estimates of SB is considerably smaller than that of BF. Corrections for variations in soil surface properties that influence the local excitation light intensity are important. An important advantage of fluorescent dyes compared with nonfluorescent dyes is that the optical soil properties that influence the local light intensity can be observed without or with minimal interference by the presence of the dyes. Since detection of a nonfluorescent dye is based on the change of optical surface properties by the presence of the dye, this correction is not possible for nonfluorescent dyes.

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Fig. 7. Summary of uncertainty factors of the estimated brilliant sulfaflavine (BF) and sulforhodamine B (SB) concentrations and of correction factors normalized to one with which the flat field corrected fluorescence signal, Aff(x), is multiplied to obtain the concentration estimates on soil surfaces in cores from the Unterehrendingen soil.
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But, the effect of these corrections can be completely undone by small shifts of the reflection against the fluorescence image. These shifts may lead to a large uncertainty of the estimated concentrations at the pixel scale. However, this uncertainty can be reduced at the price of reducing the spatial resolution of the concentration pattern by filtering the fluorescence and reflection image with a median filter with a window size corresponding with the displacement length of the image shifts. Yet, these shifts are relatively small compared with the resolution of classical sampling techniques.
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IN MEMORIAM Paul Gähwiller
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The experimental work of this contribution was a first step in the dissertation of Paul Gähwiller, who died in the mountains on 7 Oct. 1999. This is to commemorate his spirit of a profound scientific curiosity and his virtually unlimited willingness to help whenever help was needed.
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ACKNOWLEDGMENTS
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We wish to thank Dr. L. Schober (Institut für Physikalische und Theoretische Chemie, University Erlangen, Germany) for measuring the diffuse soil reflectances. The assistance of Dr. S. Bujukova, H.-P Läser, J. Leuenberg and H. Wydler with the experimental setup, the measurements of the breakthroughs, and the analysis of the fluorescence images was essential and very much appreciated. We are also indebted to reviewers for their high quality reviews.
The corresponding author is grateful to the Belgian Fund for Scientific Research, Flanders, which funded his research stay at the Soil Physics Laboratory of the Institute of Terrestrial Ecology (ETHZ). While carrying out this research, the corresponding author was a post-doctoral research assistant of the Belgian Fund for Scientific Research, Flanders.
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NOTES
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(deceased). 
Received for publication November 10, 2000.
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