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.
115
datasets available to search
ShareScore release 0.7.1
Dataset results
115 results for “Solar eclipse”
NT1D CHU 14.670 MHz from April 8, 2024 Solar Eclipse
<p>Radio:</p> <p>GPS-disciplined:</p> <p>AGC:</p> <p>Lat/lon: </p> <table> <tbody> <tr> <td>42.4717</td> <td>-71.619</td> </tr> </tbody> </table> <p>Notes: </p> <p>14.669 MHz USB (CW): Icom IC-705 connected to Mosley CL-33. PC is Dell XPS9320 Windows 11</p>
CWRU Farm SDR CHU 14.770 MHz from April 8, 2024 Solar Eclipse
<p>Collected at Squire Valleevue Farm.</p> <table> <tbody> <tr> <td>41.49308889</td> <td>-81.42378287</td> </tr> </tbody> </table>
CWRU Farm CHU 7.850 MHz from April 8, 2024 Solar Eclipse
<p>Collected at Squire Valleevue Farm.</p> <table> <tbody> <tr> <td>41.49308889</td> <td>-81.42378287</td> </tr> </tbody> </table>
CWRU Farm (ET) CHU 3.330 MHz from April 8, 2024 Solar Eclipse
<p>Collected at Squire Valleevue Farm.</p> <table> <tbody> <tr> <td>41.49308889</td> <td>-81.42378287</td> </tr> </tbody> </table>
WA4YWM CHU 7.850 MHz from April 8, 2024 Solar Eclipse
<p>Radio: <span>Elecraft K3S</span></p> <p><span>GPS-disciplined: No</span></p> <p><span>AGC: Off</span></p> <p><span>Antenna: <span>40M NVIS Dipole oriented East to West</span></span></p> <p><span><span>Lat/lon: </span></span></p> <table> <tbody> <tr> <td>40.41585</td> <td>-75.376109</td> </tr> </tbody> </table> <p>Notes: <span>Note that the first recording was briefly interrupted due to a power failure at 1500 on 4/3. The second recording was started at 1508.</span></p>
W0EJO CHU 14.670 MHz from April 8, 2024 Solar Eclipse
<p>Radio: <span>Icom-718</span></p> <p><span>GPS-disciplined: Yes</span></p> <p><span>AGC: Off</span></p> <p><span>Antenna: <span>Vertical Mosley RV4C</span></span></p> <p><span><span>Lat/lon:</span></span></p> <table> <tbody> <tr> <td>38.6559</td> <td>-90.35107</td> </tr> </tbody> </table> <p> </p>
2024-04-08 Total Solar Eclipse ESID# 517
<p>These are audio recordings taken by an Eclipse Soundscapes (ES) Data Collector during the week of the April 8, 2024 total solar eclipse. </p> <p><strong>Data Site location information:</strong></p> <ul> <li>Latitude: 29.345988</li> <li>Longitude: -99.97628</li> <li>Type of Eclipse: Total Solar Eclipse</li> <li>Eclipse %: 100%</li> <li>WAV files Time & Date Settings: Set with the automated AudioMoth time chime</li> </ul> <p><strong>Included Data:</strong></p> <ul> <li> <p><strong>Audio files in WAV format</strong> with the date and time in UTC within the file name: YYYYMMDD_HHMMSS meaning YearMonthDay_HourMinuteSecond<br>For example, 20240411_141600.WAV means that this audio file starts on April 11, 2024 at 14:16:00 Coordinated Universal Time (UTC)</p> </li> <li> <p><strong>CONFIG Text file: </strong>Includes AudioMoth device setting information, such as sample rate in Hertz (Hz), gain, firmware, etc. </p> </li> </ul> <p><strong>Eclipse Information for this location:</strong></p> <ul> <li>Eclipse Date: 4/8/2024</li> <li>Eclipse Start Time (UTC): 17:12:07</li> <li>Totality Start Time (UTC): 18:29:24</li> <li>Eclipse Maximum [when the most possible amount of the Sun in blocked] (UTC): 18:31:37</li> <li>Totality End Time (UTC): [N/A if partial eclipse] 18:33:50</li> <li>Eclipse End Time (UTC): [N/A if partial eclipse] 19:53:05</li> </ul> <p><strong>Audio Data Collection During Eclipse Week </strong></p> <p>ES Data Collectors used AudioMoth devices to record audio data, known as soundscapes, over a 5-day period during the eclipse week: 2 days before the eclipse, the day of the eclipse, and 2 days after. The complete raw audio data collected by the Data Collector at the location mentioned above is provided here. This data may or may not cover the entire requested timeframe due to factors such as availability, technical issues, or other unforeseen circumstances. </p> <p><strong>ES ID# Information:</strong></p> <p>Each AudioMoth recording device was assigned a unique Eclipse Soundscapes Identification Number (ES ID#). This identifier connects the audio data, submitted via a MicroSD card, with the latitude and longitude information provided by the data collector through an online form. The ES team used the ES ID# to link the audio data with its corresponding location information and then uploaded this raw audio data and location details to Zenodo. This process ensures the anonymity of the ES Data Collectors while allowing them to easily search for and access their audio data on Zenodo. </p> <p><strong>TimeStamp Information:</strong></p> <p>The ES team and the Data Collectors took care to set the date and time on the AudioMoth recording devices using an AudioMoth time chime before deployment, ensuring that the recordings would have an automatic timestamp. However, participants also manually noted the date and start time as a backup in case the time chime setup failed. The notes above indicate whether the WAV audio files for this site were timestamped manually or with the automated AudioMoth time chime. </p> <p><strong>Latitude & Longitude Information:</strong></p> <p>The latitude and longitude for each site was taken manually by data collectors and submitted to the ES team, either via a web form or on paper. It is shared in Decimal Degrees format.</p> <p><strong>General Project Information:</strong></p> <p>The Eclipse Soundscapes Project is a NASA Volunteer Science project funded by NASA Science Activation that is studying how eclipses affect life on Earth during the October 14, 2023 annular solar eclipse and the April 8, 2024 total solar eclipse. Eclipse Soundscapes revisits an eclipse study from almost 100 years ago that showed that animals and insects are affected by solar eclipses! Like this study from 100 years ago, ES asked for the public’s help. ES uses modern technology to continue to study how solar eclipses affect life on Earth! You can learn more at www.EclipseSoundscapes.org. </p> <p>Eclipse Soundscapes is an enterprise of ARISA Lab, LLC and is supported by NASA award No. 80NSSC21M0008. </p> <p><strong>Eclipse Data Version Definitions</strong></p> <p>{1st digit = year, 2nd digit = Eclipse type (1=Total Solar Eclipse, 9=Annular Solar Eclipse, 0=Partial Solar Eclipse), 3rd digit is unused and in place for future use}</p> <p><strong>2023.9.0 </strong>= Week of October 14, 2023 Annular Eclipse Audio Data, Path of Annularity (Annular Eclipse)</p> <p><strong>2023.0.0 </strong>= Week of October 14, 2023 Annular Eclipse Audio Data, OFF the Path of Annularity (Partial Eclipse)</p> <p><strong>2024.1.0</strong> = Week of April 8, 2024 Total Solar Eclipse Audio Data, Path of Totality (Total Solar Eclipse)</p> <p><strong>2024.0.0</strong> = Week of April 8, 2024 Total Solar Eclipse Audio Data , OFF the Path of Totality (Partial Solar Eclipse)</p> <p><em>*Please note that this dataset’s version number is listed below.</em></p> <p dir="ltr"><strong>Individual Site Citation: APA Citation (7th edition)</strong></p> <p dir="ltr">ARISA Lab, L.L.C., Winter, H., Severino, M., & Volunteer Scientist. (2025). 2024 solar eclipse soundscapes audio data [Audio dataset, ES ID# 517]. Zenodo.{Insert DOI} Collected by volunteer scientists as part of the Eclipse Soundscapes Project. The Eclipse Soundscapes project is supported by NASA award No. 80NSSC21M0008.</p> <p dir="ltr"><strong>Eclipse Community Citation</strong></p> <p>ARISA Lab, L.L.C., Winter, H., Severino, M., & Volunteer Scientists. 2023 and 2024 solar eclipse soundscapes audio data [Collection of audio datasets]. Eclipse Soundscapes Community, Zenodo. <a href="https://zenodo.org/communities/eclipsesoundscapes/">https://zenodo.org/communities/eclipsesoundscapes/<br></a>Collected by volunteer scientists as part of the Eclipse Soundscapes Project.<br>This project is supported by NASA award No. 80NSSC21M0008.</p>
ET1008 - VE3KG Radio Association of Canada - CHU 14.670 MHz from April 8, 2024 Solar Eclipse
<p>See <a href="https://doi.org/10.5281/zenodo.13293306">10.5281/zenodo.13293306</a> for system documentation. <br>See <a href="https://doi.org/10.5281/zenodo.14004715">10.5281/zenodo.14004715</a> for python code to parse these files. </p> <p>Location: Ottawa, ON.</p> <p>Lat/lon: </p> <table> <tbody> <tr> <td>45.14417295</td> <td>-76.16592324</td> </tr> </tbody> </table> <p>Data collected by <a href="https://www.qrz.com/db/ve3kg">Dave Goodwin VE3KG</a>. </p>
ET0001 - CWRU Farm - CHU 14.670 MHz from April 8, 2024 Solar Eclipse
<p>See <a href="https://doi.org/10.5281/zenodo.13293306">10.5281/zenodo.13293306</a> for system documentation. <br>See <a href="https://doi.org/10.5281/zenodo.14004715">10.5281/zenodo.14004715</a> for python code to parse these files. </p> <p>Location: Chagrin Falls, OH. </p> <p>Lat/lon: </p> <table> <tbody> <tr> <td>41.49308889</td> <td>-81.42378287</td> </tr> </tbody> </table>
Data from: Bioelectrical synchronization of Picea abies during a solar eclipse
Open the record for dataset details and reuse information.
K5JBT 40m I/Q Solar Eclipse Observations
<p>John Thurmond K5JBT</p> <p>Location: 29.762948N, -95.707518W (Houston, TX)</p> <p>Antenna: Inverted-L (ca. 25 ft vertical, 15 ft lateral oriented NE)</p> <p>Receiver type: Flex 6300</p> <p>Antenna was tuned for 20m, but also recorded on 40m</p>
K5JBT 20m I/Q Solar Eclipse Observations
<p>John Thurmond K5JBT</p> <p>Location: 29.762948N, -95.707518W (Houston, TX)</p> <p>Antenna: Inverted-L (ca. 25 ft vertical, 15 ft lateral oriented NE)</p> <p>Receiver type: Flex 6300</p> <p>Antenna was tuned for 20m, but also recorded on 40m</p>
Multi-instrument observations of the ionospheric response to the 26 December 2019 solar eclipse over Indian and Southeast Asian longitudes
<p>Here, the impact of the 26 December 2019 solar eclipse on the equatorial and low latitude ionosphere has been investigated using ground and space-based observations over Indian and Southeast Asian longitudes. The high-resolution Ionosonde observations at Tirunelveli, GPS TEC observations from a chain of GPS receivers along and across the eclipse path, TIMED-SABER, and Ionospheric Connection Explorer (ICON) satellites were utilized to investigate the eclipse-induced variations in electron density and thermospheric cooling. We noticed a tremendous increase and decrease in the base height of the F-layer, resembling the nighttime Pre-Reversal Enhancement (PRE). Near the eclipse maximum, a strong blanketing sporadic E layer was observed at Tirunelveli with a top frequency of ~18 MHz for 1 hour and 26 minutes. Satellite traces (STs) and ‘U’ shaped ionograms were noticed for the first time over Tirunelveli during eclipse maximum and end phases. The ‘STs’ and ‘U’ shaped traces indicate the presence of short-period gravity waves or TID type of wave perturbations over the Indian region. A maximum of ~5-7 TECU (30-40%) decrease in TEC is observed on the eclipse day for iisc, hyde, and tiru stations. Periodogram analyses of TEC data showed the presence of wavelike structures with periodicities of 18-24 minutes for different stations. Simultaneous observations from the ICON satellite showed an increase and decrease in hmF2 and NmF2 which matches well with the ionosonde observations from Tirunelveli. The temperature profiles from TIMED-SABER and ICON satellites showed a reduction and enhancement in the lower and upper E regions respectively.</p>
WE9V Widband IQ data High Bands 15M, 17M, and 20M during solar eclipse
<p>Chad Kurszewski</p> <p>Amateur Radio Callsign: WE9V</p> <p>Station Location: 42.554568 N, 88.050680 W</p> <p>Receiver: Software Radio Laboratory LLC | QS1R, with DX Engineering RPA-1 16dB pre-amplifier</p> <p>Antenna: 1/4 wave 30M Groundplane (vertical, omnidirectional), ground mounted</p> <p>Recorded IQ data for 96kHz bandwidth, 15M (21 MHz), 17M (18 MHz), and 20M (14 MHz), one file every 15 minutes for each band</p>
EA4GPZ Solar Eclipse 2017 wideband recording 20m
<p>Amateur radio callsign: EA4GPZ</p> <p>Station location: 40.595862, -3.699246</p> <p>Antenna: Longwire, around 20m long, untuned, pointing N-S roughly.</p> <p>Receiver: Hermes-Lite 2.0beta2, set to a gain of 12dB</p> <p>Receiver amplitude calibration: An VRMS of 1 in the I and Q channels corresponds to a power of 17dBm at the input of the receiver.</p> <p>Format: Digital RF format inside a tar.xz file. Only one band in this publication. There is a set of 3 publications with the 40m, 30m and 20m bands.</p>
EA4GPZ Solar Eclipse 2017 wideband recording 40m
<p>Amateur radio callsign: EA4GPZ</p> <p>Station location: 40.595862, -3.699246</p> <p>Antenna: Longwire, around 20m long, untuned, pointing N-S roughly.</p> <p>Receiver: Hermes-Lite 2.0beta2, set to a gain of 12dB</p> <p>Receiver amplitude calibration: An VRMS of 1 in the I and Q channels corresponds to a power of 17dBm at the input of the receiver.</p> <p>Format: Digital RF format inside a tar.xz file. Only one band in this publication. There is a set of 3 publications with the 40m, 30m and 20m bands.</p>
EA4GPZ Solar Eclipse 2017 wideband recording 30m
<p>Amateur radio callsign: EA4GPZ</p> <p>Station location: 40.595862, -3.699246</p> <p>Antenna: Longwire, around 20m long, untuned, pointing N-S roughly.</p> <p>Receiver: Hermes-Lite 2.0beta2, set to a gain of 12dB</p> <p>Receiver amplitude calibration: An VRMS of 1 in the I and Q channels corresponds to a power of 17dBm at the input of the receiver.</p> <p>Format: Digital RF format inside a tar.xz file. Only one band in this publication. There is a set of 3 publications with the 40m, 30m and 20m bands.</p>
WE9V Widband IQ data Low Bands 30M, 40M, 80M and 160M during solar eclipse
<p>Chad Kurszewski</p> <p>Amateur Radio Callsign: WE9V</p> <p>Station Location: 42.554568 N, 88.050680 W</p> <p>Receiver: Software Radio Laboratory LLC | QS1R, with DX Engineering RPA-1 16dB pre-amplifier</p> <p>Antenna: 1/4 wave 30M Groundplane (vertical, omnidirectional), ground mounted</p> <p>Recorded IQ data for 96kHz bandwidth, 30M (10 MHz), 40M (7 MHz), 80M (3.5 MHz) and 160M (1.8 MHz), one file every 15 minutes for each band</p>
The effect of the 2017 solar eclipse in the ionospheric total electron content
<p>Using 15-second RINEX files inside the totality path, I calculated the Total Electron Content (TEC) at each station-satellite pair for each epoch recorded during the day of the 2017 solar eclipse. These calculations result in TEC observations at the ionospheric piercing points (IPP), the intersection of the station-satellite line-of-sight (LOS) and the peak electron density of the ionospheric F layer at a height of ~300 km. Using the estimated TEC at each IPP, I produced a video showing the TEC change during the passage of the umbra and penumbra of the eclipse over North America over a period of one hour. The video shows that as the moon’s shadow passes and the sunlight is blocked, the TEC drops due to the recombination of the ionized particles. More information available at the UNAVCO Google+ webpage: https://plus.google.com/u/0/112042426109504523574/posts/bPJ2f7exmPk</p>
Langley Mobile Ozone Lidar observation of the O3 and aerosol variability during the 2024/04/08 solar eclipse
<p>This dataset corresponds to the observation of the O3 at Nasa Langley Research Center in Hampton, Virginia, during the Solar eclipse of 2023/04/08.</p> <p>This dataset contains, in addition to the O3 that can be found at https://tolnet.larc.nasa.gov, the aerosols backscattering and the aerosols boundary layer (which is presented in form of black mark in the accompanying image)</p>
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.