Journal of Experimental Botany, Vol. 48, No. 310, pp. 1133-1142, May 1997
Journal of
Experimental
Botany
Trace gas exchange over terrestrial ecosystems:
methods and perspectives in micrometeorology
John Moncrieff1'5, Riccardo Valentini2, Susanna Greco2, Guenther Seufert3 and Paolo Ciccioli4
1
1nstitute of Ecology and Resource Management, The University of Edinburgh, Mayfield Road, Edinburgh
EH93JU, UK
2
University of Tuscia, Dipartimento di Scienze dell'Ambiente Forestale e delle sue Risorse (Di.S.A.F.Ri), Viterbo,
Italy
3
Commission of the European Communities, Joint Research Centre (JRC), Environment Institute, Ispra (VA),
Italy
CNR-lnstitute of Atmospheric Pollution, Montelibretti, Italy
Received 15 February 1997; Accepted 25 February 1997
Provided by the author for non-commercial research and education use. Not for reproduction, distribution or commercial use
Abstract
Quantification of the surface-atmosphere exchange of
trace gases is recognized as an essential prerequisite
to understanding the role of the biosphere in the global
climate system. Among the micrometeorological
methods available to measure surface-atmosphere
fluxes, the aerodynamic gradient, the energy
balance/Bowen ratio, the eddy covariance and the
eddy accumulation methods are the most widely
employed. This brief review describes the theoretical
background and the practical applications of these
methodologies and is particularly directed to plant
ecophysiologists, ecologists and botanists who may be
interested in scaling biological processes to the
canopy level.
Key words: Trace gas exchange, biosphere, surface-atmosphere fluxes, aerodynamic gradient, Bowen ratio, eddy
covariance, eddy accumulation, micrometeorology.
Introduction
The major biogeochemical cycles on Earth play an important role in the climate system and the role of vegetation
in the cycling of carbon, nitrogen and water, at a range
of scales, is an area of major research interest. The
unresolved budget for global carbon and the location of
the 'missing sink' for carbon is a prime example of the
progress which needs to be made (Schimel, 1995).
!
Similarly, the emission of volatile organic compounds
such as the monoterpenes, isoprene etc., which are linked
to plant metabolism and photosynthesis, needs to be
investigated at the canopy scale to improve our understanding of the potential role of these substances on
tropospheric ozone formation. Scaling the functional processes of plants, from cells and organs to communities, is
important if such biosphere-atmosphere interaction is to
be understood and a quantification of trace gas exchange
is essential to validate models at regional and global scale.
Using micrometeorological methods to investigate the
surface-atmosphere exchange of trace gases is valuable
in that they produce fluxes which are integrated over a
relatively large area (typically a few km2). The methods
are also non-destructive and the results can be used as
independent tests of process-based models (Baldocchi
et al., 1988). Many reviews have been published on
micrometeorological methods in the past (Fowler and
Duyzer, 1989; Verma, 1990; Lenschow, 1995), but the
pace of change, particularly brought about by developments in available technology, means that scientists not
working directly in this field, need to be brought up-todate regularly. In addition, a number of recent papers
have clarified methodological issues such as, what is an
appropriate sampling period?; at what height should
measurements be made?; and how much 'fetch' is enough?
(Horst and Weil, 1994; Lenshow et al., 1994). This paper
is neither a comprehensive review of all aspects related
to measurements of gaseous exchange nor a full list of
the techniques available today, but will address the most
To whom correspondence should be addressed: Fax: +44 131 662 0478. E-mail: j.moncneff©ed.ac.uk.
© Oxford University Press 1997
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4
1134 Moncrieff
relevant topics which may be used by plant ecologists,
botanists and ecophysiologists interested in scaling biological processes to canopy level. Most attention will be
focused on the developments and opportunities provided
by the direct measuring techniques of eddy covariance
and eddy accumulation.
The scope of micrometeorology
Micrometeorological methods
In essence, micrometeorological methods used to quantify
turbulent exchange fall into two categories. There are
direct methods which sample the air as it flows past a
sampling point for its vertical wind speed and direction
and its gas concentration (the eddy covariance or eddy
accumulation methods) or there are indirect methods
based on quantifying the rate of diffusion down a concen-
Methods based on concepts of turbulent diffusion
Aerodynamic technique: In this method, the transport
process is described in a flux-gradient format and one
which defines the constant of proportionality K, known
as an eddy diffusivity. Thus, the flux, Fx of a trace gas
with concentration x, in this form would be:
The exchange coefficient (Kx) is obtained by invoking a
principle of similarity which says that all scalars (heat,
mass) are transported equally effectively, and, once the
exchange coefficient for one is found, the rest are equal.
In practice, the exchange coefficient for momentum is
obtained by anemometry and, via a series of empirically
determined steps, the exchange coefficient for the species
of interest is obtained. The method has been described
fully in Thorn (1975) and Monteith and Unsworth (1990).
Fowler and Unsworth (1979) showed how the method
could be used to measure fluxes of sulphur dioxide to a
cereal crop. Sutton et al. (1993) show the steps involved
in calculating fluxes of ammonia using this method,
including allowing for the influence of atmospheric
stability. In general, the method is difficult to apply when
gradients are small, as they often are near to the canopy
in tall, rough vegetation such as forests and it cannot
easily be used within the roughness sub-layer. It cannot
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Micrometeorology is the study of the interaction of the
lower atmosphere with the surface of Earth and, in effect,
it deals with the exchange processes of radiation, mass
and momentum which dictate the behaviour of much of
what is regarded as weather. Just as micrometeorology is
the study of the interface between the atmosphere and
the surface, so micrometeorology can be regarded as an
interface between the academic subjects of biology and
physics (at least fluid dynamics). The atmospheric boundary layer most frequently examined in traditional groundor tower-based micrometeorology is called the surface
layer and is usually about 10% the depth of the
Atmospheric Boundary Layer (itself denned by Lenschow
(1995) as 'the lower part of the atmosphere that interacts
with the biosphere and is closely coupled to the surface
by turbulent exchange processes'). In the surface layer,
fluxes remain within about 10% of their surface value and
it is a region where the influence of the coriolis force can
be considered negligible. Within the surface layer, two
sub-layers can be defined. The roughness sub-layer is a
region in which the vegetation elements directly influence
the nature of atmospheric turbulence through phenomena
such as wake turbulence or thermals which augment and
enhance turbulent exchange (Raupach and Thorn, 1981).
The depth of the roughness sub-layer can be difficult to
estimate, for example, it may extend up to a height of
about 3>hc where hc is the height of the canopy (Kaimal
and Finnegan, 1994) or its depth may be defined as being
within about three times the spacing of the horizontal
elements of the canopy (Lenschow, 1995). The layer
above the roughness sub-layer is known as the inertia!
sub-layer in which fluxes are more or less constant with
height and in neutral conditions the wind profile is
logarithmic with height (Thorn, 1975). Not all micrometeorological methods are appropriate in all these layers,
nor within plant canopies as will be discussed.
tration gradient (the aerodynamic and Bowen ratio
methods). Each method has distinct advantages and
disadvantages and all have been well validated over the
course of the past three decades. The direct methods
involve sampling at one height only, but with relatively
sophisticated sensors and logging equipment. The
methods based on measuring gradients obviously require
measurements at two or more heights, but use simpler
sensors. The disadvantage of the gradient technique is,
however, that a number of empirical functions may be
required to account for thermal stratification of the
atmosphere; additionally, the gradients in atmospheric
properties become very small close to vegetation canopies.
All the above techniques, when used above vegetation,
require that steady-state conditions exist, i.e. that atmospheric conditions are not changing rapidly over the
sampling period; they also all require extensive upwind
areas to be homogenous, i.e. these methods cannot be
used on isolated plots or small fields. If these conditions
are met, then it is assumed that the flux measured just
above the vegetation is equal to that at the ground or
plant surfaces, and fluxes are constant with height, up to
a level dependent on the extent of upwind surface homogeneity and atmospheric mixing. These methods will be
described briefly in turn and some accompanying methodological issues mentioned.
Trace gas exchange
be used within plant canopies because of the inapplicability of gradient diffusion theory in this region (Raupach,
1988). The method does have the advantage of using
simple instrumentation.
Bowen ratio-energy balance method: Following the energy
conservation law it is therefore possible to write the
energy balance equation for a patch of ground as a sum
of at least four energy flux densities (Thorn, 1975):
+ H + LE+G+...=0
(3)
The Bowen ratio can be determined experimentally
(Monteith and Unsworth, 1990) as the ratio of the vertical
gradients of temperature (37") (or potential temperature)
and humidity (Be):
fi = y8T/8e
(4)
where y is the psyhrometric constant. The derivation of
equation 4 assumes that the turbulent transport coefficients for sensible (H) and latent heat (LE) are equal, i.e.
KH = KE (which is reasonable given that the dominant
transport mechanism is by mechanical and convective
turbulence). The fluxes can be determined by:
H=
LE =
(1+/3" 1 )
(1+/3)
(Rn-G)
cppAT+XAq
(7)
if a direct flux measurement is available of H or LE (e.g.
by eddy covariance), plus the relevant gradients, then:
AC
AC
-=
(8)
Aq
AT
The Bowen ratio-energy balance approach can be applied
in the roughness sublayer above vegetation as it only
assumes similarity of exchange coefficient between scalars
(Lenschow, 1995).
Direct methods
Eddy covariance: The eddy flux of any scalar can be
written
c
= wPc
(9)
where Fc is the flux density of scalar c, w is the vertical
wind speed, pc is the density (or concentration) of the
scalar. The overbar represents the mean of the product
over the sampling interval.
Records of wind speed, temperature and concentration
exhibit turbulent or irregular form; it is convenient to
regard these variables as the sum of a mean and a
fluctuating part. This process is known as Reynold's
decomposition (Arya, 1988) and for wind speed and
concentration can be written:
w = w + w'
(10)
(5)
Pc = Pc + Pc
(11)
(6)
where the primes represent the fluctuation about the
mean. Equation 9 can be re-written making use of this
decomposition to produce
The energy balance technique has been used extensively
in the past for determination of sensible and latent heat
fluxes over a range of crops and forests (Kim et al., 1989;
Barr et al., 1994) and its accuracy is mainly dependent
on the ability of instrumentation to measure small gradients of temperature and humidity, to measure the other
components of the energy budget (including net radiation
and soil heat fluxes) and in conditions which avoid local
advection. It can be particularly difficult to use the
technique when the net radiation values are small, for
example, at sunrise and sunset. The energy balanceBowen ratio approach can be extended to determine the
Ec = wp~c + wyc
(12)
which shows that the total vertical flux of any scalar is
the sum of a mean vertical flux wpc and an eddy flux
w'p'c. It will be noted that in the full expansion of equation
9, some terms involving the mean of a fluctuating component have been omitted from equation 12 because, by
definition vv'and p'c = 0; terms involving the mean of the
product of two fluctuating components, e.g. w'p'c will
rarely be zero.
One assumption normally made is that over a suitable
interval of time there is no mass movement of the air in
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P = H/LE
surface-atmosphere exchange of trace gases making the
assumption that the transfer characteristics for humidity,
temperature and the trace gas species are identical. There
are two formulations possible:
If gradients are measured of temperature (AT) and
humidity (Aq) are made simultaneously with gradients of
trace gas species (AC):
(2)
where Rn is net all-wave radiative energy flux, H, sensible
heat flux, LE, latent heat flux, and G is the soil heat flux
density. These four fluxes usually account for about
90-95% of the total energy available (maximum photosynthetic fluxes could account for up to 3%; fluxes representing the horizontal transport of energy in advective
situations could be greater, but if care is taken to use flat,
extensive, homogeneous field sites, can usually be
neglected).
The determination of sensible and latent heat fluxes (H
and LE) can be achieved by introducing the definition of
the Bowen ratio (ft):
1135
1136 Moncrieff
the vertical i.e. w = 0. With this proviso, the practical
working equation for eddy covariance is obtained from
equation 10, which is
Fc = w'p'c + correction terms
(13)
(c) the entity in question must be averaged to some extent
by the finite sampling volume of the sensor, for example,
typically 20 cm between sonic transducers or between the
source and detector of infra-red radiation in an openpath analyser,
(d) the data acquisition hardware may not sample rapidly
enough to capture high frequency eddies,
(e) in the special case of using a closed-path analyser and
ducting air, some of the turbulent structure will be lost,
particularly the higher frequencies and again this will
result in flux underestimation unless accounted for,
(f) all the other usual micrometeorological requirements
must also be met including stationarity, homogeneity of
upwind surface and fetch (these issues have been well
explored in many previous reviews such as Lenschow,
1995; Verma, 1990; Baldocchhi et al. 1988).
Although this list can appear quite daunting, in practice, these corrections are well known and several papers
describing eddy covariance systems give details, for
example, Shuttleworth et al. (1988) and Moncrieff et al.
(1997). Specific experiments have been reported which
attempt to test rigorously the correction terms and the
general feeling amongst micrometeorologists is that the
corrections can be well quantified and can be relied upon
(Suyker and Verma, 1993; Leuning and Judd, 1996).
Fc=w'p'c + fjL(pJpa)LE + other correction terms (14)
Instrumentation
where n = mjmv, the ratio of the molecular masses of dry
air to water vapour, pa = density of dry air, p,. = mean
density of CO2 in air. This equation assumes that both
water vapour and CO2 are brought to a common temperature and pressure within the optical bench. Leuning
et al. (1982) provided experimental proof of the WPL
corrections, Leuning and Moncrieff (1990) developed the
arguments for a closed-path system and Leuning and
King (1992) applied the equations to both open- and
closed-path systems.
The working equation shows that it is necessary to
have instrumentation which can sample vertical wind
speed and scalar concentration and be able to perform
either real-time analysis in which means are subtracted
from raw data to yield the fluctuating components then
cross-products formed or have the facility to store all the
raw data for later processing in the laboratory.
Corrections
The other corrections can be summarized as:
(a) the sensor may not be capable of responding quickly
enough to all of the flux-carrying eddies moving past it.
In order to apply the eddy covariance equation, measurements of the fluctuating components of trace gas concentration and vertical wind speed are needed. Both vertical
wind speed and concentration have to be measured with
fast response sensors in order to catch the majority of
the fluctuating components of the turbulent structures
which are responsible for the fluxes. Sonic anemometers
can measure the vertical velocity to an accuracy of about
0.5 cm s"1 and usually measure all three components of
the turbulent wind, i.e. two horizontal and one vertical
component. Modern sonic anemometers also measure the
speed of sound and this can be used to infer air temperature and hence sensible heat flux (or more correctly and
virtually identically, virtual heat flux, Schotanus et al.,
1983). The concentration of carbon dioxide and water
vapour in air can be measured by means of a rapidly
responding infra-red gas analyser. Originally, only openpath analysers were available for fast response determinations of carbon dioxide and water vapour concentration
(Ohtaki and Matsui, 1982). In these instruments, a source
of infra-red radiation is separated from a detector by a
path which is open to air to pass freely between. Technical
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The assumption that w = 0 is problematic, but sufficient
experimental evidence suggests that it can be corrected
for in subsequent analysis. The issue is that sensible and
latent heat fluxes cause variations in air density and most
non-dispersive infra-red gas analysers measure the density
of the trace gas species in air rather than the mixing ratio
or mole fraction. The effect can be substantial for trace
gases which have fluxes which are small in relation to
their background concentration (Fowler and Duyzer,
1989). The need for a correction is also dictated by the
type of measuring system in use, i.e. measuring CO2 by
an open-path gas analyser may require corrections of
50-100% and opposite in sign simply due to simultaneous
transfer of sensible heat in the middle of the day (Suyker
and Verma, 1993). By contrast, in closed-path systems,
temperature fluctuations can be effectively eliminated by
passage down a sampling tube and the correction term
for sensible heat flux is eliminated (although a correction
for latent heat flux would remain unless the air was dried
before entering the optical bench). A paper by Webb
et al. (1980, hereafter referred to as WPL) showed how
to calculate this effect and equation 14 is written for a
typical closed-path IRGA, in this example, one measuring
CO2 and H2O in the same instrument. The flux of CO2
would be
(b) the sensor for w may be too far from the scalar sensor
and flux loss can occur,
Trace gas exchange
The design of an eddy covariance system
An eddy covariance system comprises not just the instrumentation, but also the software used to analyse the data
and to correct for any flux loss imposed by the inevitable
inability of the system to respond to all the flux-carrying
eddies. Different design criteria need to be applied in
systems employing open- or closed-path infra-red gas
analysers (Leuning and Judd, 1996). Fortunately, a
number of complete systems have been described in detail
in the literature and it is not necessary to 're-invent the
wheel' when it comes to putting together a system (Lloyd
et al., 1984; Moncrieff et al., 1997; Grelle and Lindroth,
1996). These papers can be consulted to discover the
necessary steps to be taken to correct for the inadequate
sampling of any turbulent signal in an eddy covariance
system.
Figure 1 shows a schematic of a typical eddy covariance
system in which air is ducted down a sampling tube from
a point near the sensing volume of the sonic anemometer
to a closed-path IRGA. Variations in flow rate are
automatically compensated for by having an in-line pressure transducer providing relevant information to correction algorithms within the controlling software of the
IRGA itself (Valentini et al., 1996). It is also possible to
maintain flow rates at a fairly constant level by including
a mass flow controller in the sampling line (Moncrieff
et al., 1997).
Evaluation of eddy covariance systems
Filter
Pressure
Closed Path
Analyzer
LJ6262
Air pump
O
Flow meter
PC
Fig. 1. Schematic of a typical eddy covariance system. Air is drawn
through a sample tube (with pre-filter) to the IRGAs optical bench by
a pump; the sonic anemometer digitises the turbulence signals and also
samples and digitizes the output from the IRGA, the process being
controlled by software on a PC.
heat transfer (G) and canopy heat storage (S)—is
employed as a test in many eddy covariance flux studies
(Baldocchi et al., 1988; Valentini et al., 1991; Greco and
Baldocchi, 1996). The ability to close the surface energy
balance, demonstrated by plotting net radiation against
the sum of H, LE and G is one test for an eddy covariance
system and closure over a sufficiently long period (days),
can demonstrate that the system is working properly
(Fig. 2). Typically, errors can account for variability
on the order of 10-20%. Other tests are based on comparing the spectral and co-spectral response of individual
instruments or the whole system against some well-tested
Deciduous forest 1993-1994
250
-50
-50
The quality of eddy covariance data sets can be tested by
examining the ability to close the surface energy balance
and checking the spectral response of the turbulence
measurements. Closure of the surface energy balance—
the partitioning of net radiation (R^ into H, LE and soil
3D
sonic
50
100
150
200
250
. ^ dally avaraga fWm" 2 )
Fig. 2. Typical test for an eddy covariance system showing the degree
of energy balance closure. Integrated daily values of net radiation are
plotted against the sum of sensible, latent and soil heat flux plus canopy
heat storage. (Greco and Baldocchi, 1996).
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improvements to more conventional closed-path analysers
of the kind traditionally employed in plant physiological
research has meant that eddy covariance systems based
on this design have become more common in recent years.
These instruments have optical benches with a smallvolume and through which air can be sampled at several
litres per minute to achieve the necessary response time.
Closed-path analysers are commercially available (few
open-path IRGAs can be bought commercially), they can
be easily calibrated with gas mixtures in situ and as air is
brought to a common temperature before entering the
optical bench, they require smaller corrections for air
density effects (the WPL corrections). Perhaps just as
crucially is the fact that the systems can be made weatherproof and can be left unattended for extended periods
(Moncrieff et al., 1997; Goulden et al., 1996). The adoption of such technology means that micrometeorology is
no longer regarded as a 'fair weather science'.
1137
1138 Moncrieff
standard forms. Again, details of the tests which system
builders have used appear in papers describing existing
systems (Lloyd et al, 1984; Grelle and Lindroth, 1996;
Moncrieff ef al, 1997). The implications of errors in eddy
covariance systems and how they affect the long-term
measured carbon balance of ecosystems are now also
being addressed given that the technology is now mature
enough to start monitoring over extended periods
(Baldocchi et al, 1996). Particular tests for assessing the
quality and reliability of surface-based flux measurements
have been demonstrated both theoretically (Businger and
Delaney, 1990; Foken and Wichura, 1996) and by reference to existing long-term datasets (Moncrieff et al,
1996). As an example of the long-term precision of eddy
covariance systems to measure carbon sequestration over
extended periods, the work done at Harvard forest in the
US over several years, indicates that an uncertainty of
+ 5% might be expected in well-maintained and wellcharacterized eddy flux systems (Goulden et al, 1996).
D144 1993
Whilst eddy covariance techniques overcome most of the
problems involved with gradient measurements, it is
applicable only to those gaseous species for which traditional fast response analysers are commercially available,
effectively, CO2 and H2O. Thus, for example, measure-
1800
2400
600
1200
1800
2400
1200
1800
2400
2000
Time (hour*)
Fig. 3. Daily trend of carbon dioxide flux (Fc), water vapour ( LE) and
PAR over a mixed deciduous forest in Tennessee, USA, May 1993.
Surface fluxes were obtained by eddy covariance. (Greco and
Baldocchi, 1996)
1
i
22-05-93
24-05-93
Ll
i
U
nn
r-
20 -
1
23-05-93
21-05-93
10 -
o
A
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Eddy accumulation
1200
350
Examples
Figure 3 shows daily trends of the exchange of carbon
dioxide, Fc photosynthetically active radiation, PAR, and
latent heat, LE, between a mixed deciduous forest canopy
(Tennessee, USA) and the atmosphere in May 1993
(Greco and Baldocchi, 1996). The magnitude of carbon
dioxide uptake (negative values) increases with increasing
PAR and achieves a peak value near — 2.0 mg CO2 m2
s"1 around midday. As the afternoon progressed, rates
of carbon dioxide uptake slowly decrease until around
7.30 p.m., when respiration (positive values) exceeds net
assimilation. Nocturnal rates of CO2 efflux are on the
order 0.2 mg m2 s~\ The net daily carbon dioxide flux is
-40.6 g CO2 m2 d"1 corresponding to 11.1 g C m" 2 d"1.
For LE and PAR, significant rates of exchange commence
at sunrise and peak values occur after midday. The peak
values for LE and PAR are 340 W m~2 and 1700^mol
m" 2 s"1, respectively. Figure 4 shows weekly variations
of CO2 exchange rates, Fc, over a beech forest in Central
Italy (Valentini et al, 1996). In this case, positive values
are related to CO2 accumulation by the forest during the
day and negative values of Fc represent night-time release
of carbon dioxide due to forest respiration. The weekly
averaged peak value for daytime CO2 flux density was
about + 15 /xmol m~2 s~\ while the averaged night-time
value was about -9 ^mol m~2 s~'.
600
-10 0
20
40
60
80
100
120
140
Time
(hr)
Fig. 4. Weekly variation in CO 2 exchange rate over a beech forest in
Central Italy, May 1993. Positive values indicate net uptake by the forest.
Trace gas exchange
F x = jSoaH,(Cx+-C;c-)
A Sonic anemometer
Air Pump
Solenoid valve
B
Absorbing
traps
(15)
where |3O is a semi-empirical coefficient (with a typical
value of about 0.56), ow the standard deviation of vertical
wind speed and Cx and C~, the concentration of the gas
in the up- and down-reservoirs, respectively. The basic
principle of the technique remains that the air should be
sampled according to the sign of the vertical wind speed,
but the sampling is done simply on the condition of the
vertical wind, i.e. either up or down. Relaxed eddy
accumulation (REA) is now popular and a number of
designs have appeared in the literature for compounds
such as CO 2 , CH 4 , NO 2 , non-methane hydrocarbons, and
pesticides (Beverland et al., 1996a, b; Majewski et al.,
1993). The WPL corrections may be required with this
technique according to the degree of pre-processing of
the air streams (Pattey et al., 1992). The relative errors
in this technique are similar to those in eddy covariance
as has been shown by a number of studies which use
both techniques simultaneously (Fowler et al., 1995).
Figure 5a shows a basic REA scheme with one solenoid
valve, two Teflon bags for collection of the gas and a
sonic anemometer.
Not all chemical species can be measured in exactly the
same way, however. For example, the determination of
VOCs requires particular attention, such as the use of a
pump at the top of the line and bags, whose internal
surfaces have to be previously well cleaned in order to
avoid any contamination. A second scheme is based on
the use of collecting samples on chemical absorbers
Solenoid valves
Air pump
Fig. 5. (a) A schematic of a basic configuration for an eddy accumulation system with one solenoid valve, two teflon bags for sample
collection and a sonic anemometer, (b) As above but with absorbing
tubes rather than sampling bags.
instead of in bags (Fig. 5b). The advantage of this
configuration is it avoids the problem of contamination
since air is drawn through the two traps which collect air
according to the sign of vertical wind speed (+ up-draft,
- down-draft). When air is sampled through one trap,
the other solenoid valve is open to the external air.
Improvements and innovations are regularly being suggested and these ensure that relaxed eddy accumulation
will find increasing favour in biosphere-atmosphere
experiments (Oncley et al., 1993).
Figure 6 shows an example of flux determination with
a relaxed eddy accumulation system. The graph shows
the diurnal trend of a-pinene flux emitted by a mixed
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ments of Volatile Organic Compound's (VOC's) are not
possible by eddy covariance. Developments with tunable
diode laser systems promise some widening of the scope
for eddy covariance, given that fluxes of methane and
nitrous oxide can now be measured successfully (Edwards
et al., 1994; Fowler et al., 1995), but its application to
other trace gases is still restricted. A technique related to
eddy covariance is rapidly gaining acceptance as it swaps
the difficulty of making fast analysis of the chemical
species for the much more practical high-precision of
slower responding chemical analysers, The technique is
known as eddy accumulation or conditional sampling. In
its original form (Desjardins, 1977) air was sampled into
two separate reservoirs according to the magnitude and
direction of the vertical wind. Although the technique
was used it was never a great success because of the
difficulty of collecting rapid samples at a rate proportional
to the magnitude of the vertical velocity (Speer et al,
1985). A practical solution has been the use of a 'relaxed'
form of the initial eddy accumulation theory in which an
empirical coefficient is introduced which effectively eliminates the need to sample at variable rates. This form takes
the name of relaxed eddy accumulation (Businger and
Oncley, 1990) and can be expressed as follows for the
flux Fx of a chemical species x:
1139
1140 Moncrieff
a - pincne density flux over a pine - oak forest
1.0 +
1
1
1
i
0.8 -
-
0.6 0.4 -
\
0.2
0 0 H»
h—m
i
i
10
15
20
hours
Fig. 6. Trend of a-pinene over a mixed pine-oak forest near
Castelporziano, Italy using the relaxed eddy accumulation system
shown in Fig. 5b.
Conclusions
Fetch: the concept of a 'flux footprint'
Fluxes measured by micrometeorological sensors are
effectively the integration of fluxes from a variety of
sources and sinks in the landscape for a distance of
several hundred metres upwind from the measuring point.
The height at which the measurements are chosen to be
made must be determined both by a consideration of the
frequency response of the instrumentation and also the
'fetch' or extent of the upwind area which is uniform.
Eddies become progressively larger with height up to the
depth of the planetary boundary layer, typically 1 km by
day, and this means that instrumentation with a slower
response can be used successfully at heights well above
the vegetation. As the surface is approached, however,
the spectrum of turbulence includes a greater proportion
of smaller eddies which will be actively exchanging mass
and momentum between the surface and the atmosphere.
The instrumentation then must be capable of sampling
the high frequency eddies, typically up to 10 Hz. In
principle, whilst it may be less difficult to measure surface
fluxes using the eddy covariance technique with height,
in practice, the difficulty lies in ensuring that the boundary
layer that is being measured is the one representative of
the vegetation upwind. If the instruments are placed too
high above the surface it is possible that they could extend
out of the boundary layer representative of the upwind
vegetation and instead be measuring some component of
fluxes from a different type of vegetation some greater
distance upwind. A convenient rule-of-thumb suggests a
Continued developments in both theory and instrumentation suggest that making flux measurements by micrometeorological methods will continue to play a central role
in studying land-atmosphere exchange of radiativelyactive gases. Traditional methods based on establishing
exchange coefficients will continue to be used but, increasingly, it will be possible to make routine, long-term flux
measurements by eddy covariance and eddy accumulation
methods. This is essential to ensure the questions of
global change biology are addressed and that the basic
data are available to parameterize and test simulation
models.
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