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.
107
datasets available to search
ShareScore release 0.9.0
Dataset results
107 results for “Juno”
Juno Radio Occultation Data Sets
<p>These files report data products derived from Juno radio occultations of the Io plasma torus. Juno has used two different experimental configurations to conduct radio occultation observations of the Io plasma torus. A configuration with X-band uplink coherently driving both X-band downlink and Ka-band downlink was used on Perijoves 1 and 13. In this document, this is described as the (X/X, X/Ka) configuration. It is described in Phipps et al. 2018. A configuration with X-band uplink coherently driving X-band downlink and Ka-band coherently driving Ka-band downlink was used on Perijoves 3, 6, 8, 10, 11, 14, and 15. In this document, this is described as the (X/X, Ka/Ka) configuration. It is described in Phipps et al. 2019.The work of D. Buccino, M. Parisi and O. Yang was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Government sponsorship acknowledged. This work was supported in part by NASA award 80NSSC19K0818.</p>
Dataset for Angular Dependence and Spatial Distribution of Jupiter's Centimeter-Wave Thermal Emission from Juno's Microwave Radiometer
<p>This dataset comprises all processed data (in HDF5 format) used in figures and discussion in the paper "Angular Dependence and Spatial Distribution of Jupiter's Centimeter-Wave Thermal Emission from Juno's Microwave Radiometer".</p>
ALTAR DE JUNO TEATRO DE CARTAGENA
Juno era una diosa, equivalente a la Hera griega, diosa del matrimonio y reina de los dioses. Hija de Saturno y Ops, hermana y esposa de Júpiter, con el que tuvo dos hijos, Marte y Vulcano y una hija, Lucina. This 3D Model it's a Optimized model (Triangles: 33.4k) from original (Triangles: 549.2k) 3D Model Original : https://skfb.ly/6RPZv - J.J MARTINEZ Source: Objaverse 1.0 / Sketchfab
Supporting material to "Effect of magnetospheric conditions on the morphology of Jupiter's UV main auroral emission, as observed by Juno-UVS"
Open the record for dataset details and reuse information.
FIGURE 2 in Notes on taxonomy and nomenclature of juno irises (Juno, Iridaceae)
FIGURE 2. Neotype of Iris sieheana Lynch (E00333002). Reproduced with permission (Royal Botanic Garden Edinburgh).
FIGURE 3 in Notes on taxonomy and nomenclature of juno irises (Juno, Iridaceae)
FIGURE 3. Neotype of Thelysia tarhunensis Borzì & Mattei (FI052410). Reproduced with permission (Museo di Storia Naturale, Firenze, Italy).
FIGURE 1 in Notes on taxonomy and nomenclature of juno irises (Juno, Iridaceae)
FIGURE 1. Lectotype of Juno fumosa Kamelin (JE00020054). Reproduced with permission (Herbarium Haussknecht, Friedrich-SchillerUniversität Jena, Austria).
Data for Statistics on Jupiter's Current Sheet with Juno Data: Geometry, Magnetic Fields and Energetic Particles
<p>The statistical data of paper "Statistics on Jupiter’s Current Sheet with Juno Data: Geometry, Magnetic Fields and Energetic Particles"</p>
Juno Stellar Reference Unit (SRU) image data for high energy ion detections during perijoves 22-35
<p>This is the Juno Stellar Reference Unit (SRU) image data for high energy ion detections during perijoves 22 to 35.</p>
Altar de Juno - Teatro de Cartagena
Juno era una diosa, equivalente a la Hera griega, diosa del matrimonio y reina de los dioses. Hija de Saturno y Ops, hermana y esposa de Júpiter, con el que tuvo dos hijos, Marte y Vulcano y una hija, Lucina. Source: Objaverse 1.0 / Sketchfab
Juno Waves Detection of Dust Impacts near Jupiter
<p>This is the supporting data set for the paper by the same title published in AGU JGR Space Physics. DOI 10.1029/2019JE006367</p> <p>Abstract:</p> <p>The Juno spacecraft entered orbit at Jupiter on July 5, 2016. Since then, Juno has orbited Jupiter in high inclination orbits, crossing the ring plane near perijove 21 times. During 20 of the 21 crossings, the Waves instrument detected signals induced by dust impacts. The impact rate profiles show peaks of order 6/s around the ring plane with half width at half max ~2000-3000 km. The polarity ratio of the impact signals didn't follow the areas of the antennas exposed to dust impacts that change due to the rotation of the spacecraft, suggesting Waves detects impacts on the Juno spacecraft and not just on the Waves antennas. The impact rate profile changed during Perijove 19, when the spacecraft rotation axis was tilted to the south, increasing the area of the solar panels exposed to impacts, indicating that the detected impacts were on the spacecraft body. Grain sizes of order 1 micrometer are estimated, and the differential size distribution has a slope of -5.1.</p> <p>Notes on zip archive:</p> <p>There are subdirectories for each figure including a PDF of the figure and one or more text files with the data supporting the figure. Where the labeling in the text file is not quite complete, we've added a Fign-readme.txt file.</p> <p>Figures 9 and 10 are in the same directory as the two figures just have more of the same and all the data for both figures is in the same file.</p>
Corresponding Dataset for "Electron Density in Io's Alfvén Wing Observed via Radio Occultation with Juno"
<div> Corresponding Dataset for "Electron Density in Io’s Alfvén Wing </div> <div> Observed via Radio Occultation with Juno"</div> <div> README FILE</div> <div> Dustin Buccino</div> <div> July 15, 2024</div> <div> Jet Propulsion Laboratory</div> <div> California Institute of Technology</div> <div> </div> <div>=============================================================================</div> <div>INTRODUCTION</div> <div>=============================================================================</div> <div> </div> <div> This dataset contains processed radio science data and results of the</div> <div>Juno Ganymede radio occultation. This dataset is provided in order to </div> <div>supplement the submitted article to the "Geophysical Research Letters"</div> <div>journal:</div> <div> </div> <div> Buccino, D.R., et al (2024), Electron Density in Io’s Alfvén Wing </div> <div> Observed via Radio Occultation with Juno, Geophysical Research </div> <div> Letters, submitted July 2024.</div> <div> </div> <div> </div> <div> Please note the raw data used in this analysis are not provided in this</div> <div>supplementary dataset. The raw Juno Gravity Science Data may be found at </div> <div>the Planetary Data System:</div> <div> </div> <div> Buccino, D. R. (2016). Juno jupiter gravity science raw data set </div> <div> V1.0, JUNO-J-RSS-1 JUGR-V1.0, NASA planetary data system (PDS). </div> <div> Retrieved from https://atmos.nmsu.edu/PDS/data/jnogrv_1001/</div> <div> </div> <div> </div> <div>=============================================================================</div> <div>ARCHIVE INFORMATION</div> <div>=============================================================================</div> <div> </div> <div> This archive contains ten files within the root directory.</div> <div> </div> <div> </div> <div> I57 Data</div> <div> </div> <div> i57_observed.txt</div> <div> Raw frequency observables. Reported as X-band minus Ka-band,</div> <div>see paper for details (X_freq - 880.0/3360.0*Ka_freq)</div> <div> </div> <div> i57_tec.csv</div> <div>Total electron content information from the flyby</div> <div>(uncalibrated, model, calibrated data)</div> <div> </div> <div> i57_density_inbound_raytracing.txt</div> <div>Estimated electron density inbound during the flyby </div> <div>estimated with the ray tracing method (see paper)</div> <div> </div> <div> i57_density_outbound_raytracing.txt</div> <div>Estimated electron density outbound during the flyby </div> <div>estimated with the ray tracing method (see paper)</div> <div> </div> <div> i57_density_tubes.csv</div> <div>Estimated electron density during the flyby using</div> <div>the horizontal tubes method (see paper)</div> <div> </div> <div> I58 Data</div> <div> </div> <div> i58_observed.txt</div> <div> Raw frequency observables. Reported as X-band minus Ka-band,</div> <div>see paper for details (X_freq - 880.0/3360.0*Ka_freq)</div> <div> </div> <div> i58_tec.csv</div> <div>Total electron content information from the flyby</div> <div>(uncalibrated, model, calibrated data)</div> <div> </div> <div> i58_density_inbound_raytracing.txt</div> <div>Estimated electron density inbound during the flyby </div> <div>estimated with the ray tracing method (see paper)</div> <div> </div> <div> i58_density_outbound_raytracing.txt</div> <div>Estimated electron density outbound during the flyby </div> <div>estimated with the ray tracing method (see paper)</div> <div> </div> <div> i58_density_tubes.csv</div> <div>Estimated electron density during the flyby using</div> <div>the horizontal tubes method (see paper)</div> <div> </div> <div>=============================================================================</div> <div>FILE FORMAT</div> <div>=============================================================================</div> <div> </div> <div> This dataset contains only ASCII formatted files. There are two formats,</div> <div> a plain-text file with the extension *.txt and a comma-separated file</div> <div> with the extension *.csv.</div> <div> </div> <div> </div> <div> PLAIN-TEXT FILES</div> <div> -------------------------------------------------------------------------</div> <div> </div> <div> The plain ASCII text files (TXT) files are fixed-width columns. Values in</div> <div> each data file are separated with spaces. Each column is defined </div> <div> by a header row which provides a description of each column.</div> <div> </div> <div> CSV FILES</div> <div> -------------------------------------------------------------------------</div> <div> </div> <div> The Comma-Separated Value (CSV) files are plain-text files. Values in</div> <div> each data file are separated using a comma ",". Each column is defined </div> <div> by a header row which provides a description of each column.</div> <div> </div> <div> </div> <div>=============================================================================</div> <div>ACKNOWLEDGMENTS</div> <div>=============================================================================</div> <div> </div> <div>The work of DB, MP, RP, and SL was carried out at the Jet Propulsion </div> <div>Laboratory, California Institute of Technology, under a contract with the </div> <div>National Aeronautics and Space Administration. Government sponsorship </div> <div>acknowledged.</div> <div> </div> <div>AC, LGC, MZ, EG, and PT are grateful to the Italian Space Agency (ASI) for </div> <div>financial support through Agreement No. 2023-6-HH.0 in the context of ESA’s </div> <div>JUICE mission, and Agreement No. 2022-16-HH.0, for ESA’s BepiColombo and </div> <div>NASA’s Juno radio science experiments.</div> <div> </div> <div>PW and DC acknowledge support from NASA award 80NSSC23K0020.</div> <div> </div> <div>PS was supported by NASA Contract NNM06AA75C from the Marshall Space </div> <div>Flight Center under subcontract 699054X from Southwest Research Institute.</div> <div> </div> <div>(c) 2024 California Institute of Technology. Government sponsorship </div> <div>acknowledged.</div> <div> </div> <div>=============================================================================</div> <div>PRIMARY POINT OF CONTACT</div> <div>=============================================================================</div> <div> </div> <div>Dustin Buccino</div> <div>Jet Propulsion Laboratory</div> <div>Planetary Radar and Radio Sciences</div> <div>(818) 393 - 1072</div> <div>Dustin.R.Buccino@jpl.nasa.gov</div> <div> </div> <div>=============================================================================</div> <div>ACRONYMS AND ABBREVIATIONS</div> <div>=============================================================================</div> <div> </div> <div> ASCII American Standard Code for Information Interchange</div> <div> DOY Day of year</div> <div> DSN Deep Space Network</div> <div> JPL Jet Propulsion Laboratory</div> <div> NAIF Navigation Ancillary Information Facility</div> <div> NASA National Aeronautics and Space Administration</div> <div> PDS Planetary Data System</div> <div> RS Radio Science</div> <div> RSS Radio Science Subsystem</div> <div> SIS Software Interface Specification</div> <div> TXT Text file</div> <div> UTC Universal Time, Coordinated</div>
Juno Perth Clinical Trial
ClinicalTrials.gov study NCT02317042. IPD Sharing: NO. Countries: 1. Publications: 0.
Data from: Izumo1 and Juno: the evolutionary origins and coevolution of essential sperm-egg binding partners
Open the record for dataset details and reuse information.
Comparative metabolic and transcriptional analysis of a doubled diploid and its diploid citrus rootstock (C. junos cv. Ziyang xiangcheng) suggests its potential value for stress resistance improvement
GEO Series GSE65416. Citrus junos. 4 samples. Type: Expression profiling by high throughput sequencing.
A non-canonical repressor function of JUN restrains YAP activity and suppresses YAP-dependent liver cancer growth [3prime_Seq_JUNoe]
GEO Series GSE235613. Homo sapiens. 5 samples. Type: Expression profiling by high throughput sequencing.
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 "Residual study: Testing Jupiter atmosphere models against Juno MWR observations".</p>
Statue of Juno Regina from Chesters Roman Fort
Statue of Juno Regina standing on a heifer, c. 3rd century AD from Chesters Roman Fort, currently housed in the Clayton Museum. 24 photos model made with Agisfot Photoscan https://www.english-heritage.org.uk/visit/places/chesters-roman-fort-and-museum-hadrians-wall/ Source: Objaverse 1.0 / Sketchfab
Long-term Follow-up Study for Patients Previously Treated With a Juno CAR T-Cell Product
ClinicalTrials.gov study NCT03436771. IPD Sharing: NO. Countries: 1. Publications: 0.
Effect of Intake of Citron(Citrus Junos Siebold ex Tanaka) Peel Extract on Blood Cholesterol.
ClinicalTrials.gov study NCT03332641. IPD Sharing: Not stated. Countries: 1. Publications: 0.
ScienceDex guides
Understand access before you commit
These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research 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.
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.
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.