Issue 10, March 2004
The
First Announcement of the 8th Conference on Electromagnetic and Light
Scattering by Nonspherical Particles, which will
be
held in Salobreña, Granada, Spain, on May 16-20, next year is available on the
following link:
http://www.iaa.csic.es/~confels8
Fernando Moreno,
Instituto de Astrofisica de Andalucia,
Granada, Spain
New papers on
electromagnetic scattering
Lidar Backscatter Properties of Al2O3 Rocket Exhaust
Particles
Robert A. Reed and Mitchel K. Nolen, ATA Inc., AEDC Group Arnold
Air Force Base, TN 37389
Michael E. Zolensky, NASA Johnson Space Center
John Giles and Peter Lang,
Johns Hopkins Univ. Applied Physics Lab
Michael I. Mishchenko, NASA Goddard Institute for Space Studies
Martin N. Ross, Aerospace Corp.
The lidar
backscatter cross sections of aluminum oxide rocket exhaust particles are
sensitive to slight deviations from their nominal spherical shape. We have
therefore determined
the
distribution of particle shapes using automated image analysis of scanning
electron microscope particle photographs. These shape statistics were used to
in conjunction with
T-matrix
calculations for nonspherical particles to estimate the backscatter properties
of representative rocket exhaust particles. For the range of particle sizes and
nonsphericities
relevant to
exhaust plumes, both the backscatter intensity and depolarization scale
approximately with the product of nonsphericity times the particle radius. This
correlation allows
us to
formulate a simple model for both the backscatter intensity and the
depolarization of typical Al2O3 rocket exhaust particles.
This model is applied to a recent particle collection
from the exhaust
plume of a Titan-IVA rocket obtained from the NASA WB-57F high-altitude
research aircraft at an altitude of 19 km.
Submitted
to the AIAA J Spacecraft ad Rockets
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OPTICS OF COSMIC DUST. Part I
Nikolai V. VOSHCHINNIKOV
St. Petersburg University, Russia
The optics of small particles is useful in the interpretation of observational phenomena related to the extinction, scattering and emission of radiation by dust grains in space. Three
components of dust modeling - optical constants, light scattering theories and object' models - are briefly discussed. The author aims to show how the general laws of the optics
of dust particles work and to highlight the information about cosmic dust which is reliable and the information which can be false. Part I of the review contains a detailed
analysis of the interstellar extinction and polarization (forward-transmitted radiation).. Part II will consider the scattered radiation, dust absorption and emission, radiation pressure
and dust properties in different objects.
Astrophysics and Space Physics Reviews, v. 12, pp. 1--182, 2004
Figures 45, Tables 13, References 397
ISBN: 1-904868-23-1
Price: £~30.00, Euro 45.17, $55.18 plus postage
Order from: Cambridge Scientific Publishers
P.O.Box 806, Cottenham, Cambridge CB4 8QY, UK Phone: +44 (0) 1954 251 283, Fax: +44 (0) 1954 252 517
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