2.2.9 spase://NASA/NumericalData/LANL/Avg/SOPA/PT1D LANL Daily-averaged electron fluxes from the Synchronous Orbit Particle Spectrometer (SOPA) 2020-07-07T21:14:45Z Daily-averaged electron fluxes from the Los Alamos National Laboratory (LANL) Synchronous Orbit Particle Spectrometer (SOPA) Daily averages from each geosynchronous satellite available on any given day were merged into a single, uniform daily average. Data span 22 September, 1989 through 31 December, 2009. Data are log(flux) with flux in units of electrons /(cm^2.s.sr.keV). The original SOPA data channels have been fit to a bi-Maxwelian spectra. Fluxes are evaluated at virtual "channels" for fixed energies (i.e. not for an energy passband or integral thresholds) [see 2010JA015735 _LANL_Data_and_Processing for details] (2010ja015735-readme.txt) spase://SMWG/Person/Geoffrey.D.Reeves DataProducer spase://SMWG/Person/Steven.Karl.Morley DataProducer spase://SMWG/Person/Reiner.Friedel DataProducer spase://SMWG/Person/Michael.G.Henderson DataProducer spase://SMWG/Person/Thomas.E.Cayton DataProducer spase://SMWG/Person/Glenn.F.Cunningham DataProducer spase://SMWG/Person/J.Bernard.Blake DataProducer On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake revisited https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2010JA015735 Describes the processing performed on the SOPA and ESP data that were included in Reeves et. al, 2011 Electronic supplement to "On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake Revisited” https://agupubs.onlinelibrary.wiley.com/action/downloadSupplement?doi=10.1029%2F2010JA015735&attachmentId=69009962 Detailed information concerning instruments used, algorithm, and the resulting caveats of usage for data set. 2010ja015735-readme.txt https://agupubs.onlinelibrary.wiley.com/action/downloadSupplement?doi=10.1029%2F2010JA015735&attachmentId=69009961 Readme file with basic information on processing performed. spase://ViRBO/NumericalData/LANL/SOPA/PT1D spase://VSPO/NumericalData/LANL/Avg/SOPA/PT1D spase://SMWG/Repository/AGU/JGR Online Download link for daily avg. of log LANL-GEO SOPA Avg. Daily Flux https://agupubs.onlinelibrary.wiley.com/action/downloadSupplement?doi=10.1029%2F2010JA015735&attachmentId=69009964 Daily-averaged electron fluxes from the Los Alamos National Laboratory (LANL) Synchronous Orbit Particle Spectrometer (SOPA) Daily averages from each geosynchronous satellite available on any given day were merged into a single, uniform daily average. Data span 22 September, 1989 through 31 December, 2009. Data are log(flux) with flux in units of electrons /(cm^2.s.sr.keV). The original SOPA data channels have been fit to a bi-Maxwelian spectra. Fluxes are evaluated at virtual "channels" for fixed energies (i.e. not for an energy passband or integral thresholds). Text ASCII Reeves, G. D., S. K. Morley, R. H. W. Friedel, M. G. Henderson, T. E. Cayton, G. Cunningham, J. B. Blake, R. A. Christensen, and D. Thomsen (2011), On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake revisited, J. Geophys. Res., 116, A02213, doi:10.1029/2010JA015735. Calibrated Daily-averaged electron fluxes from the Los Alamos National Laboratory (LANL) Energetic Spectrometer for Particles (ESP) spase://SMWG/Instrument/LANL/1989/SOPA spase://SMWG/Instrument/LANL/1990/SOPA spase://SMWG/Instrument/LANL/1991/SOPA spase://SMWG/Instrument/LANL/1994/SOPA spase://SMWG/Instrument/LANL/1997/SOPA spase://SMWG/Instrument/LANL/01A/SOPA spase://SMWG/Instrument/LANL/02A/SOPA EnergeticParticles 1989-02-08T00:00:00 2010-01-01T00:00:00 PT24H Earth.Magnetosphere "Only limited ‘cleaning’ of this data set is performed prior to daily averaging and merging. Any detected failures of the fitting procedure are first removed from the data archive prior to daily averaging. A small fraction of daily-averaged flux values appear to be unphysically high. A basic ‘cleaning’ is done by excluding any data points at which the evaluated daily average flux at more than four energies is over four standard deviations above the mean daily flux for each satellite. We stress that these unphysical values represent only a small fraction of the data set – many, but not all of these values are removed by the basic pre-processing applied here – and work is continuing to improve this data set. It should be noted that the very highest and lowest evaluated energies are extrapolated using the fits and may be less reliable than those energies within the detection limits of the instrument." (Electronic supplement to "On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake Revisited”) Date Date, YYYY-MM-DD PT24H Temporal E1 - .0241MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .0241MeV. PT24H electrons/cm^2/keV/s/sr Electron NumberFlux .0241 .0241 10^6 eV E2 - 0.0317 MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .0317MeV. PT24H #/cm^2/keV/s/sr Electron NumberFlux .0317 .0317 10^6 eV E3 - .0.0416MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of 0.0416MeV. PT24H #/cm^2/keV/s/sr Electron NumberFlux 0.0416 0.0416 MeV E4 - .0625MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .0625MeV. PT24H electrons/cm^2/keV/s/sr nan Electron NumberFlux .0625 .0625 10^6 eV E5 - .0900MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .0900MeV. PT24H electrons/cm^2/keV/s/sr Electron NumberFlux .0900 .0900 MeV E6 - .1275MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .1275MeV. PT24H electrons/cm^2/keV/s/sr Electron NumberFlux .1275 .1275 10^6 eV E7 - .1725MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .1725MeV. PT24H electrons/cm^2/keV/s/sr Electron NumberFlux .1725 .1725 10^6 eV E8 - .2700MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .2700MeV. PT24H #/cm^2/keV/s/sr Electron NumberFlux .2700 .2700 10^6 eV E9 - .4075MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .4075MeV. PT24H #/cm^2/keV/s/sr Electron NumberFlux .4075 .4075 10^6 eV E10 - .6250MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .6250MeV. PT24H electrons/cm^2/keV/s/sr Electron NumberFlux .6250 .6250 10^6 eV E11 - .9250MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of .9250MeV. PT24H #/cm^2/keV/s/sr Electron NumberFlux .9250 .9250 MeV E12 - 1.3000MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of 1.3000MeV. PT24H #/cm^2/keV/s/sr nan Electron NumberFlux 1.3000 1.3000 10^6 eV E13 - 2.0000MeV Base 10 logarithm of daily-averaged SOPA flux measurements selected for each day. Data are for a virtual channel at an energy of 2.0000MeV. PT24H electrons/cm^2/keV/s/sr nan Electron NumberFlux 2.0000 2.0000 10^6 eV