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Technical Comments
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| 1. |
J.-F. Molino and
D. Sabatier,
Science
294,
1702
(2001)
|
| 2. |
J. H. Connell,
Science
199,
1302
(1978)
|
| 3. | N. J. Gotelli, G. R. Graves, Null Models in Ecology (Smithsonian Press, Washington, DC, 1996). |
Response: Although apparently trivial, the mixing effect described by Arim and Barbosa fits perfectly with the intermediate disturbance hypothesis. We can assume that the two groups of species are guilds, and that disturbance is the only force that can constrain them to mix (2). Since, as the comment demonstrates, mixing automatically increases diversity, a humped pattern must appear with any efficient disturbance indicator.
Interestingly, this mixing effect does not explain our disturbance-diversity relationship. We applied the procedure of Arim and Barbosa to the 3554 heliophilic stems (HS) (91 species) and 7972 nonheliophilic stems (NHS) (404 species) of figure 2 in (1). We used 40-stem samples and Hurlbert's rarefaction method (3) to calculate the expected species richness, E(S40) = E(Shs) + E(Snhs), where hs + nhs = 40. In the corresponding model (curve a in Fig. 1A), variations in species richness result only from changes in group proportions along the gradient: When calculated separately within each group--that is, for pure heliophilic or nonheliophilic samples--E(S40) does not vary with the percent of stems that are heliophilic (curves a' and a" in Fig. 1B). The observed values on quadrats (curve c in Fig. 1A) strongly depart from this model, which indicates that other processes are involved.
Fig. 1.
Species richness in 40-stem samples
[E(S40)] as a function of the percentage of
heliophilic stems (%HS) [using data set of figure 2 in
(1)]. (A) Expected and observed species
richness, E(S40) = E(Shs) + E(Snhs),
for both heliophilic and nonheliophilic stems. Curve a shows
the expectation of the Arim and Barbosa model, which assumes invariant
species abundance distributions; the accompanying dotted curves show
corresponding 95% confidence intervals (4). Regression
curves for the data for pooled quadrats [open triangles and curve
b; R2 = 0.9784, F(2,12) = 174.83, P <<0.001] and for the
observed values for all quadrats [solid dots and curve c;
F(2,96) = 55.86, P < 0.001] are also
shown. (B) Expected and observed species richness
patterns for nonheliophilic [E(S40) = E(Snhs)] and heliophilic
[E(S40) = E(Shs)]
species, calculated separately. According to the Arim and Barbosa
model, E(S40) should not vary with %HS for
nonheliophilic or heliophilic species (curves a' and
a"). Actual data for pooled quadrats show a humped pattern
for both nonheliophilic [curve b'; F(2,12) = 21.29, P <<0.001] and heliophilic [curve
b"; F(2,12) = 47.74, P
<<0.001] species. For calculating curves b,
b', and b", quadrats were pooled in 10%
intervals, in steps of 5%.
To completely remove the mixing effect, we plotted separately E(S40) = E(Shs) and E(S40) = E(Snhs), to show the species richness for pure HS or NHS samples. We pooled quadrats in 10% HS intervals, in steps of 5% HS, to allow the calculation of E(S40) for both groups all along the gradient. The humped patterns that appear in both cases (curves b' and b" in Fig. 1B) reveal a drift in the species abundance distributions within the individual groups along the disturbance gradient. The role of this drift can be seen if we modify the procedure of Arim and Barbosa slightly by calculating E(S40) = E(Shs) + E(Snhs) using distributions from pooled quadrats (as in curves b' and b' in Fig. 1B) rather than using the overall species' abundance distributions. The curvature of the resulting humped pattern (curve b in Fig. 1A) strongly differs from the expectation of Arim and Barbosa (curve a in Fig. 1A), but is similar in magnitude to the regression curve for the observed quadrat values (curve c in Fig. 1A).
These findings fit with the intermediate disturbance hypothesis and the niche partitioning theory: Low and high disturbance levels allow dominance of few species, whereas intermediate disturbances increase both the number of niches and species evenness.
Jean-François Molino
Daniel Sabatier
Institut de Recherche pour le Développement
UMR AMAP
TA
40/PS2
34398 Montpellier Cedex 5, France
E-mail:
molino{at}mpl.ird.fr
| 1. | J.-F. Molino and D. Sabatier, Science 294, 1702 (2001) . |
| 2. | Note the impossibility of obtaining, among our quadrats, a 0% to 80% variation in group proportions without aggregating most of the heliophilic species [see supplemental figure 5 in (1)]. |
| 3. | S. H. Hurlbert, Ecology 52, 577 (1971) [CrossRef] [Web of Science]. |
| 4. | R. Lande, Oikos 76, 5 (1996) [CrossRef] [Web of Science]. |
Science. ISSN 0036-8075 (print), 1095-9203 (online)