OMI Solar Spectral Irradiance Data ################################## Authors: Sergey Marchenko and Matthew DeLand Contact: sergey.marchenko@ssaihq.com Last revision: 3 November 2022 Data Product ************ This file gives a basic description of the solar spectral irradiance data that we have produced from Aura OMI solar measurements. Detailed discussion of the procedures used and validation steps can be found in the following papers: S. V. Marchenko and M. T. DeLand (2014), "Solar spectral irradiance changes during Cycle 24", Ap. J. 789:117, doi:10.1088/0004-637X/789/2/117. S. V. Marchenko, M. T. DeLand, and J. L. Lean (2016), "Solar spectral irradiance variability in Cycle 24: Observations and models", J. Space Weather Space Climate, 6, A40, doi:10.1051/swsc/2016036. S. V. Marchenko, T. N. Woods, M. T. DeLand, S. Mauceri, P. Pilewskie, and M. Haberreiter (2019), Improved Aura/OMI solar spectral irradiances: Comparisons with independent data sets and model predictions, Earth and Space Sci., 6, 2379-2396, doi:10.1029/2019EA000624. We designate this dataset as Version 5 ('_v5') to recognize the use of the Collection 4 OMI L1B data, as described by Kleipool et al. [2022]. Other changes from the Version 3 OMI SSI product described in our 2019 paper were previously incorporated in our Version 4 product, and include the following items: 1. The instrument degradation model is now based on data from all three OMI channels (UV1, UV2, VIS) for better spectral consistency. 2. The averaging period used to define our solar minimum reference spectrum has been shifted to cover 1 July 2008 - 30 April 2009. This provides symmetric coverage around the sunspot minimum at ~2008.9 shown in NOAA NGDC (National Geophysical Data Center) data. 3. The filtering process to remove instrument noise has been revised to improve flexibility. 4. The SSI data are provided on a 0.5 nm wavelength grid for consistency with the OMI spectral resolution (~0.4-0.6 nm). Kleipool, Q., et al. (2022). Ozone Monitoring Instrument (OMI) collection 4: establishing a 17-year-long series of detrended level-1b data. Atmos. Meas. Tech., 15, 3527-3533, doi:10.5194/amt-15-3527-2022. Data Location ************* The OMI data can be retrieved at the following web site: https://sbuv2.gsfc.nasa.gov/solar/omi/ File Contents ************* The OMI irradiance data, corrected for long-term degradation, are provided in a single IDL save set named 'corrected_solar_flux_regular_diff_v5_nov2022.sav'. All data are provided separately for each of three spectral channels, where the term 'CHN' in the variable name has the following definitions: 'uv1' = UV1 channel, wavelength range = 265.0-309.5 nm 'uv2' = UV2 channel, wavelength range = 310.0-364.5 nm 'vis' = VIS channel, wavelength range = 365.0-500.0 nm The save set contains the following variables, where 'CHN' is defined as above for each channel: JUL_DATE Observation date in adjusted Julian day format [JD-2450000.0] chn_REFERENCE Reference irradiance spectrum created by averaging data between July 2008 and April 2009 [photons/cm^2/sec/nm] chn_BIN Daily spectra, expressed as normalized irradiance relative to the reference spectrum irradiance value at each wavelength chn_BIN_STD Normalized standard deviation within each spectral and daily bin LA_chn Wavelength scale [nm], sample interval = 0.5 nm For users who prefer to use data in HDF format, the file 'omi_ssi_update_v5_20221103.h5' is also available. It contains the same information as the IDL save set, with the following mapping of variables: JUL_DATE --> JulianDateAdj chn_REFERENCE --> IrradianceReference{chn} chn_BIN --> IrradianceNormalized{chn} chn_BIN_STD --> IrradianceStDev{chn} LA_chn --> Wavelength{chn} The first measurement date available in the OMI data product is 2 July 2006, and the last date included in the current data file is 24 July 2022.