Parker solar wind model
E941945
The Parker solar wind model is a foundational theoretical framework that explains how the Sun’s hot corona expands outward as a continuous, supersonic stream of charged particles that shapes the heliosphere.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Parker solar wind model canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T11709856 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Parker solar wind model Context triple: [Parker spiral model of the interplanetary magnetic field, relatedTo, Parker solar wind model]
-
A.
Parker spiral model of the interplanetary magnetic field
The Parker spiral model of the interplanetary magnetic field describes how the Sun’s rotating, magnetized solar wind stretches the solar magnetic field into an Archimedean spiral shape throughout the heliosphere.
-
B.
Parker spiral model
The Parker spiral model is a theoretical description of the Sun’s magnetic field being wound into a spiral shape throughout the heliosphere by the combination of solar rotation and the outward-flowing solar wind.
-
C.
Integrated Science Investigation of the Sun
Integrated Science Investigation of the Sun is a suite of scientific instruments aboard NASA’s Parker Solar Probe designed to study energetic particles and their role in solar and heliospheric processes.
-
D.
Solar Wind Around Pluto
Solar Wind Around Pluto (SWAP) is an instrument aboard NASA’s New Horizons spacecraft designed to study how the solar wind interacts with Pluto’s atmosphere and the outer reaches of the solar system.
-
E.
Solar Wind Monitor
Solar Wind Monitor is a space-based instrument designed to measure and analyze the properties of the solar wind, such as its speed, density, and composition, to better understand solar-terrestrial interactions.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Parker solar wind model Target entity description: The Parker solar wind model is a foundational theoretical framework that explains how the Sun’s hot corona expands outward as a continuous, supersonic stream of charged particles that shapes the heliosphere.
-
A.
Parker spiral model of the interplanetary magnetic field
The Parker spiral model of the interplanetary magnetic field describes how the Sun’s rotating, magnetized solar wind stretches the solar magnetic field into an Archimedean spiral shape throughout the heliosphere.
-
B.
Parker spiral model
The Parker spiral model is a theoretical description of the Sun’s magnetic field being wound into a spiral shape throughout the heliosphere by the combination of solar rotation and the outward-flowing solar wind.
-
C.
Integrated Science Investigation of the Sun
Integrated Science Investigation of the Sun is a suite of scientific instruments aboard NASA’s Parker Solar Probe designed to study energetic particles and their role in solar and heliospheric processes.
-
D.
Solar Wind Around Pluto
Solar Wind Around Pluto (SWAP) is an instrument aboard NASA’s New Horizons spacecraft designed to study how the solar wind interacts with Pluto’s atmosphere and the outer reaches of the solar system.
-
E.
Solar Wind Monitor
Solar Wind Monitor is a space-based instrument designed to measure and analyze the properties of the solar wind, such as its speed, density, and composition, to better understand solar-terrestrial interactions.
- F. None of above. chosen
Statements (50)
| Predicate | Object |
|---|---|
| instanceOf |
astrophysical model
ⓘ
solar physics model ⓘ space plasma physics model ⓘ theoretical model ⓘ |
| appliesTo | stellar winds of other stars ⓘ |
| assumes |
collisionless plasma at large distances
ⓘ
radial symmetry ⓘ steady-state solar wind ⓘ |
| basedOn |
hydrodynamic equations
ⓘ
isothermal corona approximation ⓘ spherically symmetric outflow assumption ⓘ |
| coreConcept |
pressure-driven coronal expansion
ⓘ
supersonic stellar wind ⓘ |
| describes |
continuous outflow of plasma from the Sun
ⓘ
expansion of the solar corona ⓘ formation of the heliosphere ⓘ radial outflow of charged particles from the Sun ⓘ solar wind ⓘ supersonic flow of the solar wind ⓘ |
| developedBy | Eugene N. Parker NERFINISHED ⓘ |
| explains |
acceleration of the solar wind
ⓘ
existence of a critical point in solar wind flow ⓘ quasi-steady nature of the solar wind ⓘ transition from subsonic to supersonic solar wind ⓘ |
| field |
astrophysics
ⓘ
heliophysics ⓘ space plasma physics ⓘ |
| influenced |
design of interplanetary missions
ⓘ
modern heliospheric physics ⓘ space weather research ⓘ |
| involves |
plasma pressure gradient
ⓘ
radial distance from the Sun ⓘ solar corona temperature ⓘ solar gravitational field ⓘ |
| namedAfter | Eugene N. Parker NERFINISHED ⓘ |
| predicts |
existence of a critical point in the solar wind solution
ⓘ
finite mass loss rate from the Sun ⓘ pressure-driven outflow of coronal plasma ⓘ solar wind becomes supersonic beyond a critical radius ⓘ solar wind speed increases with distance from the Sun near the corona ⓘ |
| publicationYear | 1958 ⓘ |
| publishedIn | Astrophysical Journal NERFINISHED ⓘ |
| relatedTo | Parker spiral model of the interplanetary magnetic field ⓘ |
| testedBy |
ACE spacecraft observations
ⓘ
Helios spacecraft observations ⓘ Mariner 2 observations ⓘ Parker Solar Probe observations ⓘ Ulysses spacecraft observations ⓘ Wind spacecraft observations ⓘ in-situ spacecraft measurements of the solar wind ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
Instruction
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Input
Subject: Parker solar wind model Description of subject: The Parker solar wind model is a foundational theoretical framework that explains how the Sun’s hot corona expands outward as a continuous, supersonic stream of charged particles that shapes the heliosphere.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.