Optical BRDF and BSDF measurements of human incisors from visible to mid-infrared wavelengths

2001 ◽  
Author(s):  
David W. Blodgett ◽  
S. C. Webb
Keyword(s):  
Mid Infrared ◽  
Infrared Wavelengths

Assessment of the accuracy of scaling methods for radiance simulations at far and mid infrared wavelengths

2021 ◽  
pp. 107739
Author(s):  
Michele Martinazzo ◽  
Davide Magurno ◽  
William Cossich ◽  
Carmine Serio ◽  
Guido Masiello ◽  
...  
Keyword(s):  
Mid Infrared ◽  
Scaling Methods ◽  
Infrared Wavelengths

Kerr nonlinearity and multi-photon absorption in germanium at mid-infrared wavelengths

2017 ◽  
Vol 111 (9) ◽  
pp. 091902 ◽  
Author(s):  
B.-U. Sohn ◽  
C. Monmeyran ◽  
L. C. Kimerling ◽  
A. M. Agarwal ◽  
D. T. H. Tan
Keyword(s):  
Kerr Nonlinearity ◽  
Photon Absorption ◽  
Mid Infrared ◽  
Infrared Wavelengths

scholarly journals The Cepheid Period‐Luminosity Relation at Mid‐Infrared Wavelengths. I. First‐Epoch LMC Data

2008 ◽  
Vol 679 (1) ◽  
pp. 71-75 ◽  
Author(s):  
Wendy L. Freedman ◽  
Barry F. Madore ◽  
Jane Rigby ◽  
S. E. Persson ◽  
Laura Sturch
Keyword(s):  
Mid Infrared ◽  
Infrared Wavelengths

scholarly journals THE NON-UNIFORM, DYNAMIC ATMOSPHERE OF BETELGEUSE OBSERVED AT MID-INFRARED WAVELENGTHS

2011 ◽  
Vol 740 (1) ◽  
pp. 24 ◽  
Author(s):  
V. Ravi ◽  
E. H. Wishnow ◽  
C. H. Townes ◽  
S. Lockwood ◽  
H. Mistry ◽  
...  
Keyword(s):  
Mid Infrared ◽  
Infrared Wavelengths

scholarly journals Earth-based observations of impact phenomena

1996 ◽  
Vol 156 ◽  
pp. 81-109
Author(s):  
Philip D. Nicholson
Keyword(s):  
Hubble Space Telescope ◽  
Common Pattern ◽  
Mid Infrared ◽  
Wide Range ◽  
Impact Phenomena ◽  
Infrared Wavelengths ◽  
Positive Correlations ◽  
The Individual ◽  
The Impact ◽  
Size Estimates

Earth-based observations at near- and mid-infrared wavelengths were obtained for at least 15 of the SL9 impacts, ranging from the spectacular G, K and L events to the barely-detected N and V impacts. Although there were a few exceptions, most of the IR lightcurves fit a common pattern of one or two relatively faint precursor flashes, followed several minutes later by the main infrared event as the explosively-ejected plume crashed down onto the jovian atmosphere. Correlations with the impact times recorded by the Galileo spacecraft and plumes imaged by the Hubble Space Telescope lead to an interpretation of the twin precursors in terms of (i) the entry of the bolide into the upper atmosphere, and (ii) the re-appearance of the rising fireball above Jupiter's limb. Positive correlations are observed between the peak IR flux observed during the splashback phase and both pre-impact size estimates for the individual SL9 fragments and the scale of the resulting ejecta deposits. None of the fragments observed to have moved off the main train of the comet by May 1994 produced a significant impact signature. Earth-based fireball temperature estimates are on the order of 750 K, 30-60 sec after impact. For the larger impacts, the unexpectedly protracted fireball emission at 2.3 μm remains unexplained. A wide range of temperatures has been inferred for the splashback phase, where shocks are expected to have heated the re-entering plume material at least briefly to several thousand K, and further modelling is required to reconcile these data.

scholarly journals Mid-infrared GaAs/AlGaAs micro-ring resonators characterized via thermal tuning

RSC Advances ◽  
2019 ◽  
Vol 9 (15) ◽  
pp. 8594-8599 ◽  
Author(s):  
Julian Haas ◽  
Philipp Artmann ◽  
Boris Mizaikoff
Keyword(s):  
Thin Film ◽  
Ring Resonators ◽  
Mid Infrared ◽  
Infrared Wavelengths ◽  
Thermal Tuning

Micro-ring resonators with a decoupling waveguide have been fabricated from thin-film GaAs/Al0.2Ga0.8As waveguides accommodating mid-infrared wavelengths, and were characterized in detail via thermal tuning.

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