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Dataset results
16 results for “radiational cooling”
Simulation results: Radiative cooling induced coherent maser emission in relativistic plasmas
<p>This repository contains some of the simulation data presented in the recent article titled <em>"Radiative cooling induced coherent maser emission in relativistic plasmas"</em> (<a href="https://arxiv.org/abs/2409.18955" target="_new" rel="noopener">https://arxiv.org/abs/2409.18955</a>). The data available are from 2D particle-in-cell (PIC) simulations, which investigate the effects of radiative cooling in relativistic plasmas and its role in inducing coherent maser emission. The simulations were performed using OSIRIS, a massively parallel and fully-relativistic PIC code.</p> <p>The electric field data in the third direction (E3) included here has been spatially averaged by a factor of 8 in both directions, resulting in a dataset that reflects a resolution 64 times lower than the actual simulation. Additionally, the raw data includes only one two-thousandth of the simulated electron macro-particles. Also included is the phase space data in the x2, p2, and p3 dimensions.</p> <p>These datasets represent key aspects of the simulation results discussed in the paper, where the focus is on understanding the interplay between radiative losses and coherent emission mechanisms.</p> <p>More details on the simulations and the analysis of these results can be found in the corresponding article.</p>
Dataset related to publication: Robust radiative cooling via surface phonon coupling-enhanced emissivity from SiO2 micropillar arrays
<p>Dataset related to the publication:</p><p>Zhenmin Ding, Xin Li, Hulin Zhang, Dukang Yan, Jérémy Werlé, Ying Song, Lorenzo Pattelli, Jiupeng Zhao, Hongbo Xu, Yao Li. Robust radiative cooling via surface phonon coupling-enhanced emissivity from SiO2 micropillar arrays. <i>International Journal of Heat and Mass Transfer</i>, 220, 125004 (2024). doi: <a href="https://doi.org/10.1016/j.ijheatmasstransfer.2023.125004">10.1016/j.ijheatmasstransfer.2023.125004</a></p><p>The repository contains MATLAB/Octave scripts to perform rigorous coupled-wave analysis (RCWA) simulations for a SiO2 layer decorated with micropillars.</p><p>The main script runs a series of rigorous electromagnetic simulations over the atmospheric transparency window wavelength range (8-13 µm) for all combination of three main structural parameters (pillar diameter, spacing and height), within a user-defined range.</p><p>Running the code requires the RETICOLO v9 RCWA code:</p><blockquote><p>Jean-Paul Hugonin, & Philippe Lalanne. (2021). Light-in-complex-nanostructures/RETICOLO: V9. Zenodo. <a href="https://doi.org/10.5281/zenodo.4419063">https://doi.org/10.5281/zenodo.4419063</a></p></blockquote>
Dataset related to publication: Nanoporous Film Layers to Enhance the Performance of Passive Radiative Cooling Paint Mixtures
<p>Dataset related to the publication:</p> <p><em>Giuseppe Emanuele Lio,</em><em> Sara Levorin</em><em>, Atakan Erdoğan</em><em>, Jérémy Werlé</em><em>, Alain J. Corso</em><em>, Luca </em><em>Schenato</em><em>, Diederik S. Wiersma</em><em>, Marco Santagiustina</em><em>, Lorenzo Pattelli</em><em>, Maria Guglielmina Pelizzo. </em><em>Nanoporous Film Layers to Enhance the Performance of Passive Radiative Cooling Paint Mixtures, accepted and in publishing on International Journal of Thermophysics. </em>DOI: 10.1007/s10765-024-03439-8</p> <p>The repository contains the temperature, relative humidity, irradiance, sky temperature and net cooling power measurements in the file named "DATA_IJT_Nanoporous_Film_ Layer.txt" and the python script (Data_analizer.py) to analyze them as done in the paper.</p> <p> </p> <p>The repository also contain the Matlab workspace (IJT_data.mat)and code (Data_R_ATR_analyzer)to evaluate all the sample reflectance and FTIR measurements. Moreover, the extra measurements performed on the Celgard thin film are available in the workspace "Celgard_UV_VIS_NIR_T.mat" and "R_Celgard.mat". Moreover in Version 2 all the used data for Reflectance and Transmittance are also available in "txt" format for a simple and fast usage. </p> <p> </p> <h2>Notes (English)</h2> <div> <table> <tbody> <tr> <td> <p>This work was partly supported by</p> <ul> <li>European Project 21GRD03 PaRaMetriC, which received funding from the European Partnership on Metrology, co-financed by the European Union's Horizon Europe Research and Innovation Programme, and from the Participating States.</li> <li>European Union - PON Research and Innovation 2014-2020 in accordance with Article 24, paragraph 3a), of Law No. 240 of December 30, 2010, as amended, and Ministerial Decree No. 1062 of August 10, 2021</li> </ul> </td> </tr> </tbody> </table> </div>
Reproduction packages for the paper "Spectral and Imaging properties of Sgr A∗ from High-Resolution 3 DGRMHD Simulations with Radiative Cooling"
<p>This is a basic reproduction package for the paper"Spectral and Imaging properties of Sgr A∗ from High-Resolution 3D GRMHD Simulations with Radiative Cooling" by Yoon et al. (2020). It aims to provide the most important data products to check and reproduce the main results of the paper.</p>
Datasets to "Turbulent radiative diffusion and turbulent Newtonian cooling"
<pre>This directory contains an index.html file with links to the run directories for Figs.1, 2-6 and idl plotting routines with secondary data for the other figures for the paper "Turbulent radiative diffusion and turbulent Newtonian cooling".</pre>
Data for the paper: Critical role of radiative cooling vertical contrast in triggering episodic deluges in small-domain hothouse climates
<p>Data for the paper: Critical role of radiative cooling vertical contrast in triggering episodic deluges in small-domain hothouse climates.</p> <p>The paper has just been submitted, which means this dataset might change before the final publication.</p>
Data and Analysis Files for Simulations of Radiatively-Cooled Magnetic Reconnection on the Z machine
<p>This dataset contains processed simulation data, representative simulation output files, and Python code for analysis of simulations presented in Datta, Rishabh, et al. "Simulations of Radiatively Cooled Magnetic Reconnection Driven by Pulsed Power." J. Plasma Phys. (2024).</p> <p>The simulations were run using GORGON, a radiative resistive MHD code with van Leer advection.<br><br>Details on GORGON can be found in Chittenden et al. (2004) 10.1063/1.1643756, and Ciardi et al. (2007) 10.1063/1.2436479.</p>
Data file needed for modified Lombardi radiative cooling approximation
<p>This is a table containing the equation of state and opacity data required for running Phantom with the radiative cooling approximation introduced in Young et al. (2024). The EoS and opacity calculations are given in Lombardi et al. (2015) and Stamatellos et al. (2007). This method is primarily used to model self-gravitating discs.</p>
Radiative transfer model and datasets for Li et al. (2023), 'Wintertime low-level clouds over sea ice cool the Arctic climate system'
<p>Source code for the radiative transfer model (RAPRAD) and cloud radiative flux data used in the study Li et al. (2022).</p>
Fig. 2 in Keeping cool: Enhanced optical reflection and radiative heat dissipation in Saharan silver ants
Fig. 2. Reflectivity of the silver ant's body surface from the visible to the MIR range of the spectrum. (A) Hemispherical reflectivity measured in the visible and NIR. (B) Measurement and simulation results showing visible and NIR reflectivity as a function of incidence angle. (C) Cross-sectional view of a two-dimensional distribution of a light field (magnitude of electric field component of light,or |E|) around a triangular hair for three exemplary Mie resonances.(D) Schematic diagram showing the interaction between visible and NIR light and a hair at small (I), intermediate (II), and large (III) incidence angles.The corrugated upper two facets may enhancediffuse reflection inthe ultravioletandvisible ranges.(E)ReflectivitymeasuredintheMIRatnormal incidence.(F)Simulated MIRreflectivity asafunction of incidence angle.
Fig.1 in Keeping cool: Enhanced optical reflection and radiative heat dissipation in Saharan silver ants
Fig.1.The bright glare of the silver ant and its structural basis.(A) Silverantoffloadingheatontopofdryvegetation(18).(B)SEMfrontalviewofthehead densely coveredbyhairs.(C)SEMimageof thehairsgraduallytaperingoff towardthetip.(D)Cross-sectionalviewof thehairsmilledwith FIB.(E)SEMimageof two hairs with one flipped upside down to exhibit the flat bottom facet.
Fig.3 in Keeping cool: Enhanced optical reflection and radiative heat dissipation in Saharan silver ants
Fig.3. Resultsof thermodynamicexperiments. (A) Thermal camera images showing the head of an ant specimen at the thermal steady state un- der different conditions. Temporal temperature profiles measured for the head before and after hair removal in vacuum (B) and in still air (C) are shown.(Dto F) Resultsobtained for thehind part (gaster) of an ant specimen.Insets in (B) and (E) are photos of specimens before and after hair removal.In the "hairs intact" picturesof head and gaster, because of the limited solid angle of illumination,the silvery glance is not shown all over the bodysurface portrayed inthe figures.
Satellite-retrieved cloud top radiative cooling data in 2014 over global ocean
<p>Satellite-retrieved cloud-top radiative cooling data in 2014 over global ocean, used in a manuscript submitted to GRL (Zheng et al., 2021, GRL).</p>
Dataset: "Resilience of small PAHs in interstellar clouds: Efficient stabilization of cyanonaphthalene by fast radiative cooling"
<p>Data supporting the article "Resilience of small PAHs in interstellar clouds: Efficient stabilization of cyanonaphthalene by fast radiative cooling"</p>
Raw data for: Rhinarium cooling and sensitivity to thermal radiation in domestic dogs
Open the record for dataset details and reuse information.
Feasibility and Patient Reported Tolerance of Cryotherapy With the Cooral ® Mouth Cooling Device [MCD) in Patients Undergoing Radiation Therapy
ClinicalTrials.gov study NCT04915599. IPD Sharing: Not stated. Countries: 1. Publications: 0.
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