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106 results for “Europa”
Evolución de precios de la electricidad en Europa
<p><strong>Este dataset comprende el historial del precio de la electricidad para cada semestre desde el año 2007 hasta el 2021, indicando el coste en euros por kilovatio-hora registrado para los consumidores domésticos de los países que forman la Unión Europea. </strong></p>
europa
<p>COVID-19 data for Europe from 2020-01-03 to 2023-05-03, including cur_hosp, cur_icu, tot_deaths, tot_positive</p> <p>Files:</p> <ul> <li>".pkl" Cache file backup</li> <li>Dataframe exported "PyCoa-DF.csv"</li> <li>Original database backup </li> </ul>
Europa Chaos Block Shapefiles and Geojson Files in Lower RegMap Images
<p>The included dataset includes the raw polygon shapefiles of the outlines for chaos blocks on Europa in the lower half of the RegMap images. The outlines were generated using the standard definitions of blocks and further subdivision in morphology of plates and knobs based on those previously published by Leonard et al. (2022) in which the author of this dataset is the same that created the majority of the Leonard et al. (2022) dataset. Images used to generate the outlines were the RegMap images within the Photogrammetrically Controlled Galileo Image Mosaics of Europa, produced by the USGS Astrogeology (Bland et al., 2021). The shapefiles do not include the entire metadata and will be uploaded at a later date, but information about chaos block morphology, area in sq km, lon/lat location of center, and chaos terrain location are included. Also included within this dataset are the Geojson files (produced by Marina Dunn) that complement the ArcMap shapefiles, so they could be implemented into other programs more easily. Both datasets have yet to be peer reviewed. </p><p> </p><p> </p><p><strong>References</strong></p><p>Leonard, E.J., Howel, S.M., Mills, A., Senske, D.A., Patthoff, D.A., Hay, H.C.F.C., and Pappalardo, R.T. (2022). Finding Order in Chaos: Quantitive Predictors of Chaos Terrain Morphology on Europa, Volume 49, Issue 8, doi: <a href="https://doi.org/10.1029/2021GL097309">10.1029/2021GL097309.</a></p><p>Bland, Michael T., Weller, Lynn A., Archinal, Brent A., Smith, Ethan, Wheeler, Benjamin H. (2021). Improving the Usability of Galileo and Voyager Images of Jupiter's Moon Europa, Earth and Space Science, Volume 8, Issue 12, doi: <a href="https://doi.org/10.1029/2021EA001935">10.1029/2021EA001935</a>.</p>
Vedlegg til "Endonymiprinsippet og flerspråklige stedsnavn i Europa"
<p>The dataset consists of one PDF document and one spreadsheet workbook, which contain the complete results of the article "<a href="https://ojs.novus.no/index.php/NON/article/view/2343">Endonymiprinsippet og flerspråklige stedsnavn i Europa</a>" [The endonymic principle and plurilingual toponyms in Europe].</p> <p>Explanations and references are provided in the PDF. All text is in Norwegian, but the maps in Appendix 1 of the PDF (pp. 34–45) are intelligible without knowledge of Norwegian. They show the geographic distribution of regional and minority languages in Europe (most recent estimates available of standardised languages). In several cases, distributions should be regarded as approximate, partly because no detailed or recent estimates are available, partly because coloured areas follow administrative borders (provinces, municipalities etc.), which are not always congruent with linguistic borders. Countries are abbreviated following ISO 3166-1 (two uppercase letters), languages following ISO 639-2/T or ISO 639-3 (three lowercase letters). Please note that national languages, which are emphasised using boldface, did not normally get a colour of their own, so that the light grey background colour can represent different languages in different countries. Also the remaining colours may represent different languages, but the same language has always the same colour. The intensity of a colour indicates the proportion of users of the language in the local population (using three intervals: 5%–25%, 25%–50% og 50%–100%).</p>
Supporting Data - Double Ridge Formation over Shallow Water Sills on Jupiter's Moon Europa
<p>This archive contains data produced in support of R. Culberg, D. M. Schroeder, G. Steinbrügge, Double Ridge Formation Over Shallow Water Sills on Jupiter’s Moon Europa, <em>Nature Communications</em>, 2022. This includes the WorldView imagery in Figure 1, the reprocessed radargrams underlying the radar analysis and inversion, and outputs of all inversion and sensitivity test runs. See the README file for a complete description of the files available in this archive.</p>
Data for "Constraints on the Observability of Energetic Neutral Atoms from the Magnetosphere-Atmosphere Interactions at Callisto and Europa" by Haynes et al.
<p>Accompanying data products for publication entitled "Constraints on the Observability of Energetic Neutral Atoms from the Magnetosphere-Atmosphere Interactions at Callisto and Europa". The manuscript was submitted to JGR Space Physics shortly after upload.</p> <p>Data includes all simulation outputs that are depicted in this work, both for the AIKEF hybrid model (i.e., Figure 4) and the model used to produce synthetic ENA images (Figures 3, 6, 8, 9, 11, A1, and B1). All other figures in the work are used for illustrative purposes and were not generated with simulation output. </p> <p>Information regarding the organization and file structure can be found in H24_data_readme.txt , as well as which dataset corresponds to which figure. Any inquiries, questions, or comments may be addressed through the email associated with this data publication.</p>
Torre de la Sal, Cabanes, Castellón, Comunitat Valenciana, España, Europa │Proyecto de digitalización 3D, 2D
<p>Proyecto de digitalización gráfico y geomático 2D y 3D realizado por <strong>AD&D 4D </strong>cofinanciado por Generalitat Valenciana.</p> <p>Torre de la Sal se localiza en el poblado marítimo de Torre la Sal, en las inmediaciones del <strong>Parque Natural del Prat de Cabanes-Torreblanca.</strong></p> <p>La Torre de la Sal es una torre defensiva de la costa castellonense, construida entre los siglos XIV y XVI. Junto a ésta, en la <strong>Ribera de Cabanes</strong> (Castellón) existe una red de torres fortificadas: la Torre del Carmen, la Iglesia Fortificada de Albalat y las torres dels Gats y Carmelet. Estas cinco torres son un aliciente cultural y turístico, señalizadas desde Cabanes en la Ruta de las Torres.</p> <p> </p> <ul> <li>Nube de puntos georreferenciada 23 Millones Ptos <strong>Ref</strong>: <a href="https://zenodo.org/api/files/253a316b-aad0-495d-8a54-1afe8bc1b46a/2020TorreLaSalNPD23M.zip">2020TorreLaSalNPD23M.zip </a></li> <li>Modelo digital de elevaciones 2 mm. pixel <strong> Ref</strong>: <a href="https://zenodo.org/api/files/253a316b-aad0-495d-8a54-1afe8bc1b46a/2020TorreDeLaSalDEM2mm.7z">2020TorreDeLaSalDEM2mm.7z </a></li> <li>Modelo 3D Georreferenciado 46 Millones de polígonos <strong>Ref</strong>:<a href="https://zenodo.org/api/files/253a316b-aad0-495d-8a54-1afe8bc1b46a/2020TorreDeLaSalDEM2mm.7z">2020TorreDeLaSalDEM2mm.7z </a></li> </ul> <p> </p> <p>Más información: <a href="https://www.castellonarqueologico.es/yacimientos/la-plana-i/torre-de-la-sal/">Español</a> - <a href="https://www.castellonarqueologico.es/va/yacimientos/la-plana-i/torre-de-la-sal/">Valencià</a> - <a href="https://www.castellonarqueologico.es/en/yacimientos/la-plana-i/torre-de-la-sal/">English</a></p> <p> </p> <p><a href="https://www.castellonarqueologico.es/yacimientos/la-plana-i/torre-de-la-sal/3d.html">Modelo 3D</a> │Sketchfab - Online</p> <p><a href="https://www.pointbox.xyz/clouds/5f6315c09cad5d2317eeacc1">Nube de Puntos</a> (Point Cloud) │ Point Box -Online</p> <p> </p> <p>Sistema de referencia geodésico:.<strong>ETRS 89 UTM 31 (EPSG 25831)</strong></p> <p>Altitudes Ortométricas referidas al nivel medio del mar de Alicante.</p> <p>Modelo de Geóide <strong>EGM08</strong> con sobrecorreción de nivelación.</p>
Abb. 3 in Hornmilben (Acari, Oribatida) aus dem Europa-Schutzgebiet Zurndorfer Eichenwald (Burgenland, Österreich)
Abb. 3: Hornmilben (Acari, Oribatida) vom Zurndorfer Eichenwald, Gemeinsame Arten mit umliegenden Gebieten (Quellen vgl. Text).
Juno Plasma Wave Observations at Europa
<p>This is the supporting data set for the paper by the same title published in AGU JGR Space Physics.</p><p><strong>Abstract</strong><br>Juno passed by Europa at an altitude of 355 km on 29 September, day 272, 2022. As one of Juno's in situ science instruments, the Waves instrument obtained observations of plasma waves that are essential contributors to Europa's interaction with its environment. Juno observed chorus, a band at the upper hybrid frequency providing the local plasma density, and electrostatic solitary structures in the wake. In addition, impulses due to micron-sized dust impacts on Juno were recorded with a local maximum very close to Europa. The peak electron density near Europa was ∼ 330 cm−3 while the surrounding magnetospheric density was in the range of 50 to 150 cm−3. There was a significant separation between the Europa flyby and Juno's crossing of Jupiter's magnetic equator, enabling a unique identification of effects associated with the moon as opposed to magnetospheric phenomena normally occurring at the magnetic equator near 10 Jovian radii.</p>
Europa spectral images of HCN, SO2, H2CO and CH3OH observed using ALMA
<p>This dataset contains observations of Europa carried out using the Atacama Large Millimeter/submillimeter Array (ALMA) on four dates in 2021, using the Band 7 receiver. The targeted spectral lines included HCN ($J=4-3$; 354.505 GHz), H$_2$CO ($J_{K_a,K_c}=5_{1,5}-4_{1,4}$; 351.769 GHz), SO$_2$ ($J_{K_a,K_c}=5_{3,3}-4_{2,2}$; 351.257 GHz), observed at 122~kHz resolution, and CH$_3$OH ($J_K = 4_0 - 3_{-1}\ E$; 350.688 GHz), observed at 61 kHz resolution. The interferometric data were cleaned and imaged using CASA, with a pixel size of 0.02'' and a clean mask of 1.1''. The resulting spatial resolution is ~0.15 arcseconds.</p> <p>The data includes FITS image cubes and PDF spectral maps for each molecule, on each observing date. See FITS headers for further details. For each PDF, the ALMA beam FWHM is indicated lower left (dot-dashed ellipse); upper right axes show physical distances in the plane of the sky, while lower left axes show the spectral units for each sub-panel.</p>
Figs. 7a y b in Sobre la posición taxonómica de Dicronychus wagneri (PečírKA, 1926)¡ presencia del género Ryukyucardiophorus Ôhira, 1973 en la Península Ibérica y Europa (Coleoptera¡ Elateridae¡ Cardiophorinae).
Figs. 7a y b.- Escutelo de forma pentagonal. Fig. 8.- Antena testácea. Figs. 9a y b.- Uñas con dentículo poco desarrollado en su base.
Figs. 1-2 in Sobre la posición taxonómica de Dicronychus wagneri (PečírKA, 1926)¡ presencia del género Ryukyucardiophorus Ôhira, 1973 en la Península Ibérica y Europa (Coleoptera¡ Elateridae¡ Cardiophorinae).
Figs. 1-2.- Habitus de los dos ejemplares ahora incluidos en el género Ryukyucardiophorus Ôhira, 1973, depositados en el Museo Nacional de Ciencias Naturales de Madrid.
Fig. 6 in Monoxia obesula Blake, 1939 (Coleoptera: Chrysomelidae) en Europa continental.
Fig. 6.- Distribución actual conocida de Monoxia obesula Blake, 1939 en Europa. Los puntos azules indican los registros previos; los puntos de color rojo indican los registros recientes que se comunican en este trabajo. Se adjunta, a la izquierda, un mapa más detallado de la Comunitat Valenciana donde se precisan las localidades de observación.
Fig. 5 in Monoxia obesula Blake, 1939 (Coleoptera: Chrysomelidae) en Europa continental.
Fig. 5.- Aspecto de varios arbustos ornamentales de Atriplex halimus, gravemente afectados por el ataque de Monoxia obesula Blake, 1939. Población de Burjassot (Valencia), julio de 2017 (Fotografía: S. Montagud).
Dataset for "Finding order in chaos: Quantitative predictors of chaos terrain morphology on Europa"
<p>Dataset S1 contains two shapefiles containing the chaos borders (ChaosBordersShapefiles.zip) and each block mapped (AllBlocksShapefiles.zip), and a text file that contains the total area (km<sup>2</sup>) of each mapped chaos terrain and the area (km<sup>2</sup>) of every block we mapped within each chaos terrain in the manuscript "Finding order in chaos: Quantitative predictors of chaos terrain morphology on Europa".</p>
Fig. 2.- A in A second record for mainland Europe of Actebia (Parexarnis) photophila (Guenée, 1852) (Lepidoptera: Noctuidae: Noctuini) Un segundo registro para Europa continental de Actebia (Parexarnis) photophila (Guenée, 1852) (Lepidoptera: Noctuidae: Noctuini)
Fig. 2.- A. (P.) photophila, Tarifa, Cádiz, 23/4.05.2022. Set specimen. Fig. 2.- A. (P.) photophila, Tarifa, Cádiz, 23/4.05.2022. Ejemplar fijado.
Figs. 1-3 in Second record for Europe of Agrotis subspinifera (Hampson, 1903) (Lepidoptera: Noctuidae: Noctuinae). Segundo registro para Europa de Agrotis subspinifera (Hampson, 1903) (Lepidoptera: Noctuidae: Noctuinae).
Figs. 1-3.- Agrotis subspinifera (Hampson, 1903), macho (Tarifa, Cádiz). 1-2.- Diferentes tomas del ejemplar, desde distintos ángulos. 3.- Detalle de la antena derecha.
Coordinates of cycloids on Europa
<p>Supporting information for: Poinelli, M., Larour, E., Castillo-Rogez, J., & Vermeersen, B. (2019). Crevasse propagation on brittle ice: Application to cycloids on Europa. <em>Geophysical Research Letters</em>, 46, 1–8. https://doi.org/10.1029/2019GL084033</p> <p>The file called Cycloids.csv includes coordinates of 4 cycloids on the surface of the Jovian moon Europa.<br> Europa reference radius is 1562 km.</p> <p>Latitude and longitude are in degrees.<br> Latitude type is planetocentric. Longitude direction is positive west while longitude domain is: 0 to 360.</p>
Geologic Map of Tyre Impact Crater on the Galilean Moon Europa - Digitized and Modified Versions (2024)
<p><strong>Geologic Map of Tyre Impact Crater on the Galilean Moon Europa - Digitized and Modified Versions (2024)</strong></p> <p>Files and deliverable documentation of the process of digitizing the geologic map of Tyre, Kadel et al. 2000. This may be useful if you are looking to learn how to digitize a geologic map using some form of mapping software, or to learn about the surface geology of Jupiter's icy moon Europa. </p> <p>Includes:</p> <ul> <li>read.me with supporting information</li> <li>map package</li> <li>Georeferenced PDF figures </li> <li>Shapefiles </li> </ul>
A Metamorphic Origin for Europa's Ocean - Supplementary Data Files
<p><strong>A Metamorphic Origin for Europa's Ocean - Supplementary Data Files</strong><br> M. Melwani Daswani, S. D. Vance, M. J. Mayne, and C. R. Glein<br> Jet Propulsion Laboratory, California Institute of Technology<br> daswani@jpl.nasa.gov</p> <p>2021-08-18</p> <p>This folder contains the Supplementary Data files consisting of input data and output data products. The paper is accepted in Geophysical Research Letters. A preprint may be found here: <a href="https://doi.org/10.1002/essoar.10507048.1">https://doi.org/10.1002/essoar.10507048.1</a>, but please see the article on Geophysical Research Letters for the properly formatted, peer-reviewed, revised version.</p> <p><strong>Contents:</strong></p> <p><strong>AccretR Europa MC-Scale composition output.xlsx</strong><br> Contains the composition of Europa after accretion, obtained by running the AccretR program. AccretR can be found on Zenodo: https://doi.org/10.5281/zenodo.3827540 or GitHub (most up to date): https://github.com/mmelwani/AccretR</p> <p><br> <strong>Fe-S core composition models</strong><br> Contains the Perple_X input and output files for constraining the composition of the Fe+-S core. Thermodynamic data used was from Saxena and Eriksson (2015), also included as a Perple_X thermodynamic file.</p> <p><br> <strong>Rcrust prograde metamorphism models</strong><br> Contains the input and output files for the Rcrust models, which are the metamorphic prograde path thermodynamic. Rcrust is required to run these models<br> (http://www.sun.ac.za/english/faculty/science/earthsciences/rcrust), as well as the "meemum" program from Perple_X (https://www.perplex.ethz.ch/). The Perple_X version used was "6.8.7", and was compiled from source to enable 12 thermodynamic components (i.e. major elements).</p> <p><br> <strong>CHIM-XPT ocean column composition models</strong><br> Contains the CHIM-XPT input and output files, which model the ocean composition from seafloor to surface, including precipitated minerals, aqueous solutes and saturated gases. Inputs for these models were the fluids extracted from the Rcrust prograde metamorphic models.</p> <p><strong>Density and volume of clathrates.xlsx</strong><br> Shows the calculations carried out to find the temperature, density and volume of CO2 clathrates in Europa's ocean.</p>
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OpenNeuro
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