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The Theory of Cosmic Grains (Paperback, Softcover reprint of the original 1st ed. 1991)
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The Theory of Cosmic Grains (Paperback, Softcover reprint of the original 1st ed. 1991)
Series: Astrophysics and Space Science Library, 168
Expected to ship within 10 - 15 working days
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Light scattering and absorption by small homogeneous particles can
be worked-out exactly for spheres and infinite cylinders.
Homogeneous particles of irregular shapes, when averaged with
respect to rotation, have effects that can in general be
well-approximated by reference to results for these two idealised
cases. Likewise, small inhomogeneous particles have effects similar
to homogeneous particles of the same average refractive index. Thus
most problems can be solved to a satisfactory approximation by
reference to the exact solutions for spheres and cylinders, which
are fully stated here in the early part of the book. The sum of
scattering and absorption, the extinction, is too large to be
explained by inorganic materials, provided element abundances in
the interstellar medium are not appreciably greater than solar, H 0
and NH3 being essentially excluded in the 2 general medium,
otherwise very strong absorptions near 3p, m would be observed
which they are not. A well-marked extinction maximum in the
ultraviolet near 2200A has also not been explained satisfactorily
by inorganic materials. Accurately formed graphite spheres with
radii close to O.02p, m could conceivably provide an explanation of
this ultraviolet feature but no convincing laboratory preparation
of such spheres has ever been achieve
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