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105 results for “Ero”

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zenodo40/100

Spherical harmonic models of the shape of (433) Eros

<p>This archive contains two spherical harmonic models of the shape of asteroid 433 Eros. One model is based on laser altimetry from the instrument NLR and the other is based on a stereo photoclinometry shape.</p> <p>The data used to generate the model based on laser altimetery were taken from the file <code>nlr125ar.img</code> on <a href="https://sbnarchive.psi.edu/pds3/near/NEAR_A_NLR_6_EROS_MAPS_MODELS_V1_0/data/img/">NASA's PDS website</a>. This image file was first converted to netcdf format using the <a href="https://www.generic-mapping-tools.org/">generic-mapping-tools</a> function <code>xyz2grd</code>, and the resulting pixel registed map was then converted to a gridline registration using the function <code>grdsample</code>. Following this, the resulting netcdf file was read into the <a href="https://shtools.github.io/SHTOOLS/index.html">pyshtools</a> software and expanded into spherical harmonics using the function <code>SHCoeffs.expand()</code>. The spherical harmonic functions were chosen to be "4pi" normalized and to exclude the Condon-Shortley phase factor of (-1)<sup>m</sup>. The units of the coefficients are meters.</p> <p>The data used to generate the model based on the stereo photoclinometric shape model were taken from the file&nbsp;<code>quad512q.tab</code> on <a href="https://sbnarchive.psi.edu/pds4/non_mission/gaskell.ast-eros.shape-model_V1_1/data/quad/">NASA's PDS website</a>. The vertices from the ICQ shape model with Q=512 were first converted from Cartesian to spherical coordinates, from which a regular gridline registered netcdf file was created using the&nbsp;<a href="https://www.generic-mapping-tools.org/">generic-mapping-tools</a> function <code>surface</code> with a tension of 0.6 and with a grid spacing of 0.17578125 degrees. This file was then read into the <a href="https://shtools.github.io/SHTOOLS/index.html">pyshtools</a> software and expanded into spherical harmonics in the same manner as the NLA based model.</p> <p>The two files in this archive are</p> <ul> <li>Eros_NLR_shape_719.bshc.gz</li> <li>Eros_SPC_shape_511.bshc.gz</li> </ul> <p>The numbers 719 and 511 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 8 and ~5.7 pixels per degree, respectively. The files are stored in the binary "bshc" format as described in the pyshtools documentation and are furthermore compressed using gzip.</p>

opencc-by-4.0Mar 2024View details →
zenodo40/100

FIGURE 14. Chancelloria eros Walcott, 1920 in Chancelloriids of the Cambrian Burgess Shale

FIGURE 14. Chancelloria eros Walcott, 1920 (1, 2), and C. cf. eros (3–5), ST. 1. ROM 49574, dry. 2. ROM 49572, dry. 3–5. ROM 49576, dry. Items 4 and 5 show details of the upper and lower portions, respectively, of 3.

opencc-by-4.0Feb 2015View details →
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FIGURE 10. Chancelloria eros Walcott, 1920. ROM 62534 in Chancelloriids of the Cambrian Burgess Shale

FIGURE 10. Chancelloria eros Walcott, 1920. ROM 62534, RT. 1. Wet. 2. Detail of 1 (position marked by frame), wet. Note the common presence of 3+0 Allonnia-type sclerites (arrows) in a scleritome dominated by 5–7+1 Chancelloria- type sclerites.

opencc-by-4.0Feb 2015View details →
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FIGURE 9. Chancelloria eros Walcott, 1920. 1–3. ROM 57604 in Chancelloriids of the Cambrian Burgess Shale

FIGURE 9. Chancelloria eros Walcott, 1920. 1–3. ROM 57604, BW -130. Specimens of the lingulate brachiopod Acrothyra gregaria appear to be attached to the spines of the Chancelloria. The brachiopods are concentrated to what is interpreted as the apical part of the chancelloriid body. 1. Wet. 2. Detail of 1 (position marked by frame), dry. 3. Detail of 2 (position marked by frame), dry. 4. ROM 63055, ST, dry.

opencc-by-4.0Feb 2015View details →
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FIGURE 11. Chancelloria eros Walcott, 1920. ROM 49599A in Chancelloriids of the Cambrian Burgess Shale

FIGURE 11. Chancelloria eros Walcott, 1920. ROM 49599A, RQ 8.0. Arrows point to examples of 3+0 sclerites. 1. Dry. 2. Detail of 1 (position marked by frame), dry.

opencc-by-4.0Feb 2015View details →
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FIGURE 8. Chancelloria eros Walcott, 1920. 1, 2. ROM 49580 in Chancelloriids of the Cambrian Burgess Shale

FIGURE 8. Chancelloria eros Walcott, 1920. 1, 2. ROM 49580, ST. 1. Dry. 2. Detail of 1 (position marked by frame), dry. 3. ROM 62590, ST, dry.

opencc-by-4.0Feb 2015View details →
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FIGURE 7. Chancelloria eros Walcott, 1920. ROM 62588B in Chancelloriids of the Cambrian Burgess Shale

FIGURE 7. Chancelloria eros Walcott, 1920. ROM 62588B, BW -320. 1. Dry. 2. Detail of 1 (position marked by frame), dry. 3. Detail of 1 (position marked by frame), wet.

opencc-by-4.0Feb 2015View details →
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FIGURE 5. Chancelloria eros Walcott, 1920. 1. ROM 62538 in Chancelloriids of the Cambrian Burgess Shale

FIGURE 5. Chancelloria eros Walcott, 1920. 1. ROM 62538, ST talus, wet. Arrow points to empty area that may represent an apical orifice. 2. Detail of 1 (position marked by frame), wet. 3. ROM 62535A, BW -300, dry.

opencc-by-4.0Feb 2015View details →
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FIGURE 6. Chancelloria eros Walcott, 1920. ROM 62539 in Chancelloriids of the Cambrian Burgess Shale

FIGURE 6. Chancelloria eros Walcott, 1920. ROM 62539, BW -320. 1. Dry. 2. Detail of 1 (position marked by frame), wet.

opencc-by-4.0Feb 2015View details →
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FIGURE 1. Chancelloria eros Walcott, 1920 in Chancelloriids of the Cambrian Burgess Shale

FIGURE 1. Chancelloria eros Walcott, 1920, lectotype, USNM 66524. Figured by Walcott (1920) as pls 86:2 and 88:1f. 1. Wet. 2. Dry, coated with ammonium chloride. Detail of 1 (position marked by frame). 3. Dry, coated with ammonium chloride. Detail of 2 (position marked by frame). Top arrow (grey): 4+0 sclerite. Middle arrow (black): 7+1 sclerite, preserved in negative relief (ascending ray towards the viewer). Bottom arrow (white): 7+1 sclerite, preserved in positive relief (ascending ray pointing away from the viewer).

opencc-by-4.0Feb 2015View details →
zenodo36/100

Эрот с петухом/ Eros with Rooster

Эрот с петухом Древняя Греция, I в. н. э. Терракота Коллекция А.Пальникова МИПУ ХФ 3034 Музей истории Пермского университета Eros with Rooster Ancient Greece, I century A.D. Terracotta Collection of A.Palnikov МИПУ ХФ 3034 Perm University History Museum Source: Objaverse 1.0 / Sketchfab

opencc-byMay 2017View details →
zenodo36/100

Weihrelief (Aphrodite und Eros am Altar)

ID: MKGHamburg 1986.60 <br> Title: Votive stele for Aphrodite <br> Object type: votive stelai, relief <br> Origin: Corinthian (?); Perachora (?) <br> Date/Period: c. 375-350 BC <br> Material: marble <br> Measurements: 137,5cm (heights); 28.3 cm (width) <br> Museum/Collection: Museum für Kunst und Gewerbe Hamburg Inv. 1986.60 <br> MKGHamburg: [dc00126829](https://sammlungonline.mkg-hamburg.de/de/object/Weihrelief-Aphrodite-und-Eros-am-Altar/1986.60/dc00126829?s=1986.60&amp;h=0) The research for this 3D object was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany´s Excellence Strategy – EXC 2176 'Understanding Written Artefacts: Material, Interaction and Transmission in Manuscript Cultures', project no. 390893796. The research was conducted within the scope of the Centre for the Study of Manuscript Cultures (CSMC) at Universität Hamburg. Source: Objaverse 1.0 / Sketchfab

opencc-zeroJun 2021View details →
zenodo36/100

3D Eros Ehrenberg Collection

Statuette of Eros, bronze, with fillet in hair and quiver. Arms and feet broken off. Hellenistic, Anatolia, 2nd cent. B.C. Height: 9 1/2 cm = 3 3/4 ". Bought for 22£ Source: Objaverse 1.0 / Sketchfab

opencc-byJul 2022View details →
zenodo36/100

Eros

Eros bowman, roman copy from greek original from the 4th century BCE, Spain (?), marble. Musée du Cinquentenaire (Brussels, Belgium). Made with ReMake and ReCap from AutoDesk. The young Eros, originally winged, is represented with his bow. This is probably a Roman copy from an copy from Eros sculpture in Brass from Lysippe had sculpted for the Thespies sanctuary between 338 and 335 BCE. For more updates, please follow @GeoffreyMArchal on Twitter. Source: Objaverse 1.0 / Sketchfab

opencc-byJun 2017View details →
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FIGURE 13. Chancelloria eros Walcott, 1920. 1. ROM 49578 in Chancelloriids of the Cambrian Burgess Shale

FIGURE 13. Chancelloria eros Walcott, 1920. 1. ROM 49578, ST, dry. 2. ROM 43126, ST, dry.

opencc-by-4.0Feb 2015View details →
zenodo32/100

Vaso (K´ero) de estilo Tiwanaku

Source: Objaverse 1.0 / Sketchfab

opencc-byJun 2019View details →
zenodo32/100

Vaso (K´ero) de estilo Tiwanaku

Source: Objaverse 1.0 / Sketchfab

opencc-byJun 2019View details →
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Figs. 39-40. Ero comoremis Emerit, 1996 in New species and interesting new records of spiders from Seychelles (Arachnida, Araneaea)

Figs. 39-40. Ero comoremis Emerit, 1996: - 39: Abdomen of female dextrolaterally. - 40: Epigyne ventrally. - Scale bars: 39 = 1.0,40 = 0.2 mm. Orig.

opennotspecifiedDec 2002View details →
zenodo32/100

Vaso (K´ero) de estilo Tiwanaku

Source: Objaverse 1.0 / Sketchfab

opencc-byJun 2019View details →
zenodo32/100

Translated spherical harmonic gravitational field models for Phobos and 433 Eros

<p>The dataset contains the spherical harmonic gravitational field models for the Martian moon Phobos and the asteroid 433 Eros, which are translated from the original models derived in the respective coordinate systems.</p> <p>The gravity model files contain the normalized spherical harmonic coefficients in the standard format in the folder "gravity". The files named with the prefix "sphcfs\_" are for: 1. base models tied to the respective shape models of Phobos and Eros; 2. four translated models for the northern and southern halves of Phobos and Eros. The models are derived via boundary-value problems. The translated models are each accompanied by an analytically transformed model for comparison. The corresponding data files are identified with the prefix "tsphcfs\_".</p> <p>The triangulated shape model for Phobos interpolated using the spherical harmonic series by Willner et al. (2014), Planetary and Space Science, vol. 102, pp. 51-59, DOI:10.1016/j.pss.2013.12.006 is given in the ".obj" format. The shape model for Eros by Thomas et al. (2002), Icarus, vol. 155, pp. 18-37, DOI:10.1006/icar.2001.6755 used in the study belongs to the ``NEAR Collected Shape and Gravity Models'' (NEAR-A-5-COLLECTED-MODELS-V1.0) at https://sbn.psi.edu/pds/resource/nearbrowse.html (retrieved in Mar. 2024), and is not included. The dissected shape models are provided for both objects, which are used for model evaluation over the northern and southern halves of the bodies.</p> <p>The parameters of the Brillouin spheres are provided in the folder "sphere".</p> <p>The numerical results in the folder "result" are modeled gravitational potentials alongside the true values around and on the surface of the bodies. The results for the ellipsoidal harmonic models are provided for comparison.</p>

opencc-by-4.0Mar 2024View details →

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