Effects of anisotropy on absorption cross-section spectra of medium-sized spheroidal corundum particles
Effects of anisotropy on absorption cross-section spectra of medium-sized spheroidal corundum particles
复制标题
各向异性对中等尺寸球状刚玉颗粒吸收截面光谱的影响
DOI:
10.1051/0004-6361/202038931
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发表时间:
--
影响因子:
6.5
通讯作者:
Th. G. Mayerhöfer
中科院分区:
文献类型:
--
作者:
S. Höfer;H. Mutschke;Th. G. Mayerhöfer
ContextIt has been widely accepted that corundum particles condense in the atmospheres of oxygen-rich asymptotic giant branch stars and effectively produce an infrared emission feature at 13μm. Laboratory experiments have predicted that these particles have the shape of oblate spheroids.AimsWe investigate the influence of the material anisotropy of uniaxial corundum on absorption cross section spectra of medium sized spheroidal particles in the infrared spectral region.MethodsWe compared absorption cross-section spectra of the anisotropic corundum particles gained by finite-difference time-domain simulations to spectra calculated by a weighted sum approximation of the according fictive isotropic materials, with one material having the dielectric function of thea–b-plane and the other having the dielectric function of thec-axis of corundum. We carried out investigations for different axes ratios of the spheroids, particles volumes, and different geometries of the dielectric axes to the particle axes as well as to the polarization and propagation direction of the incident light.ResultsWe observed several effects attributed to anisotropy that are non-additive, so that they cannot be reproduced with the combined spectra of the isotropic materials.ConclusionsCare should be taken when calculating the corundum infrared spectrum with simpler approaches. When particle sizes above 1μm are to be considered, the T-matrix formalism delivers correct band shifts and bulk modes for many, but not all bands. This remains true in orientation-averaged spectra and for particles in the 0.1μm size range.
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DOI:
10.5047/eps.2012.05.009
发表时间:
2013
期刊:
Earth, Planets and Space
影响因子:
--
作者:
K. Pitman;A. Hofmeister;A. Speck
通讯作者:
A. Speck
DOI:
10.1088/0004-637x/798/2/125
发表时间:
2015-01
期刊:
The Astrophysical Journal
影响因子:
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作者:
S. Zeidler;H. Mutschke;Th. Posch
通讯作者:
S. Zeidler;H. Mutschke;Th. Posch
DOI:
10.1016/j.jqsrt.2020.107241
发表时间:
2020
影响因子:
2.3
作者:
S. Höfer;H. Mutschke;Th. G. Mayerhöfer
通讯作者:
Th. G. Mayerhöfer
DOI:
10.1016/j.jqsrt.2020.106909
发表时间:
2020
影响因子:
2.3
作者:
S. Höfer;H. Mutschke;Th. G. Mayerhöfer
通讯作者:
Th. G. Mayerhöfer
DOI:
--
发表时间:
2007
期刊:
影响因子:
--
作者:
T. Posch;A. Baier;H. Mutschke;T. Henning
通讯作者:
T. Henning