When two spheres are brought together, there is an enhancement in the
orientation-averaged extinction per unit volume compared to isolated s
pheres; ''proximity effects'' such as this are expected to be most imp
ortant at close separations. Using finite element methods for a pair o
f nearby Rayleigh spheres, this is both verified and quantified for th
e first time. The results are also expressed in terms of a normal mode
analysis. As more spheres are added to the system there is a further
growth in the extinction enhancement, which, however, depends on the t
opology. Arrangements of touching spheres examined included stacks, cl
ose packings, radiating structures, rings, chains, and clusters. Effec
tive medium theory models are often used to describe composite or poro
us particles. It is shown that with these models the extinction predic
ted is significantly higher than with finite element treatment of roug
hly equivalent particles. Furthermore, the effects of topology, not ac
counted for explicitly in effective medium theory models, are found to
be important. The modified prescription of effective medium theory pr
oposed by Ossenkopf does not provide better agreement with finite elem
ent methods unless the filling factor is high, higher than typical of
even compact clusters. Comparison between finite element methods and e
ffective medium theory models in the case of a laboratory soot sample
with high extinction yields a paradox that is discussed briefly.