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31 results for “Space Physics”
Simulation data for "Characteristics of Wave-Particle Power Transfer as a Function of Electron Pitch Angle in Nonlinear Frequency Chirping" which will be submitted to Journal of Geophysical Research: Space Physics
<p>Simulation data for "Characteristics of Wave-Particle Power Transfer as a Function of Electron Pitch Angle in Nonlinear Frequency Chirping" which will be submitted to Journal of Geophysical Research: Space Physics.</p> <p>Including the simulation input parameter file and the necessary output data to plot each figure in the article. </p>
Data sets for "MELISSA: System description and spectral features of pre‐ and post‐midnight F‐region echoes. Journal of Geophysical Research: Space Physics" by Rodrigues et al.
<p>Observations used in the study "Rodrigues, F. S., Zhan, W., Milla, M. A., Fejer, B. G., de Paula, E. R., Neto, A. C., et al ( 2019). MELISSA: System description and spectral features of pre‐ and post‐midnight <em>F</em>‐region echoes. <em>Journal of Geophysical Research: Space Physics</em>, 124. <a href="https://doi.org/10.1029/2019JA027445">https://doi.org/10.1029/2019JA027445</a>."</p> <p>The uploaded files include the RTI maps measured by the MELISSA radar system between 2014 and 2018 (.tif files). They also include values of SNR versus local time and height and the spectra presented in the manuscript (.mat files).</p> <p>Please, see README.txt for additional details.</p>
Polar UVI Images (Intensity and Boundary) & Space Physical Parameters Joint Data
<p><span>The ultraviolet imager on board the Polar satellite is capable of capturing information about the polar and equatorial boundaries of the auroral oval, the overall morphology of the auroral oval, and the spatial distribution of auroral oval intensity. The intensity of the auroral oval are related to the amount of energy injected from the solar wind and magnetosphere into the polar ionosphere. And the position and size of the auroral oval boundary is also closely linked to changes in the space environment. In order to mitigate the influence of daylight on auroral images, we selected a total of 4215 images of both full, gap and incomplete aurora ovals. We utilized corresponding Interplanetary Magnetic Field (IMF), solar wind parameters, and geomagnetic index data from the NASA OMNI database to build a jointly dataset consist of the space physical parameters and the intensity and boundaries of the aurora oval.</span></p>
Data for manuscript # 2021JA029122 JGR-Space Physics
<p>This is a collection of files that we have used to generate our figures for the manuscript 2021JA029122. </p>
Digisonde Data files used for JGR-Space Physics paper "A simplified method of true height analysis to estimate the real height of sporadic E layers"
<p>paper submitted for publication in JGR-Space Physics.</p> <p>Digisonde Data files used for analysis</p> <p> </p> <p>A simplified method of true height analysis to estimate the real height of sporadic E layers</p> <p> </p> <p>Christos Haldoupis</p> <p>Department of Physics, University of Crete, Heraklion, Greece</p> <p>Haris Haralambous</p> <p>Frederick University and Frederick Research Center, Nicosia, Cyprus</p> <p>Chris Meek</p> <p>Institute of Space and Atmospheric Studies, University of Saskatchewan, Saskatoon, SK, Canada</p>
Dataset for "Data-driven empirical conductance relations during auroral precipitation using incoherent scatter radar and all sky imagers" JGR-Space Physics
<p><strong>Dataset for "Data-driven empirical conductance relations during auroral precipitation using incoherent scatter radar and all sky imagers" JGR-Space Physics.</strong></p> <p>Processed ACF level data can be provided by contacting me.</p> <p><strong>DOI of the publication:</strong></p> <p><strong>README file:</strong></p> <p>PFISRInversions_ASI_v1.1_Fang_01042023_v08162023.h5</p> <p>HallConductance: Altitude integrated Hall Conductance from 85-150 km altitude, [ntime], mho<br> PedersenConductance: Altitude integrated Pedersen Conductance from 85-150 km, [ntime], mho<br> EnergyFlux: Energy flux after integrating the differential number flux, [ntime], W/m^2<br> AverageEnergy: Average Energy after integrating the differential number flux, [ntime], eV<br> Measured_ElectronDensity: measured electron density from PFISR, [ntime, naltitude], #/m^3<br> Modeled_ElectronDensity: modeled electron density produced by the MEM version, [ntime,naltitude], #/m^3<br> UnixTime: time in seconds since 1970-01-01 00:00:00 UT, [ntime], seconds<br> NumberFlux: differential number flux, [ntime, nenergy], #/m^2 s^-1 eV^-1<br> EnergyGrid: energy grid spanning 1 keV - 100 keV in 25 steps, [nenergy], eV<br> ASIStatus: auroral identification number, [ntime], no units<br> 1: Discrete aurora<br> 2: Diffuse aurora<br> 3: Pulsating aurora<br> 8: Unidentified aurora<br> -1: data that was flagged as unsuitable:<br> either TEC was too low (no auroral E-region possibly associated with red aurora),<br> the modeled electron density was not consistent at all with the observed electron density (bad fit)</p> <p>ASIYEAR-Final_date.xlsx<br> This is an excel file that contains the original auroral image identification near the zenith direction<br> We used all sky imager videos located: http://optics.gi.alaska.edu/realtime/data/MPEG/PKR_DASC_256/<br> These files were converted into python pickle files and used internally for the rest of the investigation.</p> <p>The columns corresponds to days, and the rows correspond to time in UT as decimal hours:<br> The ASI Key is the following:<br> # 1 Discrete<br> # 2 Diffuse<br> # 3 Pulsating<br> # 4 Cloudy/Clear<br> # 5 Moon<br> # 6 Possible faint Aurora with moon out<br> # 7 Substorm Breakup<br> # 8 Cloudy with aurora (can't make out type)</p>
Optimizing Older Adults' Home Space for Physical Activity
ClinicalTrials.gov study NCT06407557. IPD Sharing: Not stated. Countries: 1. Publications: 1.
Evaluating the Impact of Improvements in Urban Green Space on Older Adults' Physical Activity and Wellbeing: a Natural Experimental Study
ClinicalTrials.gov study NCT03575923. IPD Sharing: NO. Countries: 1. Publications: 1.
Dataset for "Brain-wide neural recordings in mice navigating physical spaces enabled by a cranial exoskeleton"
<p>Dataset for "Brain-wide neural recordings in mice navigating physical spaces enabled by a cranial exoskeleton"</p>
The Emotional, Physical and Cognitive Benefits of Purposeful Green Space Activities on Seniors
ClinicalTrials.gov study NCT04913363. IPD Sharing: NO. Countries: 1. Publications: 0.
BUrst vs. Spaced Physical Therapy for Parkinson's Disease: The BUS PT Timing Trial
ClinicalTrials.gov study NCT05180747. IPD Sharing: YES. Countries: 1. Publications: 0.
Blue-green Space Physical Activity: the "Parco Del Mare" Study
ClinicalTrials.gov study NCT06533943. IPD Sharing: Not stated. Countries: 1. Publications: 0.
Change Physical Activity and School Play Space. Randomized Study Protocol.
ClinicalTrials.gov study NCT05020041. IPD Sharing: NO. Countries: 1. Publications: 0.
Space Life and Physical Sciences Research and Applications Program
Space Life and Physical Sciences Research and Applications Program
COHOWeb at the Space Physics Data Facility (SPDF)
Hourly-averaged deep space magnetic field, plasma, and ephemerides. This web service includes data from missions including Helios1, Helios2, OMNI_M, Pioneer10, Pioneer11, Pioneer Venus, Stereo-A, Stereo-B, Ulysses, Voyager1, Voyager2, Mariner2, Pioneer6, Pioneer7. The Space Physics Data Facility (SPDF) is the archive of non-solar data for the Heliospheric Science Division (HSD) at NASA's Goddard Space Flight Center.
FTPBrowser at the Space Physics Data Facility (SPDF)
FTPBrowser at GSFC/SPDF is an interface for graphical or digital display and/or retrieval of subsets of data that are in selected ones of SPDF's ftp-accessible ASCII or g-zipped ASCII data sets. The Space Physics Data Facility (SPDF) is the archive of non-solar data for the Heliospheric Science Division (HSD) at NASA's Goddard Space Flight Center.
SSC 4D Orbit Viewer Web Services API at the Space Physics Data Facility (SPDF)
This API allows any web application to offer an interactive 4D display of the trajectories of satellites known to SSCweb (Satellite Situation Center). The Space Physics Data Facility (SPDF) is the archive of non-solar data for the Heliospheric Science Division (HSD) at NASA's Goddard Space Flight Center.
SSCweb orbit locations at the Space Physics Data Facility (SPDF)
Display and download orbit and trajectory data for most heliophysics missions. The Satellite Situation Center (SSC) also enables complex queries between spacecraft and ground locations, tracing along magnetic field lines, and geophysical regions of space. The Space Physics Data Facility (SPDF) is the archive of non-solar data for the Heliospheric Science Division (HSD) at NASA's Goddard Space Flight Center.
GIFWalk at the Space Physics Data Facility (SPDF)
GIFWalk is an interface allowing the user to browse pre-generated data and orbit plots from missions including ACE, Cluster, Geotail, THEMIS, Polar, IMAGE, IMP 8, Wind, and Van Allen Probes (RBSP). The Space Physics Data Facility (SPDF) is the archive of non-solar data for the Heliospheric Science Division (HSD) at NASA's Goddard Space Flight Center.
OMNIWeb at the Space Physics Data Facility (SPDF)
Hourly-averaged near-Earth solar wind magnetic field and plasma, etc. The web services consists of OMNI data (spacecraft-interspersed, near-Earth solar wind data); spacecraft-specific data sets (near 1 AU, including near-Earth) including ACE, Geotail, IMP-8, IMP6&7, Wind, Explorer 33&35, Genesis, ISEE 3, Prognoz, SOHO, GOES, and Moon. Data also includes deep space data including COHOWeb-formatted hourly solar wind field and plasma, Pioneer, Ulysses, Voyager, Cassini, Helios, Mariner, and STEREO; and Interfaces for comparing multi-source data. The Space Physics Data Facility (SPDF) is the archive of non-solar data for the Heliospheric Science Division (HSD) at NASA's Goddard Space Flight Center.
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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.