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< xml version= 1.0 encoding= utf-8 > <!-- generator= Technorati API version 1.0 /bloginfo --> <!DOCTYPE tapi PUBLIC -//Technorati, Inc.//DTD TAPI 0.01//EN http://api.technorati.com/dtd/tapi-001.xml > <tapi version= 1.0 > <document> <result> <url>http://www.benhammersley.com</url> <weblog> <name>Ben Hammersley</name> <url>http://www.benhammersley.com</url> <rssurl>http://www.benhammersley.com/index.rdf</rssurl>

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and the growth and decay probabilities for adding or subtracting one molecule are and , respectively. The (i ) are proportional to c 1 = c and the (i ) are determined from detailed balance when c = c e . These equations, with extra terms allowing coagulation between clusters, were used by McMurry and Friedlander [54], McMurry [55, 56] and Rao and McMurry [57] to describe collision-controlled formation and growth of aerosols when there is no signi cant nucleation barrier. The macroscopic limit of the equations, when i (or the corresponding radius, R) becomes a continuous variable, was explored by Clement and Wood [58, 59], and the extra real-size diffusion in the aerosol size distribution which occurs with the discrete equations has been examined by Clement et al. [60]. The spreading resulting from the diffusion is only likely to be signi cant when supersaturations are small, but might apply to CCN in atmospheric water clouds. For supersaturations of greater than 10%, it was found that the largest spreading could be only 1 2 nm, so that, outside the nucleation region, it is always justi able to use the continuum equation for the growth of a size distribution, n(R, t): n(R)/ t + (n dR/dt)/ R = Sc (R, t) (3.77)

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Update the center vp and matrix Fp: vp,new = vp,old + a(xk vp,old) Fp,new = Fp,old + a ((xk vp,old)T(xk vp,old) Fp,old) Recalculate the partition matrix U. else dpk>rp Create a new cluster: vc+1 := xs; Fc+1 := Fp Calculate the number Pc+1. If Pc+1!Ptol Accept the new cluster, c:= c+1. else Refuse the new cluster and keep the old structure. end end

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