Active control of light extraction in the near-IR range with sub-wavelength periodic structures

2018 ◽  
Author(s):  
A. Heliot ◽  
S. Archambeau ◽  
S. Pelloquin ◽  
O. Gauthier-Lafaye ◽  
A. Monmayrant ◽  
...  
Keyword(s):  
Active Control ◽  
Periodic Structures ◽  
Light Extraction ◽  
Near Ir ◽  
Near Ir Range ◽  
Sub Wavelength

A novel ruthenium(ii) complex for two-photon absorption-based optical power limiting in the near-IR range

2011 ◽  
Vol 13 (38) ◽  
pp. 17304 ◽  
Author(s):  
Mickaël Four ◽  
Didier Riehl ◽  
Olivier Mongin ◽  
Mireille Blanchard-Desce ◽  
Latévi Max Lawson-Daku ◽  
...  
Keyword(s):  
Optical Power ◽  
Photon Absorption ◽  
Two Photon Absorption ◽  
Two Photon ◽  
Near Ir ◽  
Optical Power Limiting ◽  
Near Ir Range

scholarly journals Optimal spectral inversion of atmospheric radiometric measurements in the near-UV to near-IR range: A case study

2002 ◽  
Vol 10 (1) ◽  
pp. 70 ◽  
Author(s):  
Didier Fussen ◽  
Filip Vanhellemont ◽  
Christine Bingen
Keyword(s):  
Radiometric Measurements ◽  
Spectral Inversion ◽  
Near Ir ◽  
Near Ir Range

On the possibility of designing a high-resolution heterodyne spectrometer for near-IR range on the basis of a tunable diode laser

2012 ◽  
Vol 42 (3) ◽  
pp. 244-249 ◽  
Author(s):  
A Yu Klimchuk ◽  
Aleksandr I Nadezhdinskii ◽  
Ya Ya Ponurovskii ◽  
Yu P Shapovalov ◽  
A V Rodin
Keyword(s):  
High Resolution ◽  
Diode Laser ◽  
Tunable Diode Laser ◽  
Near Ir ◽  
Heterodyne Spectrometer ◽  
Near Ir Range

scholarly journals Detection of O2 Produced Abiotically on Habitable but Lifeless Planets around M-dwarfs

2012 ◽  
Vol 8 (S293) ◽  
pp. 39-45 ◽  
Author(s):  
Tong Li ◽  
Feng Tian
Keyword(s):  
Radiative Transfer ◽  
Molecular Oxygen ◽  
Uv Spectra ◽  
Radiative Transfer Model ◽  
Transfer Model ◽  
Hitran Database ◽  
M Dwarfs ◽  
Near Ir ◽  
Habitable Zones ◽  
Near Ir Range

AbstractHigh atmospheric abundances of oxygen has been widely considered to be a reliable biosignature for life on exoplanets in the habitable zones of all types of stars. Recently it was proposed that the unique UV spectra of observed planet-hosting M dwarfs could lead to the buildup of molecular oxygen in the atmospheres of habitable but lifeless planets around these stars (Tian et al. 2014). However, the detectability of the accumulated O2 was not modeled. In this work we developed a new line by line radiative transfer model based on HITRAN database and used the model to simulate the reflectivity in the visible and near IR range. We show that abiotically produced and maintained O2 in the 0.2% level is observable at 13105 cm−1 (0.76 μm) with the spectra resolution of 70.

Sign in / Sign up

Export Citation Format

Share Document