2.2.2 spase://NASA/NumericalData/TIMED/SEE/L2_EGS TIMED SEE Level2 EGS Solar Irradiance Data 2020-07-07T21:15:38Z The EUV Grating Spectrograph (EGS) aboard SEE performs measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. The Level 2 data is time averaged over the entire day, after being 1-AU corrected and removing flares. The 1-AU correction is provided. NASA, Thomas N. Woods spase://SMWG/Person/Thomas.N.Woods PrincipalInvestigator L2 EGS Data Information http://lasp.colorado.edu/home/see/data/daily-averages/level-2-egs/ spase://VITMO/NumericalData/TIMED/SEE/L2_EGS spase://VSPO/NumericalData/TIMED/SEE/L2_EGS spase://SMWG/Repository/TIMED/SEE_POC Online Open SEE Data Products web page http://lasp.colorado.edu/home/see/data/ This web page allows the request of data files for this product. To request data: for the EGS data type of interest, click the year of interest to go the the ftp directory of files and download the desired day-long file by clicking on it. NetCDF None NASA, Thomas N. Woods Calibrated SEE Level 2 EGS Solar Irradiance data Level 2 10 spase://SMWG/Instrument/TIMED/SEE Irradiance 2002-02-08T00:00:00.000 P2D Sun TIMED SEE EGS Sun DATE DATE Date of observation YYYYDOY 1 Other Wavelength intervals WAVE Array of wavelength intervals, half-Angstrom centers nm 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other EGS median solar irradiance FLUX_MEDIAN Array of median solar irradiances for each wavelength interval. This is the spectrum. W / m^2 / nm 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Electromagnetic Wavelength 26.05 194.95 nm Differences between the median and weighted averaged solar irradiances DIFF_MA Array of differences between the median and weighted averaged solar irradiances for each wavelength interval W / m^2 / nm 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Accuracy of solar irradiance ERR_TOT Accuracy of solar irradiance Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Measurement precision ERR_MEAS Measurement precision Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Standard deviation of the median STDEV_MEAS Standard deviation of the median Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Number of points used in determining the daily average NUMPT Array of the Number of points (1-Angstrom-gridded measurements) used in determining the daily average for each wavelength interval 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other AU correction factor COR_1AU AU correction factor for date 1 / (AU^2) 1 Other Order Sorting correction applied to flux_median COR_OS_MED Order Sorting correction applied to flux_median W/m^2/nm 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Order Sorting correction applied to weighted avg irradiance COR_OS_AVG Order Sorting correction applied to weighted avg irradiance W/m^2/nm 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Degradation function linear extrapolation/interpolation flag DEGRADE_MODEL Long value = 1 if degradation function is linearly extrapolated, 0 if linearly interpolated 1 Other Averaged atmospheric correction factors COR_ATMOS.AVG Array of Averaged atmospheric correction factors for each wavelength interval Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Minimum atmospheric correction factors COR_ATMOS.MIN Array of Minimum atmospheric correction factors Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Maximum atmospheric correction factors COR_ATMOS.MAX Array of Maximum atmospheric correction factors Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Average instrument degradation correction factors COR_DEGRADE.AVG Array of Average instrument degradation correction factors Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Minimum instrument degradation correction factors COR_DEGRADE.MIN Array of Minimum instrument degradation correction factors Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other Maximum instrument degradation correction factors COR_DEGRADE.MAX) Array of Maximum instrument degradation correction factors Fractional 1690 Dimensions: [Number_of_wavelength_intervals] - where Number_of_wavelength_intervals is the number of wavelength intervals. Other