Skip to main content
Powered by ShareScore

Find research datasets worth reusing

Search datasets from major research repositories and use ShareScore to quickly assess how well each record supports discovery, access, and reuse.

430

datasets available to search

ShareScore release 0.9.0

Reset

Dataset results

430 results for “Jupiter”

Learn how ShareScore rates datasets ↗
zenodo24/100

Jupiter's CPD #1

<p>Data files for simulation</p>

opencc-by-4.0Dec 2019View details →
zenodo24/100

Dataset for Residual Study: Testing Jupiter Atmosphere Models Against Juno MWR Observations

<p>This dataset includes all data values for all 14 figures in paper &quot;Residual study: Testing Jupiter atmosphere models against Juno MWR observations&quot;.</p>

opencc-by-4.0Mar 2020View details →
zenodo24/100

Models of the gravity field of Jupiter using Slepian and Spherical Harmonic functions

<p>This dataset contains gravitational models using Slepian and spherical harmonic functions for Jupiter,&nbsp;derived from the high-precision Doppler measurements collected by NASA&#39;s&nbsp;Juno mission to Jupiter from periapsis 1 to 17. This dataset is intended to be paired with the following article submitted to the Journal of Geophysical Research-Planets:</p> <p>Marzia Parisi, Eli Galanti, William M. Folkner, Yohai Kaspi and&nbsp;Dustin R. Buccino. &quot;Resolving the latitudinal short-scale gravity field of Jupiter using Slepian functions&quot;, Journal of Geophysical Research, 2020 (submitted Feb&nbsp;2020).<br> &nbsp;<br> This dataset of gravity field models was produced in part at the Jet Propulsion Laboratory by the Juno Gravity Instrument Team and Interiors Working Group.</p>

opencc-by-4.0Sep 2020View details →
zenodo24/100

Characteristics of Jupiter's X-ray auroral hot spot emissions using Chandra

<p>The data used in&nbsp;Weigt et al., study&nbsp;<em>&quot;Characteristics of Jupiter&#39;s X-ray auroral hot spot emissions using Chandra&quot;</em>. The README.pdf explains what data is used to produce each Figure in the article with links to the Chandra archive and scripts used for the polar plots.</p>

opencc-by-4.0Nov 2020View details →
zenodo24/100

Jupiter bust

A quick photogrammetry of a bust of Jupiter I have in my home, as the roman pantheon is the one true religion Base material was a plain white tho, so I've added more interesting textures in Subs. Painter Source: Objaverse 1.0 / Sketchfab

opencc-byJul 2017View details →
zenodo24/100

Ganymede with Jupiter's Eagle

Ganymede with Jupiter's Eagle, 1817, Bertel Thorvaldsen, Marble. 93,3 x 118,3 cm. Thorvaldsen Museum (Copenhagen, Copenhagen). Made with Memento Beta (now ReMake) from AutoDesk. In Greek mythology the boy Ganymede was carried up into the sky, to the home of the gods on Olympus to be the gods' taster. According to legend it was Zeus, in the shape of an eagle, who took the beautiful boy from Phrygia in the north-western part of Asia Minor (Turkey). The effect of Thorvaldsen's sculpture is created mostly by the contrast between the smooth skin of the boy and his trusting nature, which is juxtaposed by the detailed rendering of the eagle's feathers, its harsh look and its sharp beak. Ganymede was to take the place of Hebe as the taster of the gods, because she spilled the drink – the nectar – that made the gods immortal. Thorvaldsen modelled the group sculpture in 1817 and it exists in several marble copies. For more updates, please follow @GeoffreyMarchal on Twitter. Source: Objaverse 1.0 / Sketchfab

opencc-byAug 2017View details →
ClinicalTrials.gov24/100

JUPITER 4.0 - Risk Factors for Failure of Isolated Medial Patellofemoral Ligament Reconstruction

ClinicalTrials.gov study NCT06883396. IPD Sharing: Not stated. Countries: 1. Publications: 0.

restrictedIPD-UNDECIDEDFeb 2026View details →
zenodo20/100

ALTAR DE JUPITER TEATRO DE CARTAGENA

Júpiter (en latín: Iuppiter), también llamado Jove (Iovis), es el principal dios de la mitología romana, padre de dioses y de hombres (pater deorum et hominum). Su equivalente griego es Zeus (en griego antiguo Ζεύς Zéus). Sus atributos son el águila, el rayo, y el cetro. This 3D Model it's a Optimized model (Triangles: 38.9k) from original (Triangles: 647.2k) 3D Model Original : https://skfb.ly/6ROYZ - J.J MARTINEZ Source: Objaverse 1.0 / Sketchfab

opencc-by-nc-1.0Jun 2020View details →
ClinicalTrials.gov20/100

Xenon MRI in Stable Pulmonary Hypertension (Jupiter AUGEAN)

ClinicalTrials.gov study NCT06122922. IPD Sharing: NO. Countries: 0. Publications: 0.

closedIPD-NOFeb 2026View details →
nasa20/100

GO JUP POS GLL TRAJECTORY JUPITER CENTERED COORDINATES V1.0

This data set contains the Galileo spacecraft trajectory data in three coordinate systems commonly used in the analysis of jovian magnetospheric data. These include System III (1965.0), Jupiter Solar Equatorial (JSE), and Jupiter Solar Magnetospheric (JSM) coordinates. The data are sampled every minute inside of 30 Jupiter radii, every ten minutes between 30 and 100 Rj, and every 30 minutes outside of 100 Rj. The data are derived from SPICE SP kernels which are archived at the NAIF Node of the PDS.

restrictedus-pdMar 2025View details →
nasa20/100

VOYAGER 2 JUPITER MAGNETOMETER RESAMPLED DATA 1.92 SEC

This data set includes Voyager 2 Jupiter encounter magnetometer data that have been resampled at a 1.92 second sample rate. The data set is composed of 6 columns: 1) ctime - this column contains the data acquisition time. The time is always output in the ISO standard spacecraft event time format (yyyy-mm-dd-Thh:mm:ss.sss) but is stored internally in Cline time which is measured in seconds after 00:00:00.000 Jan 01, 1966, 2) br - this column contains the radial component of the magnetic field, 3) bphi - this column contains the phi component of the magnetic field, 4) btheta - this column contains the theta component of the magnetic field, 5) bmag - this column contains the magnitude of the magnetic field, 6) flag - a flag value that indicates either software error or spacecraft hardware interference reduced confidence in this record (flag value of 1 is bad , 0 is good or unchecked). All magnetic field observations are measured in nanoTeslas. The coordinate system for this dataset is Minus System III. All of the magnetic field data are calibrated (see the instrument calibration description for more details). The Jupiter System III coordinate system is defined in Dessler 1983 and the reference documents for this dataset are: Ness et al, 1979A Lepping et al, 1981 Connerney,Acuna,Ness, 1981 Behannon,Burlaga,Ness, 1981

restrictedus-pdMar 2025View details →
nasa20/100

ULY JUPITER INTERSTELLAR NEUTRAL-GAS EXPERIMENT SKY MAPS

Ulysses interstellar neutral gas (GAS) experiment sky maps of the count rates of interstellar helium particles (in the NG-mode) or from celestial UV-intensities (UV-mode).

restrictedus-pdApr 2025View details →
nasa20/100

NEW HORIZONS LEISA JUPITER ENCOUNTER V1.1

This data set contains Raw data taken by the New Horizons Linear Etalon Imaging Spectral Array instrument during the Jupiter encounter mission phase.

restrictedus-pdMar 2025View details →
nasa20/100

VG1 LECP 0.4 SEC HIGH RESOLUTION JUPITER NEAR ENCOUNTER DATA

This near encounter data set consists of electron and ion counting rate data from the Low Energy Charged Particle (LECP) experiment on Voyager 1 while the spacecraft was within the very close vicinity of Jupiter. This instrument measures the intensities of in-situ charged particles ( >15 keV electrons and >30 keV ions) with various levels of discrimination based on energy range and mass species. The LECP data are globally calibrated to the extent possible. Particles include low energy electrons, protons, alpha particles, medium energy protons and ions, high energy and intensity protons, electrons, alpha particles, and Z >= nuclei.

restrictedus-pdMar 2025View details →
nasa20/100

VOYAGER 1&2 JUPITER BRIGHTNESS NORTH/SOUTH MAP SET V1.0

This data set contains Voyager 1 and 2 measurements of the brightness of Jupiter at H Lyman alpha and in the H2 Lyman and Werner bands shortward of H Lyman alpha. Pointing has been corrected by the C-Smithing process, and these data were derived from the pre-encounter North-South Map sequences. In this sequence, the UVS field of view was located near the central meridian of the planet. The field of view stepped slowly from north to south, and then rapidly repositioned to the north. These scans were repeated until all Jovian longitudes had been sampled. Coverage in longitude was not continuous in time. Rather, some longitude ranges were covered on the preceding or following rotation of Jupiter.

restrictedus-pdMar 2025View details →
nasa20/100

NEW HORIZONS SWAP JUPITER ENCOUNTER V1.0

This data set contains Raw data taken by the New Horizons Solar Wind Around Pluto instrument during the Jupiter encounter mission phase.

restrictedus-pdMar 2025View details →
nasa20/100

VG1 JUPITER SPICE SPK KERNEL V2.0

Version 2.0 ----------- This data set replaces the Voyager 1 Jupiter SPICE data set (DATA_SET_ID = VG1-J-6-SPK-V1.0).

restrictedus-pdMar 2025View details →
nasa20/100

JUNO JUPITER MWR REDUCED DATA RECORDS V2.0

The Juno MWR RDR data sets will ultimately include all calibrated MWR science data records for the entire Juno mission. The set in this volume will contain only those data obtained during the orbital phase of the Juno mission, when this phase of the mission is completed. The RDR science records have a one-to-one correspondence with the EDR records.

restrictedus-pdMar 2025View details →
nasa20/100

NEW HORIZONS PEPSSI JUPITER ENCOUNTER V1.1

This data set contains Raw data taken by the New Horizons Pluto Energetic Particle Spectrometer Science Investigation instrument during the Jupiter encounter mission phase.

restrictedus-pdMar 2025View details →
nasa20/100

ESO NTT EMMI IMAGE DATA FROM SL9 IMPACTS WITH JUPITER V1.0

ESO MultiMode Instrument has various spectroscopic options with large-field capabilities (up to 10 x 10 arcmin with a 2048**2 CCD).

restrictedus-pdMar 2025View details →

ScienceDex guides

Understand access before you commit

These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research datasets.

Compare curated datasets

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.

allen-brain-atlas
neuroscienceopenDocumentation, web resources, and API references are available online.
Last verified 2026-04-30Open record

Annotated Behaviour and Observability Dataset (ABODe)

ABODe is a University of Edinburgh DataShare dataset for behavior classification in group-housed mice using home-cage video, identities, bounding boxes, ground-plate positions, and annotator labels.

abode-home-cage
behavioral-neuroscienceopenThe DataShare record exposes download links for annotations, documentation, license text, and the zipped per-snippet data directory.
Last verified 2026-04-30Open record

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.

dandi-nwb
electrophysiologyopenPublished Dandiset metadata and archive endpoints are available through the production DANDI API.
Last verified 2026-04-30Open record

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.

ibl
behavioral-neuroscienceopenPublic sessions can be searched and loaded from the IBL public data server through ONE.
Last verified 2026-04-29Open record

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.

openneuro
neuroscienceopenPublished datasets are available on demand over the internet.
Last verified 2026-04-29Open record