2.3.0 spase://NOAA/NumericalData/GOES/12/SEM/Z/PT5M GOES 12 Space Environment Monitor Data, X-ray, Magnetic Field, Electrons and Corrected Proton Channels, at 5 min Time Resolution GOES 12 SEM data 2019-10-11T16:15:00Z This GOES 12 SEM data set contains various parameters at 5 min time resolution. Within the data files is the Xray flux for two wavelength ranges, the magnetic field vectors, the >2 MeV uncorrected electron fluxes, and the corrected proton fluxes for several energy ranges. NOAA Environmental Research Laboratories, Terry G. Onsager, Howard J. Singer spase://SMWG/Person/Terry.Onsager PrincipalInvestigator spase://SMWG/Person/Howard.J.Singer PrincipalInvestigator spase://SMWG/Person/James.M.Weygand MetadataContact GOES 12 Space Environment Monitor https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=2001-031A-03 Introduction to the GOES 12 space environment monitor. GOES 12 Space Environment Monitor https://satdat.ngdc.noaa.gov/sem/goes/goes_docs/full/readme.txt Additional GOES Triaxial Fluxgate Magnetometer information. GOES 12 Triaxial Fluxgate Magnetometer Example ASCII file https://satdat.ngdc.noaa.gov/sem/goes/software/mag.txt Additional GOES Triaxial Fluxgate Magnetometer header information. spase://VMO/NumericalData/GOES/12/SEM/Z/PT5M spase://VSPO/NumericalData/GOES/12/SEM/Z/PT5M spase://SMWG/Repository/NOAA/SEC Online Open Direct access to the GOES 12 SEM data https://satdat.ngdc.noaa.gov/sem/goes/data/avg/ Direct link to the GOES 12 SEM data in ASCII format as well as the energetic particle data from other GOES spacecraft. The data are sorted by year. The file names indicates the data type, spacecraft number, year, month, and resolution. For example, A0558606.FIT indicates the type of particle data (A) for spacecraft 5 (05) at 5 min time resolution (5) from June 1986 (8606). Text None NOAA Environmental Research Laboratories, Terry G. Onsager, Howard J. Singer Calibrated NOAA GOES 12 SEM Level-0 spase://SMWG/Instrument/GOES/12/SEM EnergeticParticles MagneticField Irradiance 2003-01-01T00:00:00 2010-09-30T00:00:00 Time format in data files is YYMMDD HHMM DOY (2-digit year, 2-digit month, 2-digit day, 2-digit hour, 2-digit minute, and 3-digit day of year. PT5M 5 min geosynchronous GOES energetic particle monitor energetic particles magnetic field xray monitor Date and Time Time Time is given in 3 columns. Time format in data files is YYMMDD HHMM DOY (2-digit year, 2-digit month, 2-digit day, 2-digit hour, 2-digit minute, and 3-digit day of year. 3 Time array YYMMDD (2-digit year, 2-digit month, 2-digit day) 1 YYMMDD HHMM (2-digit hour, 2-digit min) 2 HHMM Day of Year 3 DOY d Temporal Solar X-ray Monitor Solar X-ray Flux Solar X-ray monitor flux in Two different wavelength ranges in units of W/m^2 W/m^2 2 Solar X-ray monitor fluxes from two wavelength ranges: 1 to 8 Å and 0.5 to 4 Å 1 to 8 Å X-ray Fluxes 1 XL 0.5 to 3.0 Å X-ray Flux 2 XS 3.27E+04 Photon Scalar Intensity Magnetic Field Sensor Magnetic Field Vectors at 5 min Time Resolution Data in Spacecraft Coordinates Magnetic Field Vectors Magnetic field vector for GOES 12 in spacecraft coordinates in units of 0.1 nT. The values must be divided by a factor of 10 to nT. HP is parallel to the satellite spin axis, which is itself: perpendicular to the orbital plane of the spacecraft. HE lies parallel: to the satellite-earth center line and points earthward. HN is: perpendicular to both HP and HE, and points eastward for GOES 12. 0.1*nT 1.0e-10>T Cartesian SC 4 HP is parallel to the satellite spin axis, which is itself: perpendicular to the orbital plane of the spacecraft. HE lies parallel: to the satellite-earth center line and points earthward. HN is: perpendicular to both HP and HE, and points eastward for GOES 12. Magnetic "Northward" Component Component.I 1 Hp Magnetic "Earthward" Component Component.J 2 He Magnetic "Eastward" Component Component.K 3 Hn Total Magnetic Field Magnitude 4 Ht 327.11 Vector Magnetic 2 MeV electrons E1 Uncorrected ≥2 MeV electrons number fluxes in units of counts/(cm^2 s sr). These values are especially unreliable during ion storms. (cm^2 s sr)^-1 Electron Magnitude NumberFlux Corrected Protons Protons Corrected Proton number fluxes in units of counts/(cm^2 s sr MeV) for 7 different energy channels. (cm^2 s sr MeV)^-1 7 Each Name provides the energy range for each channel. 0.8 to 4.0 MeV protons in counts/(cm^2 s sr MeV), Corrected Scalar 1 P1 4 to 9 MeV protons in counts/(cm^2 s sr MeV), Corrected Scalar 2 P2 9 to 15 MeV protons in counts/(cm^2 s sr MeV), Corrected Scalar 3 P3 15 to 40 MeV protons in counts/(cm^2 s sr MeV), Corrected Scalar 4 P4 40 to 80 MeV protons in counts/(cm^2 s sr MeV), Corrected Scalar 5 P5 80 to 165 MeV protons in counts/(cm^2 s sr MeV), Corrected Scalar 6 P6 165 to 500 MeV protons in counts/(cm^2 s sr MeV), Corrected Scalar 7 P7 3.27E+04 Proton Scalar NumberFlux 1