Online: http://dust.ess.uci.edu/facts Updated: Tue 5th Sept, 2006, 11:38
Particle Size Distributions:
Theory and Application to Aerosols, Clouds, and Soils
by Charlie Zender
University of California at Irvine
Department of Earth System Science zender@uci.edu
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Copyright © 2000, Charles S. Zender
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This document describes mathematical and computational considerations pertaining to size distributions. The application of statistical theory to define meaningful and measurable parameters for defining generic size distributions is presented in §2. The remaining sections apply these definitions to the size distributions most commonly used to describe clouds and aerosol size distributions in the meteorological literature. Currently, only the lognormal distribution is presented.
mdlsxn Lu and Bowman (2004) designed and optimal non-linear least squares-based procedure for converting from sectional to modal representations.
nomenclature There is a bewildering variety of nomenclature associated with size distributions, probability density functions, and statistics thereof. The nomenclature in this article generally follows the standard references, (see, e.g., Hansen and Travis, 1974; Patterson and Gillette, 1977; Press et al., 1988; Flatau et al., 1989; Seinfeld and Pandis, 1997), at least where those references are in agreement. Quantities whose nomenclature is often confusing, unclear, or simply not standardized are discussed in the text.
This section follows the carefully presented discussion of Flatau et al. (1989). The size distribution function nn(r) is defined such that nn(r) dr is the total concentration (number per unit volume of air, or # m-3) of particles with sizes in the domain [r,r + dr]. The total number concentration of particles N 0 is obtained by integrating nn(r) over all sizes
![]() | (1) |
The size distribution function is also called the spectral density function. The dimensions of nn(r) and N0 are # m-3 m-1 and # m-3, respectively. Note that n n(r) is not normalized (unless N0 happens to equal 1.0).
Often N0 is not an observable quantity. A variety of functional forms, some of which are overloaded for clarity, describe the number concentrations actually measured by instruments. Typically an instrument has a lower detection limit rmin and an upper detection limit rmax of particle sizes which it can measure.
Equations (2)(4) define the cumulative concentration, lower bound concentration, and truncated concentration, respectively. The cumulative concentration is used to define the median radius
n. Half the
particles are larger and half smaller than
n
![]() | (5) |
These functions are often used to define nn(r) via
![]() | (6) |
Note that the concentration nomenclature in (6) is N not N(r). Using N(r) would indicate
that the concentration has not been completely integrated over all sizes. By definition, the
total concentration N0 is integrated over all sizes, as defined by (1). A concentration denoted
N(r) makes no sense without an associated size bin width Δr, or truncation convention, as in
(2)(4). We try to use N and N0 for normalized (N = 1) and non-normalized (N0
1, i.e.,
absolute concentrations). However this convention is not absolute and (1) defines both N
and N0.
Describing size distributions is easier when they are normalized into probability density functions, or PDFs. In this context, a PDF is a size distribution function normalized to unity over the domain of interest, i.e., p(r) = Cnnn(r) where the normalization constant Cn is defined such that
![]() | (7) |
In the following sections we usually work with PDFs because this normalization property is very convenient mathematically. Comparing (7) and (1), it is clear that the normalization constant Cn which transforms a size distribution function (1) into a PDF p(r) is N0-1
![]() | (8) |
The merits of using radius r, diameter D, or some other dimension L, as the independent variable of a size distribution depend on the application. In radiative transfer applications, r prevails in the literature probably because it is favored in electromagnetic and Mie theory. There is, however, a growing recognition of the importance of aspherical particles in planetary atmospheres. Defining an equivalent radius or equivalent diameter for these complex shapes is not straighforward (consider, e.g., a bullet rosette ice crystal). Important differences exist among the competing definitions, such as equivalent area spherical radius, equivalent volume spherical radius, (e.g., Ebert and Curry, 1992; McFarquhar and Heymsfield, 1997).
A direct property of aspherical particles which can often be measured, is its maximum dimension, i.e., the greatest distance between any two surface points of the particle. This maximum dimension, usually called L, has proven to be useful for characterizing size distributions of aspherical particles. For a sphere, L is also the diameter. Analyses of mineral dust sediments in ice core deposits or sediment traps, for example, are usually presented in terms of L. The surface area and volume of ice crystals have been computed in terms of power laws of L (e.g., Heymsfield and Platt, 1984; Takano and Liou, 1995). Since models usually lack information regarding the shape of particles (exceptions include Zender and Kiehl, 1994; Chen and Lamb, 1994), most modelers assume spherical particles, especially for aerosols. Thus, the advantages of using the diameter D as the independent variable in size distribution studies include: D is the dimension often reported in measurements; D is more analogous than r to L.
The remainder of this manuscript assumes spherical particles where r and D are equally useful independent variables. Unless explicitly noted, our convention will be to use D as the independent variable. Thus, it is useful to understand the rules governing conversion of PDFs from D to r and the reverse.
Consider two distinct analytic representations of the same underlying size distribution. The first, nD n (D), expresses the differential number concentration per unit diameter. The second, nr n(r), expresses the differential number concentration per unit radius. Both nD n (D) and nr n(r) share the same dimensions, # m-3 m-1.
Consider an arbitrary function g(x) which applies over the domain of the size distribution p(x). For now the exact definition of g is irrelevant, but imagine that g(x) describes the variation of some physically meaningful quantity (e.g., area) with size. The mean value of g is the integral of g over the domain of the size distribution, weighted at each point by the concentration of particles
![]() | (13) |
Once p(x) is known, it is always possible to compute g for any desired quantity g. Typical quantities
represented by g(x) are size, g(x) = x; area, g(x) = A(x) ∝ x2; and volume g(x) = V (x) ∝ x3. More
complicated statistics represented by g(x) include variance, g(x) = (x -
)2. The remainder of this
section considers some of these examples in more detail.
The number mean size
of a size distribution p(x) is defined as
![]() | (14) |
Synonyms for number mean size include mean size, average size, arithmetic mean size, and
number-weighted mean size (Hansen and Travis, 1974). Flatau et al. (1989) define
n ≡
, a
convention we adopt in the following.
The variance σ2 x of a size distribution p(x) is defined in accord with the statistical variance of a continuous mathematical distribution.
![]() | (15) |
The variance measures the mean squared-deviation of the distribution from its mean value. The units of σ2 x are [m2]. Because σ2 x is a complicated function for standard aerosol and cloud size distributions, many prefer to work with an alternate definition of variance, called the effective variance.
The effective variance σ2 x,eff of a size distribution p(x) is the variance about the effective size of the distribution, normalized by xeff (e.g., Hansen and Travis, 1974)
![]() | (16) |
Because of the xeff-2 normalization, σ2 x,eff is non-dimensional in contrast to typical variances, e.g., (15). In the terminology of Hansen and Travis (1974), σ2 x,eff = v.
The standard deviation σx of a size distribution p(x) is the square root of the variance (15),
![]() | (17) |
σx has units of [m]. For standard aerosol and cloud size distributions, σx is an ugly expression. Therefore many authors prefer to work with alternate definitions of standard deviation. Unfortunately, nomenclature for these alternate definitions is not standardized.
Statistics of the gamma distribution are presented in http://asd-www.larc.nasa.gov/~yhu/paper/thesisall/node8.html. Currently, the mie program implements gamma distributions in a limited sense.
The lognormal distribution is perhaps the most commonly used analytic expression in aerosol studies.
Table 1 summarizes the standard lognormal distribution parameters. Note that
≡ ln σg.
The statistics in Table 1 are easy to misunderstand because of the plethora of subtly different
definitions. A common mistake is to assume that patterns which seems to apply to one distribution, e.g.,
the number distribution nn(D), apply to distributions of all other moments. For example, the number
distribution nn(D) is the only distribution for which the moment mean size (i.e., number mean size
n)
equals the moment-weighted size (i.e., number-weighted size Dn). Also, the number mean size
n differs
from the number median size
n by a factor of e
2∕2. But this factor is not constant and depends on the
moment of the distribution. For instance,
s differs from
s by e
2, while
s differs from
s by e3
2∕2.
Thus converting from mean diameter to median diameter is not the same for number as for mass
distributions.
Table 2 lists applies the relations in Table 1 to specific size distributions typical of tropospheric aerosols.
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