|
gptkbp:instance_of
|
gptkb:Coronaviridae
|
|
gptkbp:can_detect
|
plasma structures
|
|
gptkbp:collaborated_with
|
astrophysicists
|
|
gptkbp:contributes_to
|
understanding of solar flares
|
|
gptkbp:designed_for
|
observing solar corona
|
|
gptkbp:developed_by
|
gptkb:NASA
cutting-edge technology
scientific teams
|
|
gptkbp:first_introduced
|
solar observations
|
|
gptkbp:has_applications_in
|
gptkb:space_weather_forecasting
|
|
gptkbp:helps_study
|
gptkb:wind
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Visible Emission Line Coronagraph
|
|
gptkbp:instrument
|
advanced sensors
spectrometers
|
|
gptkbp:is_analyzed_in
|
data scientists
data accuracy
accurate measurements
solar magnetic fields
|
|
gptkbp:is_associated_with
|
solar physics advancements
|
|
gptkbp:is_capable_of
|
multi-wavelength observations
|
|
gptkbp:is_collaborative_with
|
academic institutions
international space organizations
|
|
gptkbp:is_connected_to
|
solar research initiatives
|
|
gptkbp:is_critical_for
|
understanding solar activity
|
|
gptkbp:is_designed_to
|
reduce light pollution
|
|
gptkbp:is_documented_in
|
gptkb:literature
research papers
|
|
gptkbp:is_enhanced_by
|
computer algorithms
|
|
gptkbp:is_equipped_with
|
advanced imaging technology
|
|
gptkbp:is_evaluated_by
|
peer reviews
|
|
gptkbp:is_fundamental_to
|
solar system studies
|
|
gptkbp:is_funded_by
|
government agencies
|
|
gptkbp:is_incorporated_in
|
gptkb:space_mission
|
|
gptkbp:is_integrated_with
|
gptkb:satellite
data analysis tools
|
|
gptkbp:is_involved_in
|
gptkb:space_mission
international collaborations
|
|
gptkbp:is_optimized_for
|
high sensitivity
|
|
gptkbp:is_part_of
|
gptkb:NASA_missions
gptkb:solar_dynamics_observatory
solar observation missions
solar observation technology
solar observation programs
NASA's solar exploration strategy
|
|
gptkbp:is_promoted_by
|
scientific communities
|
|
gptkbp:is_promoted_through
|
educational outreach
|
|
gptkbp:is_recognized_by
|
scientific organizations
|
|
gptkbp:is_related_to
|
solar observatories
|
|
gptkbp:is_significant_for
|
solar physics research
|
|
gptkbp:is_studied_for
|
gptkb:coronal_mass_ejections
|
|
gptkbp:is_subject_to
|
scientific scrutiny
|
|
gptkbp:is_supported_by
|
collaborative research
scientific grants
scientific funding agencies
|
|
gptkbp:is_tested_for
|
laboratory conditions
|
|
gptkbp:is_used_for
|
gptkb:scientists
|
|
gptkbp:is_used_in
|
space telescopes
|
|
gptkbp:is_utilized_by
|
researchers worldwide
|
|
gptkbp:is_utilized_for
|
educational purposes
|
|
gptkbp:is_utilized_in
|
research projects
public outreach programs
|
|
gptkbp:key
|
understanding solar phenomena
|
|
gptkbp:measures
|
magnetic fields
|
|
gptkbp:monitors
|
solar activity levels
|
|
gptkbp:operates_in
|
near-ultraviolet spectrum
|
|
gptkbp:presented_by
|
conferences
|
|
gptkbp:proposed_by
|
the 1990s
|
|
gptkbp:provides
|
high-resolution images
|
|
gptkbp:uses
|
visible light
|
|
gptkbp:bfsParent
|
gptkb:Aditya-L1
|
|
gptkbp:bfsLayer
|
5
|