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AsteriaStar
Dataset

Solar Physics & Heliosphere Dataset

The Sun from core to heliosphere — the concentric interior zones and atmosphere layers (solar regions), the surface and atmospheric features (granulation, prominences, filaments, plages, spicules, coronal loops, streamers), and the structures of the heliosphere (Parker spiral, termination shock, heliosheath, bow wave). Reuses the Sun, the space-weather phenomena, and the solar observatories. Only well-established solar physics; nothing fabricated.

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Generated from the canonical knowledge graph. Open, machine-readable, and free to reuse under CC BY-SA 4.0.

Version
1.0.0
Entities
21
Last generated
2026-06-29
License
CC BY-SA 4.0
Checksum
(published at release)

Sample (21 of 21)

NameType
Coronal LoopSolar feature
Coronal StreamerSolar feature
FilamentSolar feature
GranulationSolar feature
PlageSolar feature
Polar Coronal PlumeSolar feature
ProminenceSolar feature
SpiculeSolar feature
SupergranulationSolar feature
The ChromosphereSolar region
The Convection ZoneSolar region
The HeliosheathHeliosphere structure
The Heliospheric Bow WaveHeliosphere structure
The Parker SpiralHeliosphere structure
The PhotosphereSolar region
The Radiative ZoneSolar region
The Solar CoreSolar region
The Solar CoronaSolar region
The TachoclineSolar region
The Termination ShockHeliosphere structure
The Transition RegionSolar region

Source references

The primary and reference sources this topic draws on.

  • NASANational Aeronautics and Space Administration

    Mission data, planetary science, space telescopes, and public-domain imagery.

    Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.

  • ESAEuropean Space Agency

    European missions, observatories, and space science imagery.