Results 201 to 210 of about 31,396 (258)
Advanced Functional Materials, EarlyView.In this report, we demonstrate that a crystalline phase of 52nm thick NiFe2O4 can be grown by RF sputtering on top of γ‐Al2O3(8nm)/SrTiO3 at a significantly low temperature (150 °C) without compromising the mobility and carrier density of the 2D electron gas at the γ‐Al2O3(8nm)/SrTiO3 interface.
Amit Chanda +11 more
wiley +1 more source
Radiative Cooling with Transparent Microstructured Hybrid Organic-Inorganic Polymer Film Fabricated by Nanoimprint Lithography. [PDF]
ACS Appl Mater InterfacesDimogerontaki N +2 more
europepmc +1 more source
Photoluminescence of ligand-protected gold nanoclusters: progress in experimental and theoretical studies. [PDF]
Chem SciLi K, Wang P, Pei Y.
europepmc +1 more source
Triplet Excitons Unlock Electroluminescence from Insulating Lanthanide Nanocrystals for Light-Emitting Diode Applications. [PDF]
Research (Wash D C)Li W, Lian W, Tu D.
europepmc +1 more source
Er<sup>3+</sup>/Yb<sup>3+</sup> co-doped ZnS quantum dots: structure, optical properties and up-conversion luminescence. [PDF]
RSC AdvNgan LTT +7 more
europepmc +1 more source
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2017
Abstract Radiative transfer is the process of energy transfer during the propagation of electromagnetic radiation through a medium. The processes of extinction, due to absorption and scattering, and thermal emission are described. It is shown how they can be represented by wavelength-dependent optical thickness, due to absorption or ...
Kelly Chance, Randall V. Martin
openaire +1 more source
Abstract Radiative transfer is the process of energy transfer during the propagation of electromagnetic radiation through a medium. The processes of extinction, due to absorption and scattering, and thermal emission are described. It is shown how they can be represented by wavelength-dependent optical thickness, due to absorption or ...
Kelly Chance, Randall V. Martin
openaire +1 more source
2005
Abstract We have already seen (Chapter 2) how the Sun delivers energy to the Earth as ultraviolet, visible, and near-infrared radiation, and how the Earth maintains an overall energy balance by re-emitting an equal amount of energy as long-wave, thermal infrared radiation.
openaire +1 more source
Abstract We have already seen (Chapter 2) how the Sun delivers energy to the Earth as ultraviolet, visible, and near-infrared radiation, and how the Earth maintains an overall energy balance by re-emitting an equal amount of energy as long-wave, thermal infrared radiation.
openaire +1 more source
Journal of Mathematical Physics, 1966
This paper presents an exact solution to the equations of radiative transfer for a generalization of the Uniform-Picket-Fence model discussed in a previous work. Here the absorption coefficient is allowed to take N different values over the frequency spectrum. Case's method is used to construct the normal mode solutions to the set of N coupled integral
C. E. Siewert, P. F. Zweifel
openaire +1 more source
This paper presents an exact solution to the equations of radiative transfer for a generalization of the Uniform-Picket-Fence model discussed in a previous work. Here the absorption coefficient is allowed to take N different values over the frequency spectrum. Case's method is used to construct the normal mode solutions to the set of N coupled integral
C. E. Siewert, P. F. Zweifel
openaire +1 more source