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9 results for “Solar Chemicals”
Solar Chemicals and Fuels - SWOT ANALYSIS
<p>This dataset includes a comprehensive collection of materials and analyses used in the publication "Exploring the SWOTs (Strengths, Weaknesses, Opportunities, and Threats) of Solar Chemicals and Fuels: Findings from a Literature Review and a Workshop Exercise."</p> <p>The dataset consists of a PDF file, with the full-text NVivo coding results, and an Excel file, which contains:</p> <ol> <li>A complete list of documents analyzed, along with their bibliographic information.</li> <li>A compilation table of the SWOT analysis developed after the text-mining exercise and literature review.</li> <li>Word trees retrieved from NVivo.</li> <li>Full quantitative analysis of the NVivo codes and their references.</li> <li>Citation analysis data.</li> <li>Matrix query results on "Policy versus Workshop."</li> </ol>
Galactic chemical evolution of the solar neighborhood, solar twins and exoplanet indicators
<p>Galactic chemical evolution (GCE), solar analogues or twins, and peculiarities of<br> the solar composition with respect to the twins are inextricably related.<br> We examine GCE parameters from the literature and present newly derived values<br> using a quadratic fit that gives zero for a Solar age (i.e. 4.6 Gyr). <br> We show how the GCE parameters may be used not only to ``correct'' abundances<br> to the solar age, but to predict {\bf average} relative elemental <br> abundances as a function of age. <br> We address the question of whether the solar abundances<br> are depleted in refractories and enhanced in volatiles and<br> find that the answer is sensitive to the selection of a<br> representative standard. Our best quality data sets do<br> not support the notion that the Sun is depleted in refractories. <br> A simple model allows us to estimate<br> the amount of refractory-rich material missing from the sun<br> or alternately added to the average solar twin. The model<br> gives between zero and 1.4 earth masses. <br> </p>
From the hot carrier solar cell to the intermediate band solar cell, passing through the multiple-exciton generation solar cell and then back to the hot carrier solar cell: the Dance of the Electro-chemical Potentials
<p>Presentation titled "From the hot carrier solar cell to the intermediate band solar cell, passing through the multiple-exciton generation solar cell and then back to the hot carrier solar cell: the Dance of the Electro-chemical Potentials" given by Antonio Marti at the 36th European PV Solar Energy Conference and Exhibition in Marseille, in September 2019.</p>
Electron concentration profiles calculated using different plasma chemical models during solar X-ray flares
<p>The files contain electron concentration <em>Ne</em> profiles during solar X-ray flares that occurred on 24-25 October 2013 and 9-11 June 2014. The altitude range is 50-90 km.</p> <p>Values of electron concentration were calculated using four-, five- and eight-component models of the ionospheric D-region. Results are obtained on four VLF paths: from European transmitters ICV, FTA, GQD, DHO to Mikhnevo geophysical observatory (55°N 38°E).</p> <p>The data is presented as MATLAB files. Each .mat file contains data and variable "description" with data's structure information.</p>
Dataset of Numerical prediction of changes in atmospheric chemical compositions during a solar energetic particle event on Mars
<p>This dataset contains the input parameters and the simulated results used for figures in the paper "Numerical prediction of changes in atmospheric chemical compositions during a solar energetic particle event on Mars" by Y. Nakamura, F. Leblanc, N. Terada, S. Hiruba, I. Murata, H. Nakagawa, S. Sakai, S. Aoki, A. Piccialli, Y. Willame, L. Neary, A. C. Vandaele, K. Murase, and R. Kataoka.</p> <p>Detailed informations about the data files can be found in "README.txt".</p>
Data for PhD Thesis: "Chemical and electronic structure of Cu$_2$O, NiO, and Cu$_2$O-NiO combinatorial material libraries as hole-transport material for halide perovskite solar cells"
<p>Here, the whole data measured during the PhD time of L. CW. Bodenstein-Dresler + Labbook is uploaded. T data in the "data"-folder was measured at HZB with XPS, UPS and IPES. </p> <p> </p> <p>The PEYS and CPD and XRD data was measured by A. Kama at BIU. </p> <p> </p>
Raw Data for "Chemical etching of Sb2Se3 solar cells: surface chemistry and back contact behaviour"
<p>Raw Data for "Chemical etching of Sb2Se3 solar cells: surface chemistry and back contact behaviour". <br> <a href="https://doi.org/10.1088/2515-7655/ab3c98">https://doi.org/10.1088/2515-7655/ab3c98</a>.</p>
Sonora Cholla: A Grid of Cloud-free, Solar Metallicity Models in Chemical Disequilibrium for the JWST Era
<p>Exoplanet and brown dwarf atmospheres commonly show signs of disequilibrium chemistry. In the James Webb Space Telescope era high resolution spectra of directly imaged exoplanets will allow the characterization of their atmospheres in more detail, and allow systematic tests for the presence of chemical species that deviate from thermochemical equilibrium in these atmospheres. Constraining the presence of disequilibrium chemistry in these atmospheres as a function of parameters such as their effective temperature and surface gravity will allow us to place better constrains in the physics governing these atmospheres.</p> <p>This database contains a grid of cloud-free, solar metallicity atmospheres for brown dwarfs and wide separation giant planets with key molecular species such as CH<sub>4</sub>, H<sub>2</sub>O, CO and NH<sub>3</sub> in disequilibrium. The grid covers atmospheres with T<sub>eff</sub>~[500 K,1300 K], log<em>g</em>~[3.0,5.5] (cgs) and an eddy diffusion parameter of log K<sub>zz</sub>=2, 4 and 7 (cgs). A description of the code and a study of the effect of different parameters within the grid on the temperature and composition profiles of our atmospheres is presented in the accompanying paper "The Sonora Substellar Atmosphere Models. II. Cholla: A Grid of Cloud-free, Solar Metallicity Models in Chemical Disequilibrium for the<em> JWST </em>Era" (accepted to ApJ, Oct. 2021)</p>
Data from: Incorporation of Mn2+ into CdSe quantum dots by chemical bath co-deposition method for photovoltaic enhancement of quantum dot-sensitized solar cells
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Allen Brain Atlas
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DANDI Archive for NWB datasets
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International Brain Laboratory public data
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OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.