Space mission
SOHO (Solar and Heliospheric Observatory)
A joint ESA/NASA solar observatory at the Sun–Earth L1 point, operating since 1995. Its coronagraphs image coronal mass ejections and it is a workhorse of space-weather monitoring (and a prolific comet discoverer).
- Type
- Space mission
- Domain
- Scientific connections
- Connections
- 3
- Type: Space mission
- Domain: Scientific connections
Experience system V6
Mission dossier
A mission-story layout that emphasizes target bodies, spacecraft, timeline, agency, and evidence-backed status.
- 01
Observe
The page falls back to graph and source evidence when no cleared image is available.
- 02
Measure
Measurement panels use graph coverage, catalog identifiers, and source availability without inventing values.
- 03
Locate
Observes Solar Flare.
- 04
Connect
3 graph relations shape the knowledge viewport.
- Object type
- Space mission
- Graph relations
- 3
- Verified sources
- 2
- Image records
- 0
- Domain
- Scientific connections
- Status
- Graph entity
Scientific map
Mission context
- Observes
Solar Flare
- Observes
Coronal Mass Ejection (CME)
- Associated with
The Solar Corona
Original SVG diagram
Mission architecture
- Agency
- Not recorded
- Launch year
- Not recorded
- Mission type
- Not recorded
- Status
- Not recorded
Visual knowledge graph
Relationships, not isolated facts
This viewport is generated from the Asteria knowledge graph. Science, culture, and interpretive links remain separated by domain so visual context never changes the evidentiary meaning of a relation.
- ObservesCoronal Mass Ejection (CME)
- ObservesSolar Flare
- Associated withThe Solar Corona
Continue the atlas
Curated next objects
Solar Flare
A sudden, intense burst of radiation from the Sun's surface, released when magnetic energy in the corona is explosively reconfigured. The X-rays arrive in minutes and can ionise Earth's upper atmosphere, causing radio blackouts.
space weather phenomenonCoronal Mass Ejection (CME)
An enormous eruption of magnetised plasma from the Sun's corona, launching billions of tonnes of material into space. When aimed at Earth, a CME can drive the largest geomagnetic storms one to three days later.
solar regionThe Solar Corona
The Sun's outermost atmosphere — a tenuous, million-degree plasma extending millions of kilometres into space, visible to the eye only during a total solar eclipse or with a coronagraph. Far hotter than the surface beneath it, it is shaped by magnetic fields into loops, holes, and streamers, and it continually expands outward as the solar wind.
stellar physics conceptMagnetic Reconnection
The process by which oppositely directed magnetic field lines break and reconnect, converting stored magnetic energy explosively into heat, light, and fast particles. Reconnection powers solar flares and helps launch coronal mass ejections, and is a fundamental plasma process seen throughout the Universe.
starThe Sun
The Sun is the star at the center of the Solar System, around which the planets and other bodies orbit.
space weather phenomenonActive Regions
Areas of strong, complex magnetic field on the Sun, usually marked by sunspots, where magnetic energy builds up and is released. Active regions are the launch sites of the largest solar flares and coronal mass ejections, and are watched closely for space-weather forecasting.
Data
Scientific data & provenance
Data & provenance
- Stable ID
space_mission:soho- Type
- Space mission
- Domain
- Scientific connections
- Relationships
- 3
- Graph version
- 1.0.0
Dataset membership
Open data
In the graph export: graph.json · graph.jsonld
Planned API: GET /api/v0/entities/space_mission:soho
Scientific quality
Partial3 of 7 applicable dimensions complete
- Description
- Complete
- Source coverage
- Complete
- Relationship coverage
- Complete
- Review coverage
- None
- Citation coverage
- None
- Image coverage
- None
- Timeline coverage
- None
Scientific entity. Dimensions that cannot apply to this object are excluded rather than counted as gaps. See the evidence framework and authority dashboard.
You might also explore
- Stellar physics conceptMagnetic ReconnectionLinked through Solar Flare
- StarThe SunLinked through Solar Flare
- Space-weather phenomenonActive RegionsLinked through Solar Flare
- Solar featureCoronal LoopLinked through The Solar Corona
- Solar featureCoronal StreamerLinked through The Solar Corona
- PlanetEarthLinked through Solar Flare
Sources & references
The primary and reference sources this topic draws on.
- ESAEuropean Space Agency
European missions, observatories, and space science imagery.
- 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.