TBCD Links Centriologenesis, Spindle Microtubule Dynamics, and Midbody Abscission in Human Cells
The timing of abscission affects dispersal distance in a wind‐dispersed tropical tree
Transcript of The timing of abscission affects dispersal distance in a wind‐dispersed tropical tree
The timing of abscission affects dispersal distance in awind-dispersed tropical treeKyle D. Maurer*,1, Gil Bohrer1, David Medvigy2 and S. Joseph Wright3
1Department of Civil Environmental, & Geodetic Engineering, The Ohio State University, Columbus, Ohio, USA;2Department of Geosciences, Princeton University, Princeton, New Jersey, USA; and 3Smithsonian Tropical ResearchInstitute, Apartado 0843-03092, Balboa, Panama
Summary
1. Seed dispersal is a short-term phenomenon with long-term consequences for population sur-
vival and spread. Physiological mechanisms that target the release of seeds to particular sets of
environmental conditions that maximize the probability of long-distance dispersal should
evolve if long dispersal distance enhances fitness.
2. In this study, we use high-frequency censuses of seeds actually dispersed, high-frequency
within-canopy meteorological observations and long-term measurements of above-canopy
wind to investigate the environmental conditions that control the timing of seed abscission at
different time-scales for a wind-dispersed tropical tree, Luehea seemannii.
3. We show that seed abscission follows a typical seasonal pattern, is rare at night and is most
prevalent during periods of prolonged updrafts, higher temperature, with negative feedback
when the heat canopy flux is relatively high.
4. We use phenomenological (super-WALD) and mechanistic (coupled Eulerian–Lagrangianclosure) models to estimate the relative effects of the timing of seed release at different suban-
nual temporal scales (seconds–hours) on the resulting long-term (season–decade) dispersal ker-nels. We find that periods of high wind speed increase the probability of long-distance
dispersal between 100–1000 m, but decrease the probability at distances further than 1000 m
relative to unbiased environmental conditions. We also find abscission during updrafts to
increase the probability of long-distance dispersal at distances greater than 100 m.
5. Synthesis: We observe preferential abscission during updrafts in a tropical wind-dispersed
tree. We use mechanistic models and long-term wind statistics to estimate the dispersal conse-
quences of preferential seed release in specific environmental conditions. We find that the tim-
ing of the dispersal season may be influenced by wind conditions that maximize long-distance
dispersal; however, there are likely other environmental factors essential for their determina-
tion. Our approach provides a method to bridge between small turbulence scales and large eco-
system scales to predict dispersal kernels. These findings shed light on the evolutionary
processes that drive optimization of the timing of seed abscission and may be incorporated
into plant population movement models to increase their accuracy and predictive power.
Key-words: abscission, dispersal, long-distance dispersal, mechanistic modelling,
meteorology, seed trap, tropical forest, updraft, wind dispersal
Introduction
Seed dispersal determines the ability of plant populations
to sustain viable metapopulations (Bohrer, Nathan & Volis
2005; Poethke, Dytham & Hovestadt 2011), maintain
genetic diversity (Volis et al. 2005; Fayard, Klein & Lefe-
vre 2009) and respond to climate change through migra-
tion (Kuparinen et al. 2009; Nathan et al. 2011; Kremer
et al. 2012). Seed dispersal of an individual plant occurs
once in its lifetime and is, intrinsically, a short-term (milli-
seconds–minutes) phenomenon. However, over ecological
and evolutionary time-scales, patterns of many movement
events of individuals accumulate to long-term (seasons –
years) and large-scale (metres–kilometres) processes (Theo-
harides & Dukes 2007). Selection for traits that optimize
the dispersive potential of seeds may act on processes at*Correspondence author. E-mail: [email protected]
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society
Functional Ecology 2013, 27, 208–218 doi: 10.1111/1365-2435.12028
long time-scales, such as the timing of the annual seed dis-
persal season, as well as short time-scales, such as the exact
moment a seed will be ejected from the pod or released
from the branch.
Thompson & Katul (2008) showed that it is possible to
integrate the probability density function of the expected
end point of individual dispersal events to predict long-
term dispersal kernels, if the long-term statistics of the
wind (i.e. the distributions of speed, direction and turbu-
lence) are known. However, phenomena at short time-
scales bias the distribution of wind conditions that are
encountered by the dispersing seeds relative to long-term
wind distributions. For example, at very short time-scales,
wind conditions experienced during the first few moments
of seed flight may differ significantly from block-averaged
conditions (i.e. 30-min mean wind speeds that are typically
available from meteorological stations) due to canopy-
induced turbulence (Bohrer et al. 2008), the aerodynamic
shape of seeds (Greene & Johnson 1990; Lentink et al.
2009) or the environmental conditions that lead to seed
abscission (Greene 2005; Wright et al. 2008; Greene &
Quesada 2011). At longer time-scales, the distribution of
wind conditions when seeds are available (i.e. the dispersal
season) may differ from the distribution of wind conditions
during the entire year (Wright et al. 2008). These biases in
wind conditions may change the dispersal kernel and lead
to higher mean dispersal distances and/or more frequent/
stronger events of long-distance dispersal (LDD) (Nathan
2006; Nathan et al. 2008).
For plants that are dependent on LDD, a possible set of
traits that could be optimized involves the timing of seed
abscission such that seeds are released when external con-
ditions favour LDD (Skarpaas & Shea 2007; Soons &
Bullock 2008). Traditionally, experiments have attributed
increased LDD probability to seed abscission during
strong horizontal winds (Soons et al. 2004; Greene 2005;
Jongejans et al. 2007; Greene, Quesada & Calogeropoulos
2008), by suggesting that strong horizontal winds are cor-
related with high turbulence, including upward vertical
perturbations of the wind. Over the long term and large
scale, vertical wind is a mean-zero process, which means
that strong turbulence will produce both updrafts and
downdrafts. Therefore, strong turbulence may both
enhance and hinder dispersal over the course of each
dispersal event. Dispersal models have shown that updrafts
enhance LDD (Nathan et al. 2002; Tackenberg, Poschlod
& Kahmen 2003; Bohrer et al. 2008), and therefore,
we hypothesize that updrafts should provide the preferred
release condition for wind-dispersed seeds that are
dependent on LDD.
Physiologically, targeting updrafts is not a simple task.
Forces in all directions, such as drag forces generated by
wind flowing past the seed and the turbulent shaking of
branches, will potentially detach the seeds when the wind
is strong but not necessarily upward. Therefore, seeds need
to combine directional aerodynamic shapes and release
mechanisms that favour abscission when the applied force
pulls the seed in the desired upward direction. This intui-
tive notion that wind-dispersed plants have morphological
mechanisms to preferentially release seeds during updrafts
was demonstrated in artificial settings in maple trees
(Greene & Johnson 1992) and with the forb Tragopogon
dubius (Greene & Quesada 2011).
We used field measurements (seed arrival and meteoro-
logical measurements) and long-term data sets (seed trap
and meteorology) to disentangle the effects of different sea-
sonal and meteorological forcing on seed abscission and
dispersal at different time-scales in a natural tropical forest
environment for the neotropical tree Luehea seemannii
(Triana & Planch.). We used phenomenological and mech-
anistic dispersal models to integrate the short-term out-
comes of these environmentally driven abscission
conditions and resolve the consequences of these effects for
long-term dispersal kernels.
Materials and methods
S ITE DESCRIPT ION
The study took place at the canopy crane research facility
located in the 350-ha Parque Natural Metropolitano (PNM),
Panama (8°59′N, 79°33′W). The approximately 100-year-old
natural secondary forest is classified as a dry, lowland forest
(Holdridge et al. 1971) and contains more than 300 tree species.
Canopy heights range from 20 to 40 m. Annual precipitation
averages 1740 mm. A single dry season extends from mid-Decem-
ber through April, and a single wet season that includes 90% of
annual precipitation comprises the remainder of the year (http://
biogeodb.stri.si.edu/physical_monitoring/).
SPEC IES DESCRIPT ION
Luehea seemannii (Triana & Planch.), Malvaceae, ranges through-
out Mesoamerica and northern South America and is a canopy
tree that reaches heights of 35 and 40 m at the PNM and Barro
Colorado Island (BCI), respectively. The light-demanding seed-
lings only establish in forest gaps where light reaches the forest
floor (Molofsky & Augspurger 1992). These establishment require-
ments favour LDD because forest gaps are rare, comprising less
than 2% of forest area. The fruit is a hard dry capsule that splits
open to expose the diaspores (Fig. 1). The diaspores are 4-mm-
long samaras, weigh just 2�5 mg (fresh mass; SJW, unpublished
data) and have a low fall velocity (0�7 � 0�07 ms�1, mean � 1
S.D. (Augspurger 1986)). Most fruit are oriented vertically (above
the horizontal) so that the open fruit points skyward. The diasp-
ores disperse towards the end of the dry season, when the trade
winds are strongest, the forest canopy is relatively open due to
deciduousness and the imminent wet season will provide the mois-
ture necessary for successful germination (Nathan & Katul 2005;
Wright et al. 2008; Bohlman 2010). In this study, we investigate
the sensitivity of the seasonal dispersal kernel to varying wind dis-
tributions selected from environmental conditions and temporal
ranges associated with the dispersal season.
SEED COUNT
Ten 1-m2 seed traps were placed underneath the crowns of each of
the three L. seemannii used to determine seasonal seed release.
Our dispersal models show up to 65% and 90% of seeds released
will fall within 10 m and 30 m, respectively, from the release
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
Effects of uplift on long-distance dispersal 209
point. Therefore, we are confident our seed counts will encompass
a wide range of both short- and long-distance dispersal events. We
censused the traps at 30-min intervals from 6:00 AM to 6:00 PM
from 13 to 23 April 2010, inclusive. At each census, all traps were
emptied, and the number of L. seemannii seeds in each trap was
recorded. Total night-time seed release was documented at 6:00
AM. Night-time seed release was excluded because the exact time
of abscission during the night is not known. Just 12% of seeds
were released during the night so their exclusion did not strongly
affect our results. Counts during or immediately following rain
events (17 of 335 observations) and counts influenced by the can-
opy crane knowingly shaking branches during fruit censuses (2 of
335 observations) were also removed from the data set.
METEOROLOGICAL DATA
An 11-year data set (2000–2010) of hourly mean horizontal wind
speed and temperature at the PNM crane research facility was
acquired through the Smithsonian physical monitoring program
(http://biogeodb.stri.si.edu/physical_monitoring/). A nine-month
(February through October, 2007) data set of wind speed in three
dimensions and turbulence (wind fluctuations, frictional velocity)
above the canopy, summarized as 30-min block averaged statistics
of 10 Hz measurements, was available from BCI (Bohrer 2007)
roughly 50 km north-west of the PNM. A similar two-week data
set was collected between 12 and 26 April 2010 in the PNM.
Appendix S2 (Supporting Information) describes the methods
used to process the two 10 Hz data sets and to collect ancillary
data including air temperature, relative humidity, water vapour
pressure and incoming, outgoing and net radiation at the PNM.
EMPIR ICAL ABSC ISS ION MODEL
Seed counts were used to estimate the seasonal bias of seed abscis-
sion. We call this metric seasonally adjusted seed abscission or
DSa (see Appendix S1: Dispersal Season Determination). The sea-
sonal log-normal abscission estimate had a low correlation to
actual seed count data (r2 = 0�04), but was significant (P < 0�05).We constructed a multivariate regression model between DSa and
the observed environmental variables to determine the subseasonal
scale conditions that affect seed abscission (Table S1). All data
were averaged into 90-min bins to reduce autocorrelation and
account for potential overlap between seed counts directly before
and after their corresponding 30-min wind statistics. We followed
a stepwise procedure. At the first step, first- and second-order
polynomial regression models between DSa and each environmen-
tal variable were evaluated. We then considered the subset of
regression models that were statistically significant at the 95% CI.
Of these significant models, we selected the model with the lowest
Bayesian information criterion (BIC) value (Schwarz 1978).
To determine whether the addition of other environmental vari-
ables would lead to significant model improvement, we regressed
first- and second-order polynomials of each of the environmental
variables to the residuals of the previously selected model. Statisti-
cally significant regressions (if any) were deemed to yield signifi-
cant model improvement. Of the statistically significant
regressions (if any), we selected the one with the lowest BIC as the
new best model. This procedure was repeated until no statistically
significant regressions provided a better BIC. Although this proce-
dure assumes second-order polynomials, we found that the selec-
tion of environmental variables was insensitive to this assumption.
The goodness-of-fit of the final model was evaluated by testing the
residuals for independence (Box–Ljung test), normality (Shapiro–Wilk test) and homoscedasticity (Breusch–Pagan test). Statistical
analyses were performed using R version 2�15�1.
MODEL SELECT ION CRITER IA
A Monte Carlo study was carried out to assess the skill and
significance of the model selected. The basic protocol followed
here is similar to what was presented in Beaulieu et al. (2012)
and is designed to test for Type I and Type II errors. We
started with the null hypothesis that our best-fit model is cor-
rect. To test for Type I errors, we generated a synthetic time
series by randomly drawing (with replacement) from the residu-
als of the best-fit model and then added these random draws
to the fitted values of the best-fit model. We then applied our
fitting procedure to the synthetic time series. If our original
determination of the best-fit model is correct, then this model
should be selected to describe a strong majority of the syn-
thetic series. Our procedure for testing for Type II errors was
similar, except that this time we generated a synthetic time ser-
ies by randomly drawing (with replacement) from the residuals
of the second-best-fit model and then added these random
draws to the fitted values of the second-best-fit model. We then
applied our fitting procedure to this second synthetic series and
determined the proportion of times that our best-fit model was
selected. A small proportion would indicate that we would
rarely accept the null hypothesis when it is false. These simula-
tion schemes are appropriate because, in both the best-fit
model and the second-best-fit model, the residuals can be con-
sidered independent (Ljung-Box test, 95% confidence level). A
total number of 10,000 synthetic series were generated in the
testing of both Type I and Type II errors. In a preliminary
analysis, this number of synthetic series was found to be suffi-
cient for the results to converge.
SENSIT IV ITY ANALYS IS TO DETERMINE THE EFFECTS
OF THE T IM ING OF SEED RELEASE
Different environmental conditions lead to seed abscission at dif-
ferent times. Over the long term, these differences accumulate to
form a biased sample of the actual wind conditions. To estimate
the potential effects of seed abscission timing on the dispersal ker-
nel, we used two models forced with wind distributions derived
from long-term wind observations at BCI. These distributions are
broken into subsets based on combinations of weather and wind
conditions associated with seed abscission in the best-fit abscission
model (see Methods: Empirical abscission model). Specific wind
Fig. 1. Luehea seemannii fruit in a tropical forest. Fruit pods hold
many seeds in a start orientation, typically facing upward (above
the horizontal). Cracks in the distal end of the pod widen during
the season allowing the seeds to be released.
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
210 K. D. Maurer et al.
distributions and inclusion of abscission biases in either model are
later described in the individual model methods. We use these sim-
ulations to estimate the sensitivity of the dispersal kernel (particu-
larly the mean distance and LDD probability) to the
environmental conditions affecting the timing of seed release. The
resulting kernels are not evaluated for the specific dispersal dis-
tances and probability. Instead, each kernel is compared relative
to the others and relative to a bench-mark case of unbiased, uni-
form-in-time release rate to quantify the relative long-term effects
of the bias in wind conditions due to the selective timing of seed
release under different environmental conditions.
MODELL ING LONG-TERM EFFECTS OF
ENV IRONMENTALLY TR IGGERED ABSC ISS ION – THE
SUPER-WALD KERNEL
A good approximation of the dispersal kernel for slow-falling
seeds in turbulent environments can be calculated with the WALD
phenomenological kernel (Katul et al. 2005):
W xð Þ ¼ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
z2r4phjHx3
rexp �
V2t x� zru
Vt
� �2
4jhH uð Þ2x
0B@
1CA
264
375 eqn 1
where W xð Þ is the probability of landing at a distance x (m)
from the source, zr is the height (m) above ground at which
seeds were released from the mother plant, h is the mean
height (m) of the top of the surrounding canopy, Θ is a scal-
ing coefficient for turbulence defined as the ratio between the
standard deviation of the 10 Hz measurements over a 30-min
period of vertical wind fluctuation, rwðms�1Þ, and the mean
wind speed above the canopy, uðms�1Þ; thatis;H ¼ rw=u. Long-
term Θ is determined from the slope of the correlation between
rw and u over the data set of high-frequency wind observations.
The similarity constant, j, is assumed to be 0�6 for within-can-
opy flow conditions (Thompson & Katul 2008), and Vt is the
terminal fall velocity of the seed (m s�1). Here, we used
Vt = 0�7 � 0�07 m s�1, determined from the mean of measure-
ments of 15 seeds (Augspurger 1986). The WALD kernel
describes the distribution of dispersal distances in a given set
of wind conditions, typical of a specific 30-min period.
Thompson & Katul (2008) showed that WALD can be
expanded to represent the expected long-term dispersal kernel,
obtained as the convolution of many 30-min dispersal kernels, if
the long-term distribution of the wind is known and assumed to
fit a Weibull. A more accurate representation of the long-term
wind distribution may be obtained through explicit integration of
individual 30-min measurements over the entire period (following
the approach in Wright et al.2008). The seasonally integrated
super-WALD (SW) kernel will then follow the formulation of
SW xð Þ ¼ 1
t
Zt
W ut; xð Þdt eqn 2
where W ut; xð Þ is the WALD kernel (as a function of distance, x)
for the observed 30-min mean wind conditions at a particular time
ut (described in eqn 1). As super-WALD does not account for the
variation of wind speed with height above the canopy, we assume
the wind speed at a height of 5 m above the canopy as the effec-
tive wind speed. Super-WALD kernels were calculated using the
statistics of the 30-min mean horizontal wind at PNM for the fol-
lowing scenarios: (1) full year of uniform seed release rate; (2) dis-
persal only during the observed dispersal season (sub-sampling of
meteorological data was done following Garrity et al. 2011); (3)
dispersal during the dispersal season only during daytime hours
(6:00 AM to 6:00 PM); (4) a subset of (3) but only during strong
horizontal winds, that is, u > 0�5 m s�1 and (5) a subset of (3) but
only in relatively high (above median) temperatures, that is,
T > T50. The super-WALD kernel does not incorporate updrafts;
therefore, we include higher horizontal winds, which typically lead
to higher turbulence (i.e. more updrafts/downdrafts). We recalcu-
lated Θ based on the subset of wind observations that comply with
the conditions of each case and then recalculated the dispersal ker-
nel that corresponds with the appropriate release timing using
eqns 1 and 2. The 11-year distributions of wind speed for all cases
are presented in Figure S4. Figure S5 presents the day and night
distributions of turbulence statistics (frictional velocity and verti-
cal wind fluctuation inside the canopy) for 12–26 April 2010.
EFFECTS OF ABSC ISS ION IN UPDRAFTS
Updrafts are a short-term process and are part of the turbulent
fluctuations of vertical wind, which averages to near zero at the
30-min and longer time-scales. The coupled Eulerian–Lagrangianclosure (CELC) model (Nathan & Katul 2005) is able to simulate
turbulence by calculating random instantaneous (milliseconds–sec-onds) turbulent-driven excursions from a prescribed wind speed
field and calculate the resulting three-dimensional trajectories of
wind-dispersed seeds. In CELC, the prescribed horizontal wind
speed field is homogeneous but includes a vertical profile – weaker
wind inside the canopy and near the ground following Massman
& Weil (1999) and logarithmically increasing wind speed above
the canopy, following the Monin–Obukhov similarity theory. Sim-
ilar variation is prescribed for the turbulence statistics. The trajec-
tory calculations are repeated for many virtual seeds to produce
the large sample necessary to calculate a representative dispersal
kernel for the prescribed, half-hourly wind conditions. Repeated
CELC simulations with different sets of prescribed, observation-
based, above-canopy, half-hourly wind conditions are combined
to form an overall seasonal kernel. In this way, the resulting ker-
nel accounts for both short-term turbulence, through the effects
on the trajectories of individual seeds, and longer-term wind con-
ditions, through the combined sets of prescribed 30-min condi-
tions. We used the same CELC set-up as reported in Wright et al.
(2008). The fact that CELC utilizes both a turbulent time-scale
(during the dispersal events) and a longer time-scale (by repeated
simulations with different 30-min forcing) limit the negative effects
of time-scale choice on the estimate of the kernel (Skarpaas, Shea
& Jongejans 2011).
Inputs for CELC included the leaf drag coefficient (estimated
here as 0�25) and the half-hourly wind and turbulence statistics
above the canopy on BCI during a full dispersal season in 2007
(Bohrer 2007). Release height was assumed to be 40 m, corre-
sponding to the canopy height at BCI, where we have season-long
high-frequency measurements of wind and turbulence. Canopy
structure representation in CELC is reduced to the description of
the horizontally averaged vertical profile of leaf area density pro-
vided by Bohlman & O’Brien (2006) for BCI. Terminal velocity
for each dispersal event was randomly selected from a Gaussian
distribution, with the reported mean and standard deviation for
L. seemannii. To reduce the 2-D dispersal distribution to a 1-D
distance kernel, we converted the 2-D space to annuli centred on
the release point. The number of seeds that arrived in each dis-
tance bin were summed and then normalized by bin width and the
total number of seeds released (during the entire seasonal series of
simulations), resulting in the probability a seed fell in each dis-
tance bin. We ignore dispersal distances � 100 km, as these were
typically caused by seeds ‘caught’ at the numeric top boundary of
the model, causing unrealistically long dispersal distances due to
numerical limitations.
To directly test the effects of release in updrafts, we ran two ser-
ies of simulations with CELC: (i) bench-mark case – used to simu-
late the dispersal kernel when seed abscission rate is not affected
by updraft; (ii) updraft-biased case in which the seed is initially
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
Effects of uplift on long-distance dispersal 211
caught in an upward eddy for a period of one eddy correlation
time (calculated using formulation from Nathan & Katul (2005)).
This biased case is used to simulate abscission that is induced by
an updraft event at some point during the prescribed 30-min per-
iod. The initial vertical wind speed for each 30-min period is pre-
scribed as the median updraft velocity (i.e. the 75th percentile of
the vertical wind distribution, which includes roughly 50% up-
drafts and 50% downdrafts) assuming vertical velocity has a
Gaussian distribution with mean 0 and the observed standard
deviation, rW. This vertical eddy velocity is representative of a
typical updraft for the wind conditions during each specific half
hour and may or may not be larger than the terminal velocity of
the seed. After the initial eddy correlation time period, the seed is
allowed to experience the same wind statistics as in the bench-
mark case, driven by the observed 30-min mean and turbulence
statistics.
Results
OBSERVAT IONS : SEED ABSC ISS ION IS DETERMINED
BY METEOROLOGICAL CONDIT IONS
Seed abscission is intermittent, as can be seen by the
large deviations from predicted seasonal distribution of
seed release (DSa, Fig. S3). The majority of seeds were
released during a few large events. Over 158 half-hour
periods, we found all meteorological variables to be
significantly directly correlated with the rate of seed
abscission, with the exception of u. Because most
environmental variables were intercorrelated (Table S2),
it is not surprising that many variables show significant
effects. The variable with the highest predictive power of
seed abscission was the root mean square of the upward
wind perturbations, rWup (r2adj = 0�490, P < 0�001), whichindicates that updrafts have the strongest effect of any
environmental variable on seed abscission in L. seemannii.
In the subsequent steps of the regression analysis, the
sensible heat flux (H), temperature (T) and mean horizon-
tal wind speed (�u) also significantly affected abscission, but
the addition of further environmental variables did not
significantly improve the fit. Null hypotheses of indepen-
dence and homoscedasticity were not rejected (P = 0�72and P = 0�62, respectively). However, the residuals were
not normally distributed (P < 0�001). While non-normality
can in principle introduce biases, our parameter estimates
from ordinary least-squares were consistent with the
results of a robust regression. The seed abscission model
resulting from the stepwise procedure (r2adj = 0�714,P < 0�001) follows:DSa ¼ 1700r2Wup � 580rWup � 1040H2 þ 3�6T� 44u2 þ 45u
� 63
eqn 3
We used Markov Chain Monte Carlo analysis to test
the significance of adding each of the above model vari-
ables. rWup was selected as the first predictor variable in a
strong majority (89%) of the cases (Fig. S6a). Wmax was
selected as the first predictor variable in almost all of the
remaining cases. Thus, if our best-fit model accurately
describes the data, then rWup would be correctly identified
as the most important predictor variable with 89% proba-
bility. The probability that H was chosen as the second
predictor variable, conditional on rWup being previously
chosen, was 73% of cases (Fig. S6b). Similarly, probability
of choosing T as the third variable conditional on have
previously chosen rWup and H was 76% (Fig. S6c), and
the probability of choosing �u as the fourth variable condi-
tional on having previously chosen rWup, H and T was
74% (Fig. S6d). If �u was not chosen in the fourth step, the
next most likely outcome (23%) was that no model gave a
statistically significant improvement to the fit. Overall, the
independent variables of the best-fit model were chosen in
37% of the synthetic series. Because of the relatively low
proportion of cases for which �u was chosen, including it as
a predictor variable should be regarded as speculative. In
our analysis of Type II error, we found that the second-
best-fit model consisting of rWup, H and T was selected in
56% of the series. The best fit was (spuriously) selected
2% of the time, indicating relatively low probability of
incorrectly accepting the null hypothesis. Following the
results from the Monte Carlo study, the most significant
model (evaluated in Fig. 2) (r2adj = 0�646, P < 0�001)follows:
DSa ¼ 1700r2Wup � 600rWup � 1130H2 þ 3�3T� 43 eqn 4
This model was selected as the final abscission model,
which describes positive feedback towards abscission
during periods of updrafts and high temperature and a
negative feedback towards abscission during temperature-
driven highly convective periods. Coefficients to the model
correspond to a 30-min estimate of seed abscission.
MODELL ING: INTEGRAT ING ABSC ISS ION CONDIT IONS
TO PREDICT LONG-TERM DISPERSAL KERNELS
We created dispersal kernels using the super-WALD
model, with 11-year wind data from PNM and
−10 0 10 20 30 40 50 60
−10
0
10
20
30
40
50
60
Measured ΔSa
Mo
del
ed Δ
Sa
Fig. 2. Modeled abscission vs. measured abscission (eqn 4,
r2 = 0.646, P < 0.001). Solid line is the 1 : 1 line.
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
212 K. D. Maurer et al.
corresponding 11-year dispersal season–timing observa-
tions from BCI. The results show that kernels representing
cases 1–3 have very similar shapes (Fig. 3). The strong
wind conditions (case 4) show the highest probability of
dispersing between 20–255 m. From 255–4988 m, the high
temperature conditions (case 5) show the highest probabil-
ity, with yearly conditions (case 1) having the highest
probability of distances further than 4988 m. The dispersal
probabilities near these transitions are on the order of
10�4–10�7; however, we show for each case that roughly
1% of the seed population will travel at least 1 km and
0�1% of the seed population will travel multiple km. For
the yearly conditions, the 99�9% cumulative threshold was
not reached in the maximum search area of this study
(25 km). Although the strong wind kernel becomes less
probable than the yearly and daytime dispersal season ker-
nels, the mean dispersal distance under strong wind condi-
tions (91 m) is further than the means of the yearly,
seasonal and daytime, seasonal conditions (67, 63 and
84 m, respectively). The high-temperature kernel has the
furthest mean dispersal distance at 105 m.
MODELL ING: DETERMIN ING THE EFFECTS OF
ABSC ISS ION IN UPDRAFTS
Dispersal kernels were calculated by the CELC model
using two cases: one with an updraft bias and the other,
a control with no bias for updraft-driven seed abscission.
Dispersal distance is consistent between each case up to
roughly 100 m, as can be seen by the equivalent distance
travelled by the first cumulative 99% of seeds. At dis-
tances further than 100 m, we find a shift to higher dis-
persal distance probability in the updraft-biased scenario
relative to the control scenario (Fig. 4). At the cumula-
tive 99�9% seed population threshold, the control case
sees dispersal distances of 364 m, compared to distances
of 840 m (2�3 times as far). This roughly 2 : 1 dispersal
distance ratio of the updraft case vs. the control case
continues for the duration of the seed population, and
the difference in probability of LDD of the updraft case
becomes as large as an order of magnitude more than
the control case for dispersal distances larger than
10 km. Although this distance corresponds to a probabil-
ity on the order of 10�5–10�6, integration of the kernel
shows roughly 0�01% of the seed population will travel
further than 10 km. The mean dispersal distance during
the updraft case is 28% further than the mean dispersal
distance during the control case.
Discussion
Dispersal is a very short-term event (seconds–minutes)
which, aggregated over many events over days and sea-
sons, controls the slow, long-term dynamics (years – mil-
lennia) of population spread and survival. Therefore, we
hypothesize that the physiological traits that control the
timing of seed release should be selected to respond to
environmental conditions in a way that will optimize the
resulting dispersal. The species we studied, L. seemannii, is
shade-intolerant and depends on germination in canopy
gaps, which are rare in its closed canopy forest habitat.
These establishment limitations suggest L. seemannii
would benefit from LDD, which provides a large ‘search
area’. Selection should favour morphological traits that
promote LDD in this tree. The dispersal unit morphology
(light weight, thin ‘wings’, upward-facing capsule) suggests
10–1
10–2
10–3
10–4
10–5
10–6
10–7
10–8
100 101 102 103 104
Dispersal Distance [m]
pd
f
99%
99·9%
YearSeasonSeason (Daytime)Season (Daytime, u >0·5)Season (Daytime, T >T50)
Fig. 3. Super-WALD dispersal kernels presented as the probabil-
ity seeds disperse a given distance under five sets of environmental
conditions. The inset provides a key to the environmental condi-
tions. Both the probability of seed arrival and distance are on log-
arithmic scales. Vertical lines correspond to the distance to which
the listed percentage of seeds have traveled.
Dispersal Distance [m]
pd
f
99%
99·9%
UpdraftControl
10–1
10–2
10–3
10–4
10–5
10–6
10–7
100 101 102 103 105104
Fig. 4. The coupled Eulerian–Lagrangian closure (CELC) dis-
persal kernels presented as the probability seeds disperse a given
distance under two sets of environmental conditions. The inset
provides a key to the environmental conditions. Both the proba-
bility of seed arrival and distance are on logarithmic scales. Verti-
cal lines correspond to the distance to which the listed percentage
of seeds have traveled.
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
Effects of uplift on long-distance dispersal 213
that selection for LDD has affected the seed traits to
increase their flight time and dispersal distance. The mean
dispersal distance may also be affected by long-term
(multi-annual) interactions between population viability,
seedling survival, habitat and climate (Kuparinen et al.
2009; Nathan et al. 2011). However, in this study, we focus
on subannual time-scales. We use super-WALD kernels to
test the effects of environmental variables such as wind
speed and the seasonal and diurnal distributions of the
wind and CELC to test the effects of seed release in
updraft conditions.
EFFECTS OF THE T IM ING OF THE DISPERSAL SEASON
The year-round super-WALD kernel (case 1) had the high-
est probability of dispersing further than 4 km and the
highest mean long dispersal distance for the farthest 0�1%of seeds (Fig 3). However, the mean dispersal distance is
higher during seasonal daytime conditions (84 m) (case 3)
compared to the year-round (67 m) and dispersal season
(63 m) conditions. While the mean wind speed (�u) for the
seasonal daytime case is higher than both the seasonal and
year-round cases (Fig. S4), the year-round wind speed dis-
tribution shows a thicker tail, indicating more frequent
events of relatively strong wind. This is due to the fact that
there are more extreme turbulent wind gusts during the
wet season than during the dry season, as indicated by the
wind speed skewness and kurtosis (Table S3). Nonetheless,
our study species, and most other wind-dispersed species
in central Panama, disperse their seeds during the dry sea-
son. These findings suggest that the timing of the dispersal
season is not driven only by consideration of dispersal dis-
tance and that other factors, such as the impending rains
that favour germination and seedling establishment, may
also lead to selective forces that determine the timing of
the dispersal season.
In our simulations, we neglect the effects of spatial het-
erogeneity and the seasonality of canopy structure. It is
probable that the effects of reduced canopy density during
the dry season play an important role. During the dispersal
season, canopy density is at its minimum, which improves
dispersal distance (Nathan & Katul 2005), and the canopy
is rich with temporary gaps caused by leafless deciduous
trees surrounded by evergreen trees (Bohlman 2010), which
leads to ejection hotspots and increased LDD probability
(Bohrer et al. 2008, 2009). These effects cannot be resolved
by either the super-WALD or the CELC models as they
are driven by the spatial interaction between canopy heter-
ogeneity and turbulence. Due to these model limitations,
we cannot rule out wind as a selective driver of the timing
of the dispersal season.
EFFECTS OF DAYT IME RELEASE
As seen in our seed trap data, daytime abscission was
roughly an order of magnitude greater than night-time
abscission. Wind conditions at night tend to be weaker
than those during the day. During the strongly convective
tropical periods, daytime means of u = 0�540 m s�1,
u* = 0�280 m s�1 and rWup = 0�223 m s�1 were much lar-
ger than night-time means of u = 0�334 m s�1, u* =0�168 m s�1 and rWup = 0�158 m s�1 (Fig. S5). The day-
time vertical wind is more negatively skewed (�0�518 m
s�1) than night-time vertical wind (�0�437 m s�1), dem-
onstrating a thicker above-mean tail and higher tendency
for updrafts. These statistics, and correspondingly, our
simulation results, suggest that seeds will have higher
chances to uplift and experience LDD with the strongly
convective conditions during the day rather than during
the night.
EFFECT OF SEED ABSC ISS ION AT H IGH WIND SPEED
AND HIGH TEMPERATURE
It is interesting to note that heat flux and temperature,
which have been shown to influence seed abscission in pre-
vious studies in the same tropical environment but for a
different species, Jacaranda copaia, which disperses during
the wet season (Wright et al. 2008), were also found to sig-
nificantly influence the high-frequency seed release timing
of L. seemannii, which disperses during the dry season.
Previous studies demonstrated that drying of the dispersal
unit increases seed abscission (Greene & Johnson 1992;
Jongejans et al. 2007). It is possible that temperature pro-
vides the mechanism for the daytime release through the
drying and opening of the pod. Both temperature and
humidity have a significant positive effect on abscission;
however, the strong correlation between temperature and
humidity led to humidity not having a significant indepen-
dent effect on abscission.
Strong wind (red line, Fig. 3) and high temperature
(cyan line, Fig. 3) show enhanced dispersal probabilities
at moderate distances (100–5000 m) compared to yearly,
seasonal and seasonal daytime cases. LDD at strong
wind becomes less probable around the 99th percentile
(~1 km) of seeds released, whereas high-temperature LDD
becomes less probable around the 99�9th percentile (few
km). We found the ratio between vertical wind fluctua-
tions and mean horizontal wind speed, Θ, to be the rea-
son for the observed differences between the shape of the
dispersal kernel with strong wind and other seasonal ker-
nels. At our site and typical of other tropical sites, low
values of u are characteristic of weather conditions with
high thermally driven turbulence and therefore high Θ.
This occurs because strong wind produces more shear-
driven eddies that tend to be smaller and less energetic
than thermally driven eddies. Θ shows a twofold reduc-
tion when wind is subsampled from u > 0�5 m s�1com-
pared to the year-round and daytime dispersal season
and high temperature winds (0�59, 1�31, 1�25 and 1�18,respectively). Combined, higher u and lower Θ create
large effects on the shape of the dispersal kernel, particu-
larly, increasing the mean dispersal distance while
reducing the probability of LDD.
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
214 K. D. Maurer et al.
Table
1.Summary
ofthestatisticsfrom
thestepwiseem
piricalmodel
selectionforseed
abscission,expressed
astheresidualfrom
theexpectedseasonalseed
availabilityrate,DSa
Model:DSa=
Environmentalvariable
(x)andMonte
Carloparameter
index
BIC
TRH
W95
Wmax
Wmin
r Wr W
up
uu*
gust
rU
HSWnet
VPD
ZE
12
34
56
78
910
11
12
13
14
15
Ax+B
0.268
0.222
0.302
0.343
0.251
0.241
0.388
�0.019
0.147
0.235
0.182
0.031
0.107
0.255
0.073
–Ax2+B
0.277
0.210
0.324
0.388
0.269
0.239
0.443
�0.020
0.110
0.228
0.158
�0.012
0.048
0.291
0.066
–Ax2+Bx+C
0.318
0.243
0.318
0.401
0.258
0.226
0.490
0.021
0.178
0.219
0.197
0.094
0.165
0.279
0.054
391.7
Ar W
up2+Br W
up+Cx+D
0.509
0.491
0.533
0.480
0.480
0.517
0.519
0.514
0.488
0.501
0.544
0.480
0.498
0.483
–Ar W
up2+Br W
up+Cx2+D
0.510
0.489
0.551
0.480
0.483
0.534
0.539
0.535
0.493
0.519
0.579
0.484
0.512
0.481
372.2
Ar W
up2+Br W
up+Cx2+Dx+E
0.512
0.496
0.581
0.487
0.490
0.559
0.558
0.551
0.492
0.574
0.573
0.520
0.512
0.477
–Ar W
up2+Br W
up+CH
2+Dx+E
0.646
0.637
0.571
0.571
0.578
0.570
0.580
0.570
0.570
0.570
0.575
0.653
0.588
364.8
Ar W
up2+Br W
up+CH
2+Dx2+E
0.650
0.629
0.574
0.570
0.577
0.570
0.595
0.572
0.570
0.571
0.570
0.678
0.585
–Ar W
up2+Br W
up+CH
2+Dx2+Ex
+F
0.660
0.659
0.590
0.569
0.568
0.575
0.638
0.578
0.567
0.605
0.594
0.672
0.581
–Ar W
up2+Br W
up+CH
2+DT+Ex
+F
0.642
0.639
0.639
0.652
0.638
0.674
0.646
0.638
0.643
0.644
0.650
0.639
–.Ar W
up2+Br W
up+CH
2+DT
+Ex2+F
0.640
0.640
0.639
0.650
0.639
0.694
0.650
0.639
0.648
0.646
0.672
0.641
–Ar W
up2+Br W
up+CH
2+DT
+Ex2+Fx+G
0.668
0.640
0.631
0.646
0.639
0.714
0.645
0.634
0.655
0.640
0.675
0.635
347.6
Ar W
up2+Br W
up+CH
2+DT
+Eu
2+Fu+Gx+H
0.713
0.709
0.711
0.711
0.707
0.707
0.710
0.713
0.708
0.720
0.708
–Ar W
up2+Br W
up+CH
2+DT
+Eu
2+Fu+Gx2+H
0.710
0.710
0.711
0.710
0.707
0.707
0.709
0.711
0.709
0.738
0.710
–Ar W
up2+Br W
up+CH
2+DT
+Eu
2+Fu+Gx2+Hx+I
0.732
0.702
0.704
0.708
0.701
0.701
0.705
0.708
0.703
0.736
0.709
–
Thetable
showsther2
oflinear,
quadraticandsecond-order
polynomialregressionbetweendifferentcombinationsofenvironmentalvariables,
x,andDSa.Ateach
iteration,thevariable
withthe
highestr2
(highlightedbold)amongthose
withasignificantrelationship
wasadded
tothemodel.Thetypeofrelationship
forthisvariable
(linear,quadratic)
wasalsodetermined
accordingto
the
highestr2.Bayesianinform
ationcriterion(BIC
)analysiswasusedto
determinewhether
addingthisvariable
tothemodel
isjustified.In
each
iteration,thelowestmodel
BIC
valueisshownonthe
last
column.BIC
values
ofthelast
iterationare
leftblank,asnoBIC
waslower
thanthatofthepreviousiteration.Thesignificance
oftheim
provem
entto
themodel
incomparisonwiththesimpler
modelfrom
thepreviousiterationwastested
usingaMarkovChain
Monte
Carloanalysis(Figure
S6).
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
Effects of uplift on long-distance dispersal 215
EFFECTS OF ABSC ISS ION IN UPDRAFTS
Long-distance dispersal of wind-dispersed seeds in forests
is dependent on ejection of the seeds above the canopy
(Nathan et al. 2002; Bohrer et al. 2008). During its dis-
persal event, a seed spends a few seconds to minutes in
the air, held up by turbulent eddies that produce updrafts
that are faster than its terminal fall velocity. As the long-
term mean vertical wind is near zero, short-term turbulent
fluctuations are the major source of uplift. While at a
longer time-scale turbulence is a chaotic process, at short
time-scales turbulent motion is characterized by organized
waves – eddies. If a seed can time its release to co-occur
with the passage of an upward eddy (ejection), it can
‘ride’ this eddy for a short period before the eddy breaks
and dissipates. The average time for eddy dissipation is
the eddy dissipation time, which we used in the CELC
model. This short period (few seconds) of upward motion
may be long enough and the updraft strong enough for
the seed to be ejected above the canopy and into the
stronger horizontal winds aloft that can carry seeds long
distances.
The CELC model simulation confirmed that updraft-
targeted seed release generates a higher probability of
LDD. Dispersal events will only be meaningful when
leading to seedling establishment, which in most instances
involved LDD to escape predation and/or find suitable
habitat (Thompson et al. 2009). Yearly seedling establish-
ment events may occur at dispersal probabilities as low as
10�10 (Nathan 2006), which demonstrates our large LDD
advantage during updraft conditions at probabilities of
10�5–10�6 to be significant. Furthermore, from seed
counts per individual fruit (385 � 53, n = 18) and on the
order of 103 fruit per tree, we estimate the total annual
seed production per individual to be on the order of 105–
106 seeds, and roughly 107–109 during each tree’s lifetime.
By factoring these magnitudes into our calculated dis-
persal kernels, we show that when released in an updraft
hundreds of seeds per individual per dispersal season (and
tens-hundreds of thousands in a lifetime) will travel more
than 1 km farther than seeds whose release does not
target updrafts.
The idea that ejections (updrafts) enhance dispersal dis-
tances may seem intuitive, yet it has seldom been directly
modelled or measured. Nathan et al. (2002) used the
CELC model to show that ejected seeds would have a
large LDD advantage over those seeds not ejected from
the canopy. Our CELC simulation is the first to compare
dispersal distance of seeds that were released uniformly
without respect to updrafts with seeds released preferen-
tially in updraft conditions. Although updraft bias may
play an important role in both abscission timing and dis-
persal distance, it remains difficult to incorporate into
dispersal kernel models. The problem arises because tar-
geted abscission and turbulent momentum ejections are
coupled phenomena that operate at very short time-
scales. Timing the release to favour LDD is only possible
if short-term high-frequency information is used. The
challenge for the plant is to detect these conditions and
target the release of seeds to these turbulence ejection
events. In the case of wind-dispersed seeds, a closer
inspection of the dispersal unit may resolve the link
between morphology and LDD.
Greene & Johnson (1992) showed that drag from hori-
zontal wind (induced with a household fan) affected the
rate of seed abscission in a maple tree and that the shape
of the maple seed wings and detachment mechanisms inter-
acted with the wind direction such that under updrafts the
seeds deflected at a larger angle which increased their
probability of detachment of the peduncle. In a wind-tun-
nel experiment, Greene & Quesada (2011) showed that the
shape of the capitulum of T. dubius suppresses seed release
in downdrafts and therefore provides a morphological
mechanism for updraft-selective release. Our study is the
first to observe this updraft bias phenomenon in a natural
environment and a tropical tree. The fruits of L. seemannii
have an upward-facing cone that opens narrow cracks that
begin at its top end (Fig. 1). Bernoulli’s equation along a
vertical streamline starting from the seed location and
extending outward through the pod crack describe the
physical mechanism through which the seed pod orienta-
tion interacts with updrafts to generate lee-side wake vorti-
ces that create a pressure gradient strong enough to
dislodge the seeds.
Conclusions
To correctly estimate the movement capability of dispers-
ing seeds, the full range of time-scales of the signal that
drives seed release in plants must be represented by the
modelling methods used to predict dispersal kernels.
Super-WALD kernels that were generated with long-term
wind observations, subselected for particular seed release
dynamics, showed that the timing of the dispersal season
does not necessarily optimize dispersal distance. At shorter
time-scales, preferential dispersal timing during the day-
time with frequent updrafts increased dispersal distances
and LDD. Mechanistic dispersal simulations showed that
including an updraft bias to the abscission conditions
would further increase the probability of LDD.
Our finding of preferential abscission during updrafts is
consistent with recent hypotheses, model simulations and
laboratory experiments (Tackenberg, Poschlod & Kahmen
2003; Bohrer et al. 2008; Soons & Bullock 2008; Greene &
Quesada 2011). To date, this study and those of Greene &
Johnson (1992) and Greene & Quesada (2011) are the only
ones that report cases of morphological mechanisms for
upward-directional abscission bias. This research high-
lights the need to further investigate the mechanisms of
seed abscission in wind-dispersed plants. Specifically, we
suspect that further inspection of the morphology of their
specialized dispersal units will show how this has evolved
in many species to select release events during environmen-
tal conditions that will lead to optimal LDD.
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
216 K. D. Maurer et al.
Acknowledgements
We thank Ran Nathan for early discussion that helped inspire this
study. We thank Mirna Samaniego for data collection assistance. KM
was supported by the Smithsonian Tropical Research Institute (STRI), a
French Graduate Fellowship through the Department of Civil, Environ-
mental & Geodetic Engineering, an Ohio State University Fellowship
and an NSF IGERT Fellowship #DGE-0504552 awarded through the
University of Michigan Biosphere-Atmosphere Research Training
(BART) program. GB was supported by NSF grant #DEB-0918869.
Any opinions, findings and conclusions expressed in this material are
those of the authors and do not necessarily reflect the views of the
National Science Foundation.
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Received 20 June 2012; accepted 17 October 2012
Handling Editor: Ken Thompson
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
Effects of uplift on long-distance dispersal 217
Supporting Information
Additional Supporting Information may be found in the online
version of this article:
Appendix S1. Dispersal Season Determination.
Appendix S2. Meteorology.
Table S1. Environmental Variables.
Table S2. Environmental Correlations.
Table S3. Super-WALD Inputs.
Fig. S1. BCI Seed Trap Data.
Fig. S2. PNM Dispersal Estimates.
Fig. S3. PNM DSa.Fig. S4. Conditional Wind Distributions.
Fig. S5. Day–Night Wind Statistics.
Fig. S6. Monte Carlo Results.
© 2012 The Authors. Functional Ecology © 2012 British Ecological Society, Functional Ecology, 27, 208–218
218 K. D. Maurer et al.