The role of numerical aperture in efficient estimation of spatially resolved reflectance by a Monte Carlo light propagation model

2017 ◽  
Author(s):  
Matic Ivančič ◽  
Peter Naglič ◽  
Boštjan Likar ◽  
Franjo Pernuš ◽  
Miran Bürmen
Keyword(s):  
Monte Carlo ◽  
Light Propagation ◽  
Numerical Aperture ◽  
Propagation Model ◽  
Efficient Estimation ◽  
Spatially Resolved

Extraction of optical properties from hyperspectral images by Monte Carlo light propagation model

2016 ◽  
Author(s):  
Matic Ivančič ◽  
Peter Naglič ◽  
Franjo Pernuš ◽  
Boštjan Likar ◽  
Miran Bürmen
Keyword(s):  
Monte Carlo ◽  
Optical Properties ◽  
Light Propagation ◽  
Propagation Model ◽  
Hyperspectral Images

scholarly journals Virtually increased acceptance angle for efficient estimation of spatially resolved reflectance in the subdiffusive regime: a Monte Carlo study

2017 ◽  
Vol 8 (11) ◽  
pp. 4872 ◽  
Author(s):  
Matic Ivančič ◽  
Peter Naglič ◽  
Franjo Pernuš ◽  
Boštjan Likar ◽  
Miran Bürmen
Keyword(s):  
Monte Carlo ◽  
Monte Carlo Study ◽  
Efficient Estimation ◽  
Acceptance Angle ◽  
Spatially Resolved

scholarly journals Bringing high spatial resolution to the far-infrared

2021 ◽  
Author(s):  
Hendrik Linz ◽  
Henrik Beuther ◽  
Maryvonne Gerin ◽  
Javier R. Goicoechea ◽  
Frank Helmich ◽  
...  
Keyword(s):  
Spatial Resolution ◽  
Formation Process ◽  
Far Infrared ◽  
Main Theme ◽  
Spatially Resolved ◽  
Research Areas ◽  
External Galaxies ◽  
Emergence Of Life ◽  
Fine Structure Lines

AbstractThe far-infrared (FIR) regime is one of the wavelength ranges where no astronomical data with sub-arcsecond spatial resolution exist. None of the medium-term satellite projects like SPICA, Millimetron, or the Origins Space Telescope will resolve this malady. For many research areas, however, information at high spatial and spectral resolution in the FIR, taken from atomic fine-structure lines, from highly excited carbon monoxide (CO), light hydrides, and especially from water lines would open the door for transformative science. A main theme will be to trace the role of water in proto-planetary discs, to observationally advance our understanding of the planet formation process and, intimately related to that, the pathways to habitable planets and the emergence of life. Furthermore, key observations will zoom into the physics and chemistry of the star-formation process in our own Galaxy, as well as in external galaxies. The FIR provides unique tools to investigate in particular the energetics of heating, cooling, and shocks. The velocity-resolved data in these tracers will reveal the detailed dynamics engrained in these processes in a spatially resolved fashion, and will deliver the perfect synergy with ground-based molecular line data for the colder dense gas.

Efficient estimation of unconditional capital by Monte Carlo simulation

2016 ◽  
Vol 16 ◽  
pp. 75-84
Author(s):  
Alex Ferrer ◽  
José Casals ◽  
Sonia Sotoca
Keyword(s):  
Monte Carlo Simulation ◽  
Monte Carlo ◽  
Efficient Estimation
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