HKU DataHub + figshare + Loughborough Research Repository + UP Research Data Repository2026 · Astronomical catalogue
Electron Energy Transport at the Inflow Edge of the Electron Diffusion Region in Three-dimensional Magnetic Reconnection<p dir="ltr">Source data and reproduce code.</p>
figshare2026 · Astronomical catalogue
Catalog of sinuous rilles on Tharsis Montes' Rift Aprons, Mars<p dir="ltr">Sinuous rilles have been observed on the Moon, Venus, and Mars and appear to have been carved by hot, flowing lava. Sinuous rilles are observed on the slopes of three large shield volcanoes on Mars, collectively known as the Tharsis Montes, which occur in a line oriented NE-SW. Specifically, the sinuous rilles occur on the rift aprons - large fan-shaped deposits located to the southwe
figshare2026 · Astronomical catalogue
Data associated with “Quasi 6-day Wave Variability in the Thermosphere and Ionosphere: Observations and Modeling”<p dir="ltr">Satellite observations of the upper mesosphere and lower thermosphere from TIMED-SABER and ICON-MIGHTI reveal a clear Quasi 6-Day Wave (Q6DW) event in the winds and temperatures in this region. This Q6DW event is seen to be persistent in multiple datasets throughout the middle to upper thermosphere and the F-region ionosphere, including in observations from GOLD disk temperatures (TDi
figshare2026 · Astronomical catalogue
TIEGCM simulation data for the X2.2 solar flare on 6 September 2017<p dir="ltr">This dataset contains processed TIEGCM output used to study the equatorial wind jet response to the X2.2 solar flare on 6 September 2017. It includes zonal winds, neutral temperatures, electron densities, ion–neutral relative velocities, and momentum diagnostics at 450 km. The data are provided in MATLAB format, with variable definitions and units in the README.</p>
Teesside University Research Data Repository2026 · Astronomical catalogue
First Lidar Observations of Ionosphere–Thermosphere–Mesosphere (ITM) Na Transition Layer (~120–95 km): Regular Occurrence Over Boulder (40.13°N, 105.24°W) and Possible Formation MechanismsThe dataset published here supports the article entitled "First Lidar Observations of Ionosphere–Thermosphere–Mesosphere (ITM) Na Transition Layer (~120–95 km): Regular Occurrence Over Boulder (40.13°N, 105.24°W) and Possible Formation Mechanisms", submitted to Geophysical Research Letters (GRL) in 2026. The data are provided in MatLab format along with MatLab plotting code.
figshare2026 · Astronomical catalogue
<b>The Soon Joe Cavity as a Modelling Platform</b><p dir="ltr">The control programme of the series named orientation reversal — physically inverting the apparatus — as its most decisive test, on the reasoning that mains coupling and circuit response are indifferent to which way up a device is whereas a gravitational term is not. The recorded terminal voltages were being used to build a specific potential Ψ<sub>g</sub>, and through it the compactn
ZivaHub2026 · Astronomical catalogue
Adiabatic Modification of the Pitch Angle Distribution of Outer Radiation Belt Electrons by Large-scale Changes in Magnetic Fields<p dir="ltr">Calculated data for Figures 2, 5 and 7 in the paper "Adiabatic Modification of the Pitch Angle Distribution of Outer Radiation Belt Electrons by Large-scale Changes in Magnetic Fields "</p>
e-cienciaDatos2026 · Astronomical catalogue · unknown
Interplanetary Coronal Mass ejections multi-catalogThe main idea of the project is to gather the information of different Interplanetary Coronal Mass Ejections (ICMEs) seen by different spacecraft to obtain a combined catalog that ranges between 0.25 to 5 AU and between 1975 and 2022. This allows us to study statistically the different structures present in the ICMEs along with their evolution with distance and time. We have obtained a list of aro
Edmond2025 · Astronomical catalogue · unknown
TRAPPED (Testbed for Radiation and Plasma Planetary Environments Development): Energetic Particle DatasetsWithin the framework of the ESA's TRAPPED project (Testbed for Radiation and Plasma Planetary Environments), a collaborative effort by ONERA, IRAP, the Max Planck Institute for Solar System Research, and the Academy of Athens, has yielded a versatile, user-friendly environment model framework and associated software, tailored to gas giant planet moon systems and grounded in the rich datasets from
Teesside University Research Data Repository2025 · Astronomical catalogue
Relative Contributions of Lower-Atmosphere Tidal and Solar-Magnetospheric Forcings to the Day-to-Day Variability of F-region Electron DensityThis data contains simulations from three TIEGCM model runs for ionospheric electron density (Ne), and Ne tides at 300 km.
e-cienciaDatos2025 · Astronomical catalogue · unknown
World map of geomagnetic disturbances for 2003 (LDi-GMap 2003)The world map of geomagnetic disturbances are images of the world with contour plot of the level of geomagnetic disturbance in a scale from -9 to +9 (only integer numbers). The contour plots are also filled with a color corresponding for each level. Data input is obtained after processing measurements of the horizontal geomagnetic field taken at different observatories.
NASA Data Portal2025 · Astronomical catalogue · unknown
NASA Earth Exchange (NEX)The NASA Earth Exchange (NEX) represents a new platform for the Earth science community that provides a mechanism for scientific collaboration and knowledge sharing. NEX combines state-of-the-art supercomputing, Earth system modeling, workflow management, NASA remote sensing data feeds, and a knowledge sharing platform to deliver a complete work environment in which users can explore and analyze l
NASA Data Portal2025 · Astronomical catalogue · unknown
NASA Scientific Visualization Studio GalleriesThe Scientific Visualization Studio hosts a collection of media galleries on Earth, air, and space themes.
IVOA Registry (Virtual Observatory)2024 · Astronomical catalogue
Alma-Ata Station Neutron Monitor Data ServiceThe Alma-Ata Cosmic Ray Station operates the 18NM-64 neutron supermonitor at an altitude of 3340 meters above sea level, with a geomagnetic cutoff rigidity of 6.7 GeV. The station provides real-time, minute-level measurements of cosmic ray intensity, contributing to the international NMDB network. These data support the study of cosmic ray variations and space weather phenomena. The provided datas
Teesside University Research Data Repository2024 · Astronomical catalogue
Seasonal Variation in the Mesospheric Ca Layer and Ca+ Layer Simultaneously Observed over Beijing (40.41°N, 116.01°E)This dataset supports the article "Seasonal Variation in the Mesospheric Ca Layer and Ca+ Layer Simultaneously Observed over Beijing (40.41°N, 116.01°E) " . The data are provided in MatLab format. Plotting programs are also included.
e-cienciaDatos2022 · Astronomical catalogue · unknown
UAH VLF Antenna Python Software DevelopmentAbstract. Solar flares are powerful releases of electromagnetic energy in the solar atmosphere, which are observed at all wavelengths from radio waves to gamma-rays. For flaring monitoring, major agencies rely nowadays on measurements of solar soft X-ray emission such as from the GOES spacecraft observations, although other ground-based flare monitoring activity exist, e.g. in H-alpha observations
Teesside University Research Data Repository2022 · Astronomical catalogue
Tunis dataVLF data
e-cienciaDatos2021 · Astronomical catalogue · unknown
Local Geomagnetic index (LDi) for 2015 at different locationsThis local geomagnetic index indicates the perturbation of the geomagnetic field (horizontal component) for several locations. It is a measure of the external to the Earth irregular geomagnetic variations. It is obtained after removing a baseline and the daily regular variation from observed measurements. See also Files description.
e-cienciaDatos2021 · Astronomical catalogue · unknown
Local Geomagnetic index (LDi) for 1997 at different locationsThis local geomagnetic index indicates the perturbation of the geomagnetic field (horizontal component) for several locations. It is a measure of the external to the Earth irregular geomagnetic variations. It is obtained after removing a baseline and the daily regular variation from observed measurements. See also Files description.
e-cienciaDatos2021 · Astronomical catalogue · unknown
Local Geomagnetic index (LDi) for 2012 at different locationsThis local geomagnetic index indicates the perturbation of the geomagnetic field (horizontal component) for several locations. It is a measure of the external to the Earth irregular geomagnetic variations. It is obtained after removing a baseline and the daily regular variation from observed measurements. See also Files description.
e-cienciaDatos2021 · Astronomical catalogue · unknown
Local Geomagnetic index (LDi) for 2005 at different locationsThis local geomagnetic index indicates the perturbation of the geomagnetic field (horizontal component) for several locations. It is a measure of the external to the Earth irregular geomagnetic variations. It is obtained after removing a baseline and the daily regular variation from observed measurements. See also Files description.
e-cienciaDatos2021 · Astronomical catalogue · unknown
Local Geomagnetic index (LDi) for 2002 at different locationsThis local geomagnetic index indicates the perturbation of the geomagnetic field (horizontal component) for several locations. It is a measure of the external to the Earth irregular geomagnetic variations. It is obtained after removing a baseline and the daily regular variation from observed measurements. See also Files description.
e-cienciaDatos2021 · Astronomical catalogue · unknown
Local Geomagnetic index (LDi) for 2013 at different locationsThis local geomagnetic index indicates the perturbation of the geomagnetic field (horizontal component) for several locations. It is a measure of the external to the Earth irregular geomagnetic variations. It is obtained after removing a baseline and the daily regular variation from observed measurements. See also Files description.
e-cienciaDatos2021 · Astronomical catalogue · unknown
Local Geomagnetic index (LDi) for 2016 at different locationsThis local geomagnetic index indicates the perturbation of the geomagnetic field (horizontal component) for several locations. It is a measure of the external to the Earth irregular geomagnetic variations. It is obtained after removing a baseline and the daily regular variation from observed measurements. See also Files description.
e-cienciaDatos2021 · Astronomical catalogue · unknown
Local Geomagnetic index (LDi) for 2019 at different locationsThis local geomagnetic index indicates the perturbation of the geomagnetic field (horizontal component) for several locations. It is a measure of the external to the Earth irregular geomagnetic variations. It is obtained after removing a baseline and the daily regular variation from observed measurements. See also Files description.