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Allometry and evaluation of in situ optical LAI ... - Tree Physiology

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726 JONCKHEERE, MUYS AND COPPIN<br />

Table 4. Regression models used to establish allometric equations <strong>in</strong><br />

the experimental Scots p<strong>in</strong>e st<strong>and</strong> <strong>in</strong> Pijnven Forest, Hechtel-Eksel,<br />

Belgium.<br />

Regression Equation<br />

Logarithmic lny = a + bln x<br />

(10)<br />

Gaussian<br />

−b( x−c) y = ae 2<br />

(11)<br />

Log-normal<br />

2<br />

( −(ln( b−x) −c)<br />

/ 4)<br />

y = a/( b − x) e<br />

(12)<br />

Rayleigh<br />

x b c<br />

y = a −e − ( / )<br />

( 1 )<br />

(13)<br />

Power y ax b<br />

= (14)<br />

Polynomial<br />

2<br />

y = ax + bx+ c<br />

(15)<br />

L<strong>in</strong>ear y = ax+ b<br />

(16)<br />

7, 23, 38, 53 <strong>and</strong> 68°. A built-<strong>in</strong> <strong>optical</strong> filter blocked <strong>in</strong>com<strong>in</strong>g<br />

radiation with wavelengths above 490 nm, to ensure maximum<br />

contrast between leaf <strong>and</strong> sky. A reference measurement was<br />

taken <strong>in</strong> an open area directly before <strong>and</strong> after the po<strong>in</strong>t measurements<br />

to estimate above-canopy irradiance. A 90° view<br />

lens cap blocked the <strong>in</strong>vestigator from the field <strong>of</strong> view. Leaf<br />

area <strong>in</strong>dex was automatically calculated by the built-<strong>in</strong> C2000<br />

s<strong>of</strong>tware (Li-Cor 1992), based on <strong>in</strong>version <strong>of</strong> the Poisson light<br />

ext<strong>in</strong>ction model for compar<strong>in</strong>g transmittances. The ext<strong>in</strong>ction<br />

model is based on four assumptions: (1) foliage is an <strong>optical</strong><br />

black body that absorbs all the light it receives; (2) light-block<strong>in</strong>g<br />

plant elements are r<strong>and</strong>omly distributed <strong>in</strong> the canopy; (3)<br />

plant elements have the same projection as simple geometrical<br />

convex shapes; <strong>and</strong> (4) plant elements are small compared to<br />

the area covered by each r<strong>in</strong>g. Additional <strong>in</strong>formation on the<br />

operational theory <strong>of</strong> the <strong>in</strong>strument has been given by Welles<br />

<strong>and</strong> Norman (1991) <strong>and</strong> Jonckheere et al. (2004).<br />

Measurements with TRAC The TRAC <strong>in</strong>strument measures<br />

the gap fraction at the solar zenith angle. Specifically, TRAC<br />

measures the photosynthetic photon flux (PPF) through a canopy<br />

(Chen <strong>and</strong> Cihlar 1995). The <strong>in</strong>strument is carried by a person<br />

walk<strong>in</strong>g at a rate <strong>of</strong> about 0.3 m s –1 , <strong>and</strong> accounts for both<br />

canopy gap fraction <strong>and</strong> canopy gap size distribution. The measured<br />

gap fraction is used to estimate effective <strong>LAI</strong> (<strong>LAI</strong> e), <strong>and</strong><br />

the gap size distribution is used to estimate the element-clump<strong>in</strong>g<br />

<strong>in</strong>dex (Ωe).<br />

The value <strong>of</strong> Ωe, which quantifies the effects <strong>of</strong> nonr<strong>and</strong>om<br />

spatial distribution <strong>of</strong> foliage, was obta<strong>in</strong>ed by compar<strong>in</strong>g the<br />

measured gap size distribution with a theoretical gap size distribution<br />

associated with a canopy hav<strong>in</strong>g r<strong>and</strong>omly distributed<br />

foliage elements (Chen <strong>and</strong> Cihlar 1995). The value <strong>of</strong> Ωe<br />

depends on the leaf <strong>in</strong>cl<strong>in</strong>ation angle (G-function), which <strong>in</strong><br />

turn varies with the view angle. However, for a view angle <strong>of</strong><br />

57.5°, G ≅ 0.5 <strong>and</strong> can be considered <strong>in</strong>dependent <strong>of</strong> leaf <strong>in</strong>cl<strong>in</strong>ation.<br />

Therefore, by keep<strong>in</strong>g the solar radiation angle constant<br />

at 57.5°, Ωe <strong>and</strong> <strong>LAI</strong> e values for the st<strong>and</strong> can be obta<strong>in</strong>ed<br />

with TRAC alone (Leblanc et al. 2002).<br />

Measur<strong>in</strong>g <strong>LAI</strong> by hemispherical photography To estimate<br />

<strong>LAI</strong> by digital hemispherical photography, images <strong>of</strong> the canopy<br />

are acquired from below through a hemispherical (fisheye)<br />

lens with a 180° field <strong>of</strong> view. Leaf area <strong>in</strong>dex is computed from<br />

TREE PHYSIOLOGY VOLUME 25, 2005<br />

the hemispherical photographs from gap fraction estimates <strong>in</strong><br />

different zenithal <strong>and</strong> azimuthal ranges. We used a Kodak DCS<br />

660 digital camera (Eastman Kodak, New York, NY) with an<br />

8-mm fisheye lens (8 mm, f/4, Sigma, Tokyo, Japan). The camera<br />

<strong>and</strong> lens were placed <strong>in</strong> a self-level<strong>in</strong>g mount oriented by<br />

corner p<strong>in</strong>s on a tripod. The top <strong>of</strong> the lens was 1.3 m above<br />

ground <strong>and</strong> the camera was oriented such that the magnetic<br />

north was always located at the top <strong>of</strong> the photographs. Photographs<br />

were taken dur<strong>in</strong>g overcast conditions to m<strong>in</strong>imize<br />

glare from direct sunlight.<br />

For every grid po<strong>in</strong>t, six photographs were taken with an aperture<br />

<strong>of</strong> f/8 at five shutter speeds (1/60, 1/125, 1/250, 1/500<br />

<strong>and</strong> 1/1000 s) <strong>and</strong> at the highest possible resolution, i.e., 3040<br />

× 2008 pixels. The photograph result<strong>in</strong>g <strong>in</strong> the best contrast<br />

between sky <strong>and</strong> canopy was selected visually from these<br />

bracketed exposures. A total <strong>of</strong> 30 photographs provided <strong>in</strong>put<br />

for analysis by the Gap Light Analyzer (GLA) s<strong>of</strong>tware which<br />

computes gap fraction data <strong>and</strong> <strong>LAI</strong> (Frazer et al. 1999, Frazer<br />

et al. 2001). First, a threshold value was <strong>in</strong>teractively selected<br />

for each photograph to dist<strong>in</strong>guish between visible sky <strong>and</strong> foliage,<br />

thereby convert<strong>in</strong>g the RGB color images to black <strong>and</strong><br />

white. The border can be difficult to estimate because <strong>of</strong> the<br />

penumbral effect; therefore, all photographs were analyzed by<br />

the same experienced operator to reduce variation (Beaudet<br />

<strong>and</strong> Messier 2002). To compare <strong>LAI</strong> estimates from the hemispherical<br />

photography technique with the <strong>LAI</strong>-2000 results,<br />

gap fractions from the photographs were similarly separated <strong>in</strong><br />

five zenith r<strong>in</strong>gs from 0–75°. The five zenith r<strong>in</strong>gs were divided<br />

<strong>in</strong>to sky sectors by 10° azimuth angles (36 azimuth sectors).<br />

In a second step, <strong>LAI</strong> e was calculated for each<br />

photograph from the gap fraction data obta<strong>in</strong>ed by <strong>in</strong>version <strong>of</strong><br />

the Poisson model us<strong>in</strong>g 4 <strong>and</strong> 5 r<strong>in</strong>gs, represent<strong>in</strong>g 0–60° <strong>and</strong><br />

0–75°, respectively (Stenberg et al. 1994). The s<strong>of</strong>tware takes<br />

terra<strong>in</strong> corrections, based on local aspect <strong>in</strong>puts <strong>and</strong> lens corrections,<br />

<strong>in</strong>to account. As <strong>in</strong>put to the GLA program, data for<br />

the terra<strong>in</strong> corrections were gathered <strong>in</strong> the field <strong>and</strong> data for<br />

the lens correction were supplied by Sigma. We then converted<br />

<strong>LAI</strong> e to corrected <strong>LAI</strong> by correct<strong>in</strong>g for clump<strong>in</strong>g <strong>and</strong> nonleafy<br />

material.<br />

Foliage clump<strong>in</strong>g Estimates <strong>of</strong> <strong>LAI</strong> acquired by <strong>optical</strong> techniques<br />

are based on light <strong>in</strong>terception by both foliage <strong>and</strong><br />

stems, <strong>and</strong> assume a r<strong>and</strong>om foliage distribution (Chen <strong>and</strong><br />

Cihlar 1995). The result<strong>in</strong>g <strong>in</strong>dex is therefore considered to be<br />

the effective leaf area <strong>in</strong>dex (<strong>LAI</strong> e) (Chen et al. 1991). Consequently,<br />

when convert<strong>in</strong>g <strong>LAI</strong> e to <strong>LAI</strong> it is necessary to correct<br />

both for light obstruction from non-leafy canopy material <strong>and</strong><br />

for the effects <strong>of</strong> foliage clump<strong>in</strong>g. Foliage clump<strong>in</strong>g occurs<br />

mostly at the shoot level <strong>in</strong> conifers (Stenberg et al. 1994). Foliage<br />

clump<strong>in</strong>g also occurs at the branch <strong>and</strong> crown levels for<br />

most forest types (Chen <strong>and</strong> Black 1992), as a result <strong>of</strong> branch<strong>in</strong>g<br />

patterns <strong>and</strong> irregular tree distribution (Chen et al. 1997).<br />

We applied several corrections to <strong>in</strong>vestigate the <strong>in</strong>fluence <strong>of</strong><br />

clump<strong>in</strong>g at the shoot, branch <strong>and</strong> tree levels on the conversion<br />

<strong>of</strong> <strong>LAI</strong> e measured <strong>optical</strong>ly to corrected <strong>LAI</strong>.<br />

Shoot-level clump<strong>in</strong>g We corrected for clump<strong>in</strong>g at the shoot<br />

level based on the method <strong>of</strong> Gower <strong>and</strong> Norman (1991), which<br />

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