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gptkbp:instance_of
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gptkb:space_mission
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gptkbp:analysis
|
image processing
spectral analysis
coronagraphic techniques
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gptkbp:availability
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publicly available
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gptkbp:collaboration
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gptkb:international_collaboration
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gptkbp:collaborator
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gptkb:European_Space_Agency
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gptkbp:collection
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remote sensing
in situ measurements
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gptkbp:community
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astrophysicists
solar physicists
space weather scientists
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gptkbp:community_outreach
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gptkb:educational_programs
workshops
scientific publications
public lectures
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gptkbp:data_type
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spectral data
imaging data
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|
gptkbp:data_usage
|
gptkb:space_weather_forecasting
astrophysics research
solar physics research
|
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gptkbp:funding
|
gptkb:European_Space_Agency
gptkb:NASA
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gptkbp:has_ability
|
multi-wavelength observations
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|
https://www.w3.org/2000/01/rdf-schema#label
|
Large Angle and Spectrometric Coronagraph Experiment
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gptkbp:impact
|
enhanced understanding of solar phenomena
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gptkbp:instruments
|
gptkb:spectrometer
gptkb:Coronaviridae
|
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gptkbp:launch_date
|
1996-04-02
|
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gptkbp:launch_site
|
gptkb:Kennedy_Space_Center
|
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gptkbp:launch_vehicle
|
gptkb:Space_Shuttle
|
|
gptkbp:legacy
|
improved solar models
advancements in coronagraph technology
influence on future solar missions
|
|
gptkbp:mission_duration
|
approximately 2 years
|
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gptkbp:mission_type
|
solar observation
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gptkbp:notable_mission
|
gptkb:Solar_Orbiter
gptkb:Parker_Solar_Probe
gptkb:SOHO
gptkb:STEREO
ACE
|
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gptkbp:objective
|
study the solar corona
|
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gptkbp:operated_by
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gptkb:NASA
|
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gptkbp:operational_status
|
completed
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gptkbp:resolution
|
high resolution
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gptkbp:scientific_goals
|
understand solar wind
map solar magnetic fields
observe solar flares
|
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gptkbp:successor
|
gptkb:Solar_and_Heliospheric_Observatory
|
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gptkbp:bfsParent
|
gptkb:Solar_and_Heliospheric_Observatory
gptkb:the_Solar_and_Heliospheric_Observatory
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gptkbp:bfsLayer
|
6
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