Statements (47)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:Model
|
gptkbp:bfsLayer |
5
|
gptkbp:bfsParent |
gptkb:In_Return
|
gptkbp:analyzes |
solar magnetic fields
solar atmosphere solar interior |
gptkbp:applies_to |
gptkb:observatory
|
gptkbp:based_on |
gptkb:physicist
observational data |
gptkbp:collaborates_with |
gptkb:spacecraft
observatories |
gptkbp:contributed_to |
stellar astrophysics
|
gptkbp:developed_by |
solar physicists
|
https://www.w3.org/2000/01/rdf-schema#label |
Sun Models
|
gptkbp:impact |
solar energy research
|
gptkbp:includes |
gptkb:Standard_Solar_Model
3 D models 1 D models Helioseismic Models Solar Evolution Models magnetohydrodynamic models |
gptkbp:influenced_by |
theoretical advancements
technological improvements |
gptkbp:influences |
space weather predictions
|
gptkbp:involves |
parameter estimation
data assimilation |
gptkbp:is_compared_to |
other stellar models
|
gptkbp:is_considered |
solar observations
helioseismology |
gptkbp:is_critical_for |
understanding stellar evolution
predicting solar impacts on Earth |
gptkbp:is_described_as |
gptkb:coronal_mass_ejections
solar flares solar cycles the structure of the Sun |
gptkbp:is_informed_by |
climate science
|
gptkbp:is_used_for |
understanding solar dynamics
predicting solar activity studying solar radiation |
gptkbp:origin |
historical solar models
|
gptkbp:provides |
insight into solar magnetic activity
insight into solar wind |
gptkbp:requires |
advanced algorithms
high-performance computing |
gptkbp:supports |
gptkb:railway_station
|
gptkbp:utilizes |
numerical simulations
computational methods |