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Note on the compatibility of ICOS, NEON, and TERN sampling designs, different camera setups for effective plant area index estimation with digital hemispherical photography


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Introduction

Leaf Area Index (LAI), a measure of the amount of plant leaf material in an ecosystem, is defined as one half of the total green leaf area per unit ground surface area (Chen & Black, 1992; Fernandes et al., 2014). LAI is included in many models describing vegetation-atmosphere interactions (GCOS-138, 2010) as a critical variable controlling processes such as photosynthesis, respiration, and rain interception. LAI estimates using different Earth Observation (EO) data and algorithms have been developed and made available to the user community over the last decades (Fang et al., 2019) as ready-for-use products. When no adjustments are made for the clumping effect or for the interception of light by woody canopy elements when estimating LAI, the variable is the effective Plant Area Index (PAIe) instead (Chen, 1996).

The Global Climate Observing System (GCOS) has specified the need to update and validate global LAI predictions systematically. The Land Product Validation (LPV) sub-group of the Committee for Earth Observation Satellites (CEOS) developed a strategy for validating the predictions (Fernandes et al., 2014). The CEOS LPV currently encourages validation and intercomparison of the so-called LPV Supersites. The majority of the LPV Supersites come from well-known and established networks, including the Integrated Carbon Observation System (ICOS) (Gielen et al., 2017) in Europe, the National Ecological Observatory Network (NEON) (Meier & Jones, 2018) in the U.S., and the Terrestrial Ecosystem Research Network (TERN) (Karan, 2015) in Australia. However, the networks employ different sampling designs (i.e. number of measurements, location of sampling points within the test site) and camera setups for in situ LAI estimation. Previous studies have reported apparent differences in the LAI estimates from different sampling schemes (Calders et al., 2018; Liu et al., 2021; Majasalmi et al., 2012; Nackaerts et al., 2000; Zou et al., 2020).

The objective of this study is to compare the three different schemes adopted within the ICOS, NEON, and TERN networks instead of searching for the most optimal, new sampling scheme. We carried out the intercomparison measurements with digital hemispherical photography during diffuse light conditions, adopting the established ICOS, NEON, and TERN sampling schemes. We use data from a measurement campaign conducted in 2021 at the Järvselja Radiation Transfer Model Intercomparison (RAMI) (Widlowski et al., 2015) birch stand. The impacts of the sampling schemes and camera setups on the gap fraction and (PAIe) prediction and estimation from digital hemispherical photography (DHP) were analysed.

Material and Methods
Study site

The measurements were conducted in a 63-year-old, mature fertile silver birch (Betula pendula Roth) forest stand in Järvselja, Estonia (58°16′ 49.81″ N, 27°19′ 51.53″ E), which belongs to the RAMI dataset (Widlowski et al., 2015). It is an intensively studied site that serves in various forest reflectance modelling and remote sensing experiments. The dominating upper layer has a basal area of 28.2 m2 ha−1 that is distributed between silver birch 55%, common alder (Alnus glutinosa (L.) Gaertn.) 31%, and European aspen (Populus tremula L.) 14%. The stocking density was 966 trees per hectare according to 2019 measurements (Lang et al., 2021). Kuusk et al. (2013, 2009) and Lang et al. (2021) have given a more detailed site description. The stand contains a 100 m × 100 m sample plot, within which all digital hemispherical photographs were taken (Figure 1). Lang & Pisek (2019) describe the changes in the canopy gap fraction regarding the growth of the forest stand understorey and dominant tree layer.

Figure 1.

Positions for digital hemispherical photography within the test site of Järvselja RAMI birch stand.

Joonis 1. Mõõtmispunktide asukohad Järvseljal RAMI kaasikus vastavalt erinevatele skeemidele. 

Data acquisition and processing

Three sampling schemes corresponding to the ICOS, NEON, and TERN schemes (each consisting of 36 individual sampling points) were used in this study (Figure 1). The ICOS (Gielen et al., 2017) scheme has four circular continuous plots, each consisting of 9 sampling points. The NEON (Meier & Jones, 2018) scheme has three “tower” type plots that consist of 12 sampling points in a cross pattern oriented in the cardinal directions. The TERN (Karan, 2015) scheme is a regular 6 by 6 grid of measurement points across the whole plot. The position of each sampling point in the field was established with a land survey tape and a compass, and marked with stakes and flags to facilitate the DHP image collection.

Three camera setups were used (Table 1), with each operated by a different individual. At each sampling point, the DHP images were taken in immediate sequence with the three different camera setups under overcast, diffuse illumination conditions on August 30, 2021. All the images were stored in a camera-specific raw format. The cameras were fixed to a tripod approximately 1.3 m above the ground at each measurement point. The top of the image was oriented to the magnetic north using a compass. Each camera was pointed upwards and levelled using a two-axis bubble level, the focus setting on the lenses was set to infinity. The weather was dry, the ambient temperature was 15–20 °C, with almost no wind.

Camera setup specifications.

Tabel 1. Mõõtmisteks kasutatud kaamerad. 

Variable Camera setup

I II III
Camera model Canon EOS 5D Canon EOS 600D Canon EOS 2000D
Fisheye Lens Sigma 8 mm F3.5 EX DG Sigma 4.5 mm F2.8 EX Sigma 4.5 mm F2.8 EX
Camera height 1.3 m 1.3 m 1.3 m
Camera orientation magnetic north magnetic north magnetic north
Initial ISO 640 400 100
Initial exposure compensation 0 0 −1
Initial shutter speed 1/32 1/60 Aperture priority
Image aquisition single single auto-bracketing
F-stop f/8 f/8 f/8
Light metering Spot Evaluative Evaluative
Sensor size, pixels 12.8×106 18.0×106 24.1×106
Raw image radius* 1386 1450 1730

Image radius on senor (pixels for 90 deg. zenith angle).

For camera setups I and II, the camera settings (shutter speed and ISO) were adjusted manually at each sampling point to take images with no overexposure and to keep pixel maximum value within the interquartile range of the camera's dynamic range (Lang et al., 2017). This was necessary, because the incident radiation varied over time, with the sun rising and cloud cover thickness changing. Image blue-channel histogram was used to assess the necessity for adjustments. For camera setup III, an auto exposure bracketing function was used to take images. The base exposure was set to −2 EV at ±1 EV stop, resulting in a series of images at three consecutive EVs: −3, −2, and −1. However, later we discovered that this still caused overexposure on all of the photos at some measurement points because the camera was operated in a semiautomatic aperture priority mode.

All acquired DHP images were processed with the free image processing software Hemispherical Project Manager (https://kosmos.ut.ee/en/services/free-hemispherical-software). The HSP implements the LinearRatio method (Cescatti, 2007) that takes into account the linear response to light on the camera sensors and implements the method for a single below-the-canopy-operated camera (LinearRatioSC). As some acquired DHP for setup III encountered overexposure, we processed the images taken at −2 EV exposure compensation to reduce such effects. The pixel values were extracted with dcraw version 9.17 for setup I and version 9.28 (Coffin, 2018) for setups II and III, without colour interpolation and brightness scaling (-D switch). Dark frame values were subtracted (-K switch), and the 16-bit linear output was selected (−4 switch). Authentic blue pixels were sampled according to the sensor filter pattern. Circular fisheye images with linear projection were obtained after correcting for projection distortion and vignetting in setup I. No vignetting correction was applied for setups II and III because it had not been measured for them. However, all camera setups used the F-stop value of f/8, and in that configuration the vignetting effects are noticeable only at extreme viewing angles. Also, because of its principle, the LinearRatioSC method is much less sensitive to vignetting compared to methods based on threshold or pixel classification. For the LinearRatioSC unobscured sky pixel values were sampled from canopy gaps. The above-canopy reference images were then predicted using standard overcast sky models (ISO/CIE, 2004) fitted to sky radiance samples in combination with interpolation of pixel values similar to Lang et al. (2017, 2010). The canopy gap fraction Po for each pixel was then calculated as Po=IbIa {P_o} = {{{I_b}} \over {{I_a}}} where Ia is the predicted above-canopy radiance and Ib is the measured below-canopy radiance.

Effective Plant Area Index calculation

The gap fraction function Po(θ) can be used to calculate the effective LAI (Le) using the formula proposed by Miller (1967): Le=20π/2[lnPo(θ)]cosθsinθdθ. {L_e} = 2\int_0^{\pi /2} { - \left[ {ln {P_o}\left( \theta \right)} \right]cos \theta sin \theta d\theta } . In our case we have gap fraction data over the hemisphere, sampled from 20 rings on the projected hemispherical image, each covering 4.5 degrees (0.0785 radians) of the zenith view angle. Therefore, we replace the integral calculation with a sum. Also, as we do not distinguish between foliage and woody material, we use the term effective Plant Area Index (PAIe) instead of LAI: PAIe2Δθn=1NlnPo(θn)cosθnsinθn, {PAI_e} \approx - 2\Delta \theta \sum\limits_{n = 1}^N {ln {P_o}\left( {{\theta _n}} \right)cos {\theta _n}sin {\theta _n},} where Δθ is constant 0.0785 radians in our case and θn is the view zenith angle for the n-th ring. We use Equation (2) to calculate the mean PAIe for a set of images by taking the logarithm of the average of the gap fractions Po(θn)¯ \overline {{P_o}\left( {{\theta _n}} \right)} sampled from the images for each ring.

Results

The layout of image locations, i.e. sampling grid has some effect on the gap fraction estimate at stand level (Figure 2). The most significant differences between the sampling schemes occur near the zenith and smaller viewing angles. The differences in camera setups can also be noticed. Results from all setups correlate well with each other with R2 values around 0.99, but setups I and II give a more similar gap fraction across view angles (average difference 0.005), whereas setup III deviates more from setups I and II (average difference 0.01 from setup I). Gap fractions from setups I and II consistently differ a little. Setup I almost always has a slightly smaller value for the gap fraction in all viewing zenith angles except the very small and the very large ones (Figure 2).

Figure 2.

Comparison of the average gap fraction of the test stand with different camera setups (SI, SII, SIII) using ICOS, NEON and TERN sampling schemes.

Joonis 2. ICOS, NEON ja TERN võrgustikel kolme erineva kaameraga (SI, SII, SIII) tehtud mõõtmis-test arvutatud keskmised võrastiku läbipaistvused sõltuvalt vaatesuuna seniitnurgast. 

Based on the gap fraction, PAIe estimates also vary between schemes and camera setups. The overall PAIe, for the test site based on all schemes and all camera setups, comprising a total of 324 images, was 3.09 with a standard error (SE) of 0.02. Following Majasalmi et al. (2012), it is assumed that this very large set of 324 measurements is representative of the population mean. Here it is assumed that there is no influence of different measurement devices and operators on observations, however, later we show that each measurement series with a particular device had its own uncertainty characteristics. The ICOS and TERN schemes result in slightly smaller estimations for the PAIe (2.99 and 3.03, respectively) than the NEON (3.26) scheme (Table 2). As the gap fraction estimation was consistently different between setups I and II, the resulting PAIe estimation also reflects this difference, and the PAIe values are consistently a little bit greater for setup I than for setup II. The PAIe estimation for setup III stays close to the estimates of other two setups. Overall average PAIe estimations for all setups and schemes ranged from 2.90 to 3.38, with standard errors ranging from 0.04 to 0.06 (Table 2).

Estimations of effective plant area index PAIe for each sampling scheme taken with each setup and their corresponding standard errors (SE).

Tabel 2. Mõõtmisvõrgustike (ICOS, NEON, TERN) ja kaamerate (Setup I, II ja III) kaupa võrastiku läbipaistvusest arvutatud efektiivne taimkatteindeks PAIe ja selle standardviga (SE).

Camera Sampling network


ICOS NEON TERN



PAIe SE PAIe SE PAIe SE
Setup I 3.11 0.06 3.38 0.05 3.11 0.06
Setup II 2.99 0.06 3.22 0.05 2.94 0.05
Setup III 2.90 0.05 3.21 0.04 3.08 0.06

All three cameras took images at the same marked locations within a few minutes. Still, there are always slight deviations in positioning the cameras precisely at the same spot with identical levelling and orientation. This causes some variability in the recording of the scene content. Each camera operator processed the images taken with a particular camera. This also introduces some small variability into the results because (1) the markers of open sky pixel sampling markers can be freely chosen and (2) identification of canopy gaps at larger view zenith angles for extracting sky pixel samples requires some practicing and experience. However, Lang et al. (2013) show that the influence of randomness in open sky sampling point locations due to different analysts is marginal for the LinearRatioSC. The PAIe calculated from camera setups I and II has a very strong correlation (R2 = 0.94) within image pairs, but setup III varied more in the results, giving often quite large deviations in the sampling points compared to setups I and II (Figure 3). Although setups I and II correlate well, the linear model fitted on the data has a slope around 0.91 and is also slightly shifted away from the 1 to 1 line, indicating a small systematic difference in the PAIe.

Figure 3.

Effective plant area index PAIe calculated from the data of three camera setups. RSE is the linear regression residual error. Overexposed measurements with Setup III are marked with red crossed circles and excluded from the regression.

Joonis 3. Mõõtmispunktides saadud efektiivse taimkatteindeksi PAIe võrdlus erinevate kaamerate (Setup I, II ja III) kaupa. Kaamera III ülevalgustatud mõõtmised on tähistatud punaste ringristidega ja regressioonimudelist välja jäetud. RSE on mudeli jääkviga. 

As the forest stand is natural, i.e. not perfectly homogeneous, it can be expected that the PAIe obtained at different measurement points would vary, for example for setup I, the PAIe calculated from single images ranges from 2.45 to 4.06 (Figures 4, 5, 6). However, the PAIe includes both – the true value and uncertainty that is introduced during the measurements and data processing.

Figure 4.

PAIe values from three camera measurements for the ICOS scheme and the locations of the sample images shown in Figure 7.

Joonis 4. Efektiivse taimkatteindeksi PAIe väärtused mõõtmiste jadas ICOS võrgustiku punktides. Ristiga on näidatud joonisel (8) toodud näidispildi mõõtmispunkt. 

Figure 5.

PAIe values from three camera measurements for the NEON scheme.

Joonis 5. Efektiivse taimkatteindeksi PAIe väärtused mõõtmiste jadas NEON võrgustiku punktides. 

Figure 6.

PAIe values from three camera measurements for the TERN scheme.

Joonis 6. Efektiivse taimkatteindeksi PAIe väärtused mõõtmiste jadas TERN võrgustiku punktides. 

Figure 7.

Zoomed-in central parts of the blue channel of the photos taken from ICOS point A8 with setup I (A), setup II (B), and setup III (C).

Joonis 7. Suurendus kaameratega (I, II ja III) ICOS võrgustiku punktis A8 tehtud ülesvõtte keskosast. Kaamera III pildil on näha tugeva ülevalgustatuse ilminguid. 

Setup III had a problem with overexposure due to the semiautomatic imaging mode. Some images were out of focus – possibly due to accidental turning of the focus wheel, resulting in loss of detail in smaller gaps, leaves and branches (Figure 8). Even though setup III had the highest pixel resolution, the loss of small details due to the wrong focus setting combined with overexposure did contribute to inconsistent results at many sampling points demonstrated by PAIe values compared to setups I and II (Figure 3B, C). We identified overexposed measurements of setup III based on possible maximum pixel values according to the camera radiometric resolution (also known as bit depth) and found that the concordance of the rest (i.e. correct measurements with setup III) with the other measurements was strong (Figure 3B, C).

Figure 8.

Comparison of differences in average gap fractions in the ICOS scheme calculated from measurements with setup I and setup II and processed by the camera operators OpI or OpII. The influence of the image analyst is small compared to the camera factor.

Joonis 8. ICOS mõõtmisvõrgu andmetel saadud võrastiku keskmise läbipaistvuse erinevus kaamerate I ja II andmetel. Sama kaamera piltide töötlemisel on operaatori mõju (OpI, OpII) väike võrreldes kaamera faktoriga. 

The impact of image overexposure on the measurements of the canopy gap fraction and consequently PAIe was not constant. The PAIe of some of the overexposed measurements was not much different from setup I and setup II, which can be attributed to the magnitude of overexposure and also to the amount of mixed pixels in the scene where “burn-in” effects occur first. Additionally, the out-out-of-focus problem tended to fill small canopy gaps of few pixels in size, effectively decreasing the canopy gap fraction. Therefore, it is the responsibility of the camera operator to keep the camera in the linear sensitive range of the sensor to avoid overexposure and systematic errors in the canopy gap fraction and PAIe.

The PAIe values obtained at each sampling point correlated well between setups I and II with R2 values of 0.97 for ICOS, 0.89 for NEON, and 0.92 for TERN (Table 3). The differences in correlation are probably due to the uncertainty of measurements and cannot be attributed to a particular sampling scheme. Overexposed measurements decreased substantially the correlation of setup III with the others. However, in the subset of correct measurements that did not suffer from overexposure, the correlations were of the same strength than between setup I and setup II (Table 3).

Linear relationships between effective plant area index between three camera setups by sampling schemes and using only correct (C) i.e. non-overexposed images of setup III or all (A). RSE is model residual error and N is the number of observations.

Tabel 3. Lineaarsed regressioonmudelid kaamerate ning mõõtmisskeemide kaupa. Kaamera III mudelid on antud kõikide (A) või ainult korrektsete mõõtmiste ehk ülevalgustamata piltide andmete (C) järgi. RSE on mudeli jääkviga ning N on vaatluste arv.

Camera setup Sampling Linear regression Sy = a + bSx



Sx Sy Network Subset R2 a b RSE N
I II ICOS A 0.97 0.21 0.89 0.06 36
I II NEON A 0.90 0.05 0.94 0.10 36
I II TERN A 0.92 0.21 0.88 0.09 36
I III ICOS A 0.28 1.55 0.45 0.27 36
I III ICOS C 0.92 0.10 0.96 0.10 21
I III NEON A 0.23 1.90 0.40 0.23 36
I III NEON C 0.84 −0.52 1.15 0.12 23
I III TERN A 0.71 0.55 0.81 0.18 36
I III TERN C 0.84 0.10 0.97 0.13 24
II III ICOS A 0.29 1.44 0.50 0.27 36
II III ICOS C 0.93 0.02 1.02 0.09 21
II III NEON A 0.17 2.15 0.35 0.24 36
II III NEON C 0.85 −0.73 1.28 0.12 23
II III TERN A 0.77 0.36 0.92 0.16 36
II III TERN C 0.87 0.16 1.01 0.12 24

As we noticed some systematic differences in camera setups I and II, we conducted an experiment where the images of the ICOS scheme were cross-processed by the camera operators to see if there was some human error or bias. We found a small difference in the estimated gap fraction around the large viewing angles (Figure 8) but overall, the results are not statistically different from each other with a one-tail t-test p-value of 0.486.

Discussion and Conclusion

An estimation of plant or leaf area index for a test site using optical measurements of canopy gap fraction or gap size distribution is influenced by many factors that introduce uncertainty into the results. In our study, we focused on the sampling design, field measurements, and image processing. Sampling design, in an ideal case, (1) provides that enough measurements are made to obtain sufficiently narrow confidence intervals for the estimates and (2) ensures that repeated measurements in time series are comparable by fixing, for example, the arrangement of permanent and random sampling points. The stage of field measurements involves uncertainties related to configuring cameras, locating measurement points, setting up the camera on the point, observing illumination conditions according to the measurement protocol, determining exposure settings to keep the camera in its linear sensitivity range, and the physical process of taking images. Image processing involves extracting the data from camera output files, applying radiometric and geometric corrections, selecting the image processing method and its parameters and software, and calculating the gap fraction according to the view zenith angle from the processed images for the Equation (2). Prediction of the true green leaf area index further from the canopy gap fraction includes another wide range of models and methods.

We used three different sampling schemes and obtained the PAIe in the range of 2.99–3.26 for the Järvselja RAMI birch stand. The result is close to Kuusk et al. (2009), who reported PAIe 2.94 measured at nine positions with the LAI-2000 instrument within the same test site. The small increase in PAIe values compared to Kuusk et al. (2009) can be explained by a growth of dominant and lower tree layers during the period (>15 years) between the measurements (Lang & Pisek, 2019). The PAIe derived from ICOS and TERN sampling schemes were more similar to each other (two-tailed t-test p-value 0.229) than NEON (t-test p-value < 0.00001) results (Table 2). The difference between NEON results compared to the other schemes may be explained by the distribution of the sampling points in the forest. The NEON scheme has three tightly packed locations in the forest where images are taken, whereas TERN and ICOS are more spread out over the whole plot (Figure 1). With NEON, the initial selection of the three sub-section locations is important because if two or all three locations fall into either more open or closed canopy areas, the sample is not representative of the forest as a whole. Even though we followed the scheme layout instructions carefully, with our testing, two of the locations happened to have rather closed canopy conditions and the resulting images gave on average a smaller gap fraction when compared to the ICOS and TERN sampling schemes (Figure 2). The NEON protocol uses this kind of sampling in conjunction with a second larger set of distributed plots that are sampled less frequently but cover more of the forests. The tower plots described in the NEON protocol can give a good time series of the area near the sampling points, but they should be viewed together with the distributed plots results to properly represent a forest site.

Proper camera configuration is essential to get consistent and comparable measurements. As our goal was to measure incident radiation as precisely as possible, it was necessary to avoid over- or underexposing the image. In our testing, setup III illustrated possible issues with overexposed and out-of-focus images where smaller details of the canopy were often lost (Figure 7C). This resulted in occasional inconsistent results when compared to setups I and II, which had a very good correlation with each other (Figure 3A). When tested afterwards, reducing the focus setting of the camera decreased the effective PAIe by 1.3% on average when the focus was turned down from infinity to 0.2 meters. When intentionally overexposing the images the PAIe decreased significantly. When an image with no overexposed pixels was compared to another one that had 0.1% of pixels overexposed to the maximum digital value of the sensor, the PAIe decreased by around 1.7%. When the amount of overexposed pixels was around 0.4%, the PAIe decreased substantially by 14%. Here we see that for obtaining data for the canopy gap fraction it is crucial to operate hemispherical cameras in their linear sensitive range.

Our intercomparison test allowed us to search for possible influences of cameras and image analysts on the canopy gap fraction and calculated PAIe. There was very strong correlation between the PAIe of setups I and II with a small systematic difference. In a time series this could be interpreted as a possible change in the PAIe, but in our experiment the measurements were done almost within a few minutes in time that excludes the change in the PAIe. For image processing we used a well-established method LinearRatioSC that, by its principle, is an analogue for LAI-2000 when compared to various threshold-based and pixel classification-based algorithms. To apply LinearRatioSC the image analyst has to place sky pixel sampling marks for constructing open sky reference which involves a subjective decision to some extent.

We tested the influence of operator subjectivity by cross-reprocessing the ICOS scheme images that were taken with setup I and II by corresponding operators. However, no statistically relevant differences were found in the gap fraction calculated from the same set of images processed by two different people (Figure 8). This indicates that there is a more fundamental reason stemming from the raw images or cameras themselves. We also tested the effects of vignetting and projection models, subtracting the dark images, and the effects of different versions of dcraw. They all had negligible or no impact on the results. Setup I consistently had a little but smaller gap fraction than setup II. Addressing all these possible sources of uncertainty, we conclude that the difference may be caused by light scattering and colour crosstalk within cameras. Another possible reason could be a small systematic difference in camera height over the ground or vertical levelling during field measurements. For example, a two-degree error in camera levelling changes the path length at 57° view zenith angle up to three metres (10%) in the stand. As a conclusion, we recommend always to carry out intercomparison measurements with old and new cameras when devices are upgraded.

Overall, we illustrate that the three different employed schemes produce comparable results for estimating the gap fraction and PAIe. Although different setups and schemes gave differing results, with Anova Two-Factor test p-values <0.001, there was no connection between the camera setup used and the scheme (p-value 0.178). Our testing shows that more evenly spread out sampling schemes are more consistent with each other, exemplified by ICOS and TERN, and could be more representative of the overall conditions of the forest. The results vary when different cameras with different operators are used, but it appears that 36 images employed by all three setups are enough to deliver an average with sufficiently narrow confidence limits. It depends on the application what type of cameras and how high accuracy of calibration is required. From this study we cannot conclude which scheme or camera setup is best used in the field, because all these established schemes vary slightly in their intended use and purpose and are not necessarily intended to yield site level mean estimates. But we did conclude that some layout schemes may have inherited problems when applied to estimate the PAIe for our 1-hectare plot. The CEOS Land Product Validation Subgroup (Morisette et al., 2006) suggests in their proposed framework, for validating LAI products, to use a two-staged sampling design. In the case of NEON and ICOS, the circular and cross shaped compact sampling areas would be considered elementary sampling units used together with high spatial resolution satellite data to capture the variability in the site extent. These two sampling schemes are not directly designed to capture the average PAIe for a 1-hectare site as in our case.

The CEOS LPV is currently in the process of selecting supersites with a fully characterized land surface and vegetation cover for the parameterization of 3D radiative transfer models. Our study contributes towards establishing the procedures for uncertainty estimation by evaluating potential systematic errors stemming from collecting in situ measurements with DHP using different scheme designs, methods and devices currently in use at most LPV Supersites.

Future work can include efforts to investigate the impact of sampling schemes on the LAI estimation of forests from other indirect LAI measurement methods (e.g. terrestrial laser scanner and LAI-2200). Ground-Based Observations for Validation (GBOV) of Copernicus Global Land Products (GBOV, 2023) uses schemes studied in this paper to validate its decametric and hectometric satellite-derived LAI products (Brown et al., 2020) and thus it is important to study these schemes. More comparisons between measurement methods and data processing methods would be useful in determining the most reliable ways to gather data on the gap fraction. Forest plots with different plant functional types may also be included to consolidate the findings of this study.

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Life Sciences, Plant Science, Ecology, other