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Several groups have, therefore, studied the emission properties of lasing dyes or quantum dots infiltrated into inverted opal backbones [8].
In summary, we have studied the emission properties of semi-polar InGaN/GaN MQWs in the V-shaped pits.
We studied the emission mechanism of such novel GaN NPs, which showed controllable red shift of approximately 80 nm (approximately 600 meV) with increased optical excitation power.
Chichibu et al. (65) studied the emission mechanisms of GaN and InGaN quantum wells (QWs) by comparing their optical properties as a function of TD density, which was controlled by lateral epitaxial overgrowth technique.
In this Letter, we theoretically studied the emission spectra of 9 firefly oxyluciferin analogs in the gas phase and in solutions.
Here we further studied the emission heights of the BPs above the photosphere in the bipolar magnetic loops that are apparently associated with them.
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Since one cannot subject a piece of a distant star to conventional chemical analysis, studying the emission or absorption of starlight is the only way to determine the composition of stars or of interstellar gases and dust.
When studying the emission reduction related decision making problems, similar modelling methods are adopted.
Photoluminescence, Current Voltage and Electroluminescence measurements were used to study the emission and electron injection properties.
This work also aims at studying the emission intensities of active species generated during plasma polymerization and the chemical structure of the SPP films and correlates the results with the observed properties of the films.
More conventional PL mapping has also been found to be useful in examining the exciton diffusion in quantum wells [3], investigating the doping and structural composition of semiconductor heterostructures [4] and studying the emission properties of microcavity devices [5].
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