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30 results for “Mola mola”
Spherical harmonic models of the shape of Mars [MOLA]
<p>This archive contains four spherical harmonic models of the shape of Mars truncated at different maximum spherical harmonic degrees. The highest resolution model has a maximum spherical harmonic degree of 5759, which was generated from a Mars shape model sampled at 64 pixels per degree.</p> <p>The data used to generate these models are from the MOLA instrument on the Mars Global Surveyor spacecraft, as found in the files <code>MEGR00N000GB.IMG</code>, <code>MEGR00N180GB.IMG</code>, <code>MEGR90N000GB.IMG</code> and <code>MEGR90N180GM.IMG</code> on <a href="https://pds-geosciences.wustl.edu/mgs/mgs-m-mola-5-megdr-l3-v1/mgsl_300x/meg064/">NASA's PDS website</a>. These four image files were first converted to netcdf format using the <a href="https://www.generic-mapping-tools.org/">generic-mapping-tools</a> function <code>xyz2grd</code>, and then turned into a single file using the function <code>grdpaste</code>. 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 four files in this archive are</p> <ul> <li>Mars_MOLA_shape_5759.bshc.gz</li> <li>Mars_MOLA_shape_2879.bshc.gz</li> <li>Mars_MOLA_shape_1439.bshc.gz</li> <li>Mars_MOLA_shape_719.bshc.gz</li> </ul> <p>The numbers 5759, 2879, 1439, and 719 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 64, 32, 16, and 8 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. The lower resolution models were generated by truncating the spherical harmonic coefficients of the highest resolution model.</p> <p>These models supercede <a href="../records/3870922">Spherical harmonic model of the shape of Mars: MarsTopo2600</a> and <a href="../records/6475460">Spherical harmonic model of the shape of Mars: MarsTopo719</a>.</p>
Fig. 3 in Molecular and Morphological Identification of Mola Sunfish Specimens (Actinopterygii: Tetraodontiformes: Molidae) from the Indian Ocean
Fig. 3. Photographs of the clavus of the two specimens of Mola sp. A from Oman (A: OMMSFC 1085; B: OMMSTC 1097). Solid arrows indicate clavus fin rays. Open arrows indicate ossicles. The double-headed arrow indicates the width of the smooth band. Question marks indicate unclear ossicles.
Fig. 4 in Molecular and Morphological Identification of Mola Sunfish Specimens (Actinopterygii: Tetraodontiformes: Molidae) from the Indian Ocean
Fig. 4. Specimens of Mola sp. A as illustrated in earlier literature. A, OMMSFC 1085, 91.6 cm TL, fig. 1 (fresh) in Jawad et al. (2012); B, OMMSTC 1097, 135.0 cm TL, fig. 1 (fresh) in Jawad (2013); C, KMNH VR 100,123, 325.0 cm TL, fig. 2C (stuffed) in Sawai et al. (2015). Arrows indicate bumps developing with age. Scale bars: 10 cm. Redrawn with permission from Jawad et al. (2012), Jawad (2013), and Sawai et al. (2015).
Fig. 1 in Molecular and Morphological Identification of Mola Sunfish Specimens (Actinopterygii: Tetraodontiformes: Molidae) from the Indian Ocean
Fig. 1. Correspondence between species names of Mola sunfishes in previous studies. The dotted arrows indicate unclear relationships, while the solid arrows indicate clear relationships.
Fig. 5. Metynnis mola spermatozoa. A and B in Spermiogenesis and spermatozoa ultrastructure in the Serrasalminae (Ostariophysi: Characiformes) with further evidence on the relationships of the piranhas and pacus
Fig. 5. Metynnis mola spermatozoa. A and B - Spermatozoa in longitudinal sections. C and D - Longitudinal sections of the nuclear fossa region. E to H - Midpiece in cross sections. I - Flagellum in longitudinal section. J, K and L - Flagella in cross sections. Scale bars, A = 0.6 µm; B = 0.55 µm; C = 0.4 µm; D = 0.35 µm; E= 0.5 µm; F = 0.4 µm; G = 0.35 µm; H = 0.25 µm; I = 0.35 µm; J - K = 0,15 µm; L = 0.1 µm. A: axoneme; C: centriole; D: distal centriole; F: flagellum; M: mitochondria; N: nucleus; P: proximal centriole; V: vesicle; Asterisk: tubule-vesicular compartment; Arrow: electron dense material; Arrowhead: cytoplasmic canal; Double arrow: nuclear fossa; Star: cytoplasmic sleeve.
Figure 1 in First record of a rare sunfish, Mola mola (Linnaeus, 1758) from coastal waters of West Bengal, India
Figure 1. Mola mola (Linnaeus 1758), MARC/ZSI/F4629, 780 mm.
Figure 1 in Coris julis cleaning a Mola mola, a previously unreported association
Figure 1. - Location of the observation in La Herradura, Spain.
FIGURE 4 in Response to Britz (2022) regarding the validity of the giant sunfish Mola alexandrini (Ranzani, 1834) (Teleostei: Molidae)
FIGURE 4. Preservation status and labels of two specimens of the genus Mola in the Museo di Zoologia dell' Università di Bologna, Italy (December 2013). (A) putative holotype of Mola alexandrini (PHMA) hanging on the museum wall; (B) the specimen label of the PHMA specimen; (C) holotype of Ozodura orsini in a glass display case; (D) The specimen label of the holotype of Oz. orsini.
FIGURE 2 in Response to Britz (2022) regarding the validity of the giant sunfish Mola alexandrini (Ranzani, 1834) (Teleostei: Molidae)
FIGURE 2. Similarities between (A) the bulgy clavus edge of the putative holotype of Mola alexandrini (PHMA) specimen at the Museo di Zoologia dell' Università di Bologna (MZUB), and (B) the clavus edge on the illustration of the holotype of Orthragoriscus alexandrini in Ranzani (1839a). Arrows indicate the bulgy edge of the clavus; red enclosures indicate the area of comparison.
FIGURE 1 in Response to Britz (2022) regarding the validity of the giant sunfish Mola alexandrini (Ranzani, 1834) (Teleostei: Molidae)
FIGURE 1. Specimens of the genus Mola preserved in the Museo di Zoologia dell' Università di Bologna, Italy (MZUB). (A) extant putative holotype of Mola alexandrini (PHMA); (B) holotype of Orthragoriscus alexandrini illustrated by Ranzani (1939); (C) extant holotype of Ozodura orsini [designated by Sawai et al. (2018) as neotype of Mola mola]; (D) holotype of Oz. orsini illustrated by Ranzani (1939). Arrows indicate the open part of the gill slit (white crescent; see text).
FIGURE 3 in Response to Britz (2022) regarding the validity of the giant sunfish Mola alexandrini (Ranzani, 1834) (Teleostei: Molidae)
FIGURE 3. Illustration of the specimens of the genus Mola from (A) Swainson (1839), and (B) Storer (1839).
Fig. 2 in Molecular and Morphological Identification of Mola Sunfish Specimens (Actinopterygii: Tetraodontiformes: Molidae) from the Indian Ocean
Fig. 2. The phylogenetic placements of the two specimens from Oman in the neighbor-joining tree of Mola species inferred from D-loop sequences available in the DDBJ/EMBL/GenBank databases. The Omani specimens are shown in bold. The numbers beside branches indicate bootstrap values (values of less than 50% and those within the Mola sp. B and Mola sp. C clades are not shown). The scale indicates expected nucleotide substitutions per site.
Molae de ladrillo del Torcularium de villaricos
Molino rotatorio cilindrico Info: http://aespa.revistas.csic.es/index.php/aespa/article/view/532/528 Source: Objaverse 1.0 / Sketchfab
MOLA MISSION EXPERIMENT GRIDDED DATA RECORD
The Mars Global Surveyor spacecraft includes a laser altimeter instrument. The primary objective of the Mars Orbiter Laser Altimeter (MOLA) is to determine globally the topography of Mars at a level suitable for addressing problems in geology and geophysics. The MOLA Experiment Gridded Data Record (EGDR) is a topographic map of Mars based on altimetry data acquired by the MOLA instrument and accumulated over the course of the mission. The Mission Experiment Gridded Data Record (MEGDR), consists of data accumulated over the whole primary mission.
MOLA PRECISION EXPERIMENT DATA RECORD
The Precision Experiment Data Record (PEDR) archive contains Mars Global Surveyor (MGS) Mars Orbiter Laser Altimeter (MOLA) science mode telemetry data that has been converted to engineering and physical units.
MOLA INITIAL EXPERIMENT GRIDDED DATA RECORD
The IEGDR product is a global map of planetary radius, areiod,topography, and number of observations, derived from MOLA PEDR products and aggregated into latitude-longitude bins. The IEGDR is released in two formats, an ASCII table and an image. The table (this data set) has one row for each latitude-longitude bin, from 90 to -90 degrees latitude and from 0 to 360 degrees longitude. Values for planetary radius, areoid, topography, and number of observations per bin are stored as columns in the table.
MOLA SPHERICAL HARMONICS TOPOGRAPHY MODEL
The Mars Global Surveyor spacecraft included a laser altimeter instrument. The primary objective of the Mars Orbiter Laser Altimeter (MOLA) is to determine globally the topography of Mars at a level suitable for addressing problems in geology and geophysics.
MOLA PRECISION EXPERIMENT DATA RECORD ASCII TABLES
The Mars Global Surveyor spacecraft included a laser altimeter instrument. The primary objective of the Mars Orbiter Laser Altimeter (MOLA) is to determine globally the topography of Mars at a level suitable for addressing problems in geology and geophysics.
MOLA AGGREGATED EXPERIMENT DATA RECORD
The MOLA AEDR data set contains the raw altimetry measurements acquired by the Mars Orbiter Laser Altimeter on the Mars Global Surveyor spacecraft. The AEDR data are used as input to the MOLA Precision Experiment Data Record (PEDR) data set, in which the altimetry data have been corrected according to precise measurements of the orbit. The PEDR data set is preferred for science analysis.
MOLA INITIAL EXPERIMENT GRIDDED DATA RECORD
The Mars Global Surveyor spacecraft included a laser altimeter instrument. The primary objective of the Mars Orbiter Laser Altimeter (MOLA) is to determine globally the topography of Mars at a level suitable for addressing problems in geology and geophysics.
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Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
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DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
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.