Results 41 to 50 of about 4,004,079 (302)

Radiative transfer simulations of magnetar flare beaming [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2016
17 pages, 8 figures, accepted for publication in ...
van Putten, T.   +3 more
openaire   +4 more sources

Optimised frequency grids for infrared radiative transfer simulations in cloudy conditions

open access: yes, 2012
This paper shows that radiometer channel radiances for cloudy atmospheric conditions can be simulated with an optimised frequency grid derived under clear-sky conditions. A new clear-sky optimised grid is derived for AVHRR channel 5 ð12 m m, 833 cm 1 Þ.
Mendrok, Jana,   +7 more
core   +1 more source

Radiative Transfer Modeling of Simulation and Observational Data [PDF]

open access: yesProceedings of the International Astronomical Union, 2010
AbstractRadiative Transfer (RT) is considered to be one of the four Grand Challenges in Computational Astrophysics aside of Astrophysical Fluid Dynamics, N-Body Problems in Astrophysics, and Relativistic Astrophysics. The high dimensionality (7D instead of 4D for MHD) and the underlying integro-differential transport equation have forced coders to ...
Jürgen Steinacker   +2 more
openaire   +1 more source

PORT, a CESM tool for the diagnosis of radiative forcing [PDF]

open access: yesGeoscientific Model Development, 2013
The Parallel Offline Radiative Transfer (PORT) model is a stand-alone tool, driven by model-generated datasets, that can be used for any radiation calculation that the underlying radiative transfer schemes can perform, such as diagnosing radiative ...
A. J. Conley   +4 more
doaj   +1 more source

A MODEL TO SIMULATE THE RADIATIVE TRANSFER OF FLUORESCENCE IN A LEAF [PDF]

open access: yesThe International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, 2018
Abstract. Light is reflected, transmitted and absorbed by green leaves. Chlorophyll fluorescence (ChlF) is the signal emitted by chlorophyll molecules in the leaf after the absorption of light. ChlF can be used as a direct probe of the functional status of photosynthetic machinery because of its close relationship with photosynthesis.
F. Zhao, Q. Ni
openaire   +3 more sources

Multidimensional simulations of radiative transfer in Type Ia supernovae [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2007
11 pages, 8 figure. Accepted for publication by MNRAS.
openaire   +4 more sources

Radiation-hydrodynamics Effects in an Inhomogeneous Medium

open access: yesThe Astrophysical Journal
Radiation flow through an inhomogeneous medium is critical in a wide range of physics and astronomy applications, from transport across cloud layers on the Earth to the propagation of supernova blast waves producing ultraviolet and X-ray emission ...
Christopher L. Fryer   +11 more
doaj   +1 more source

Enhanced Cloud Top Longwave Radiative Cooling Due To the Effect of Horizontal Radiative Transfer in the Stratocumulus to Trade Cumulus Transition Regime

open access: yesGeophysical Research Letters, 2023
Recent studies develop the SPeedy Algorithm for Radiative TrAnsfer through CloUd Sides (SPARTACUS) to handle the influence of horizontal RT on vertical radiative fluxes within an atmospheric column.
Tong Ren   +4 more
doaj   +1 more source

Air‐Pressure–Actuated Vibroacoustic Metamaterial With Tunable Bandgap: Design, Modeling, and Characterization

open access: yesAdvanced Engineering Materials, EarlyView.
This article presents the design, modeling, and characterization of air‐pressure–actuated programmable vibroacoustic metamaterials (PVAMM). The study focuses on leveraging air pressure to dynamically tune resonance frequencies for effective noise attenuation.
William Kaal   +2 more
wiley   +1 more source

Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events

open access: yesThe Astrophysical Journal Supplement Series
Radiation hydrodynamics (RHD) determines the bulk evolution and observable emission in a wide variety of high-energy astrophysical phenomena. Due to their complexity, RHD problems must usually be studied through numerical simulations.
Itamar Giron   +3 more
doaj   +1 more source

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