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Instruments > Solar/Space Observing Instruments > Ultraviolet Instruments > SEE

Preferred term

SEE  

Definition

  • The Solar EUV Experiment (SEE) is an experiment designed to measure the full-disk solar irradiance from 0.1 to 200 nm using a grating spectrograph and silicon photodiodes coated with thin film transmission filters. The spectral resolution of the measurements is 0.4 nm above 25 nm and about 7 nm below 25 nm. The solar sensors are designed to let the Sun drift through their field of view once per orbit, so only an one-axis pointing platform is employed for SEE. SEE is being designed and built primarily at the LASP Space Technology Building. The only major subcontract for the SEE instruments is to Schaeffer Magnetics, Inc. for the SEE pointing platform hardware. Additional information available at http://lasp.colorado.edu/see/ [Summary provided by the Laboratory for Atmospheric and Space Sciences] Group: Instrument_Details Entry_ID: SEE Group: Instrument_Identification Instrument_Category: Solar/Space Observing Instruments Instrument_Class: Ultraviolet Instruments Short_Name: SEE Long_Name: Solar EUV Experiment End_Group Group: Instrument_Associated_Sensors Short_Name: XUV-SEE Short_Name: EGS-SEE End_Group Group: Associated_Platforms Short_Name: TIMED End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Ultraviolet Spectral_Frequency_Coverage_Range: 0.1 - 200 nm Spectral_Frequency_Resolution: 0.4 nm and 7 nm End_Group Online_Resource: http://lasp.colorado.edu/see/ Sample_Image: http://lasp.colorado.edu/see/SEE_Instrument_Labels.JPG Group: Instrument_Logistics Data_Rate: 210 bps Instrument_Start_Date: 2001-12-07 Instrument_Owner: University of Colorado End_Group End_Group (en)

Broader concept

URI

https://gcmd.earthdata.nasa.gov/kms/concept/58cd5aaa-aa46-4104-af05-48c028d609f3

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