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Data from New Horizons Solar Wind Around Pluto instrument. Elliott, H. A., D. J. McComas, P. Valek, G. Nicolaou, S. Weidner, and G. Livadiotis (2016), ApJS, 223(2), 1-21, doi:10.3847/0067-0049/223/2/19. McComas, D. et al. (2008), The Solar Wind Around Pluto (SWAP) Instrument Aboard New Horizons, Space Sci Rev, 140(1), 261-313, doi:10.1007/s11214-007-9205-3.
Data from New Horizons Solar Wind Around Pluto instrument. Elliott, H. A., D. J. McComas, P. Valek, G. Nicolaou, S. Weidner, and G. Livadiotis (2016), ApJS, 223(2), 1-21, doi:10.3847/0067-0049/223/2/19. McComas, D. et al. (2008), The Solar Wind Around Pluto (SWAP) Instrument Aboard New Horizons, Space Sci Rev, 140(1), 261-313, doi:10.1007/s11214-007-9205-3.
THe histogram data set is before the culling described in McComas et al. (2017), for times when the solar wind speed varied over the ~24 hour period by >1% (~13% of the samples) or when the PUI fitting routine experienced a failing (see McComas et al. 2017 for more details).
Data from New Horizons Solar Wind Around Pluto instrument. Elliott, H. A., D. J. McComas, P. Valek, G. Nicolaou, S. Weidner, and G. Livadiotis (2016), ApJS, 223(2), 1-21, doi:10.3847/0067-0049/223/2/19. McComas, D. et al. (2008), The Solar Wind Around Pluto (SWAP) Instrument Aboard New Horizons, Space Sci Rev, 140(1), 261-313, doi:10.1007/s11214-007-9205-3.
TIROS/NOAA SEM MEPED Data Archive This is the re-processed version of the MEPED (Medium Energy Proton Electron Detector) data archive from the TIROS/NOAA spacecraft. The raw data from the NOAA archive have been processed to 1 minute resolution; magnetic field parameters (GSM Bx, By, Bz, B/Bmin, and L) are derived in 4 magnetic field models: IGRF, Tsyganenko 89 (T89), Tsyganenko 96 (T96), Tsyganenko 01 (T01); T89, T96, and T01 magnetic field models are driven with solar wind parameters and geomagnetic indices obtained from OMNI-2 data detector counts, omni and perpendicularelectron and proton flux are archived. Details of the processing can be found from .http://radbelts.gsfc.nasa.gov. Processing was done by: Shing F. Fung, Lun C. Tan, Xi Shao Space Physics Data Facility Goddard Space Flight Center, NASA Greenbelt, MD 20771 USA . e-mail: Shing.F.Fung@nasa.gov
Created Sept. 2005
TIROS/NOAA SEM MEPED Data Archive This is the re-processed version of the MEPED (Medium Energy Proton Electron Detector) data archive from the TIROS/NOAA spacecraft. The raw data from the NOAA archive have been processed to 1 minute resolution; magnetic field parameters (GSM Bx, By, Bz, B/Bmin, and L) are derived in 4 magnetic field models: IGRF, Tsyganenko 89 (T89), Tsyganenko 96 (T96), Tsyganenko 01 (T01); T89, T96, and T01 magnetic field models are driven with solar wind parameters and geomagnetic indices obtained from OMNI-2 data detector counts, omni and perpendicularelectron and proton flux are archived. Details of the processing can be found from .http://radbelts.gsfc.nasa.gov. Processing was done by: Shing F. Fung, Lun C. Tan, Xi Shao Space Physics Data Facility Goddard Space Flight Center, NASA Greenbelt, MD 20771 USA . e-mail: Shing.F.Fung@nasa.gov
Created Sept. 2005
TIROS/NOAA SEM MEPED Data Archive This is the re-processed version of the MEPED (Medium Energy Proton Electron Detector) data archive from the TIROS/NOAA spacecraft. The raw data from the NOAA archive have been processed to 1 minute resolution; magnetic field parameters (GSM Bx, By, Bz, B/Bmin, and L) are derived in 4 magnetic field models: IGRF, Tsyganenko 89 (T89), Tsyganenko 96 (T96), Tsyganenko 01 (T01); T89, T96, and T01 magnetic field models are driven with solar wind parameters and geomagnetic indices obtained from OMNI-2 data detector counts, omni and perpendicularelectron and proton flux are archived. Details of the processing can be found from .http://radbelts.gsfc.nasa.gov. Processing was done by: Shing F. Fung, Lun C. Tan, Xi Shao Space Physics Data Facility Goddard Space Flight Center, NASA Greenbelt, MD 20771 USA . e-mail: Shing.F.Fung@nasa.gov
Created Sept. 2005
TIROS/NOAA SEM MEPED Data Archive This is the re-processed version of the MEPED (Medium Energy Proton Electron Detector) data archive from the TIROS/NOAA spacecraft. The raw data from the NOAA archive have been processed to 1 minute resolution; magnetic field parameters (GSM Bx, By, Bz, B/Bmin, and L) are derived in 4 magnetic field models: IGRF, Tsyganenko 89 (T89), Tsyganenko 96 (T96), Tsyganenko 01 (T01); T89, T96, and T01 magnetic field models are driven with solar wind parameters and geomagnetic indices obtained from OMNI-2 data detector counts, omni and perpendicularelectron and proton flux are archived. Details of the processing can be found from .http://radbelts.gsfc.nasa.gov. Processing was done by: Shing F. Fung, Lun C. Tan, Xi Shao Space Physics Data Facility Goddard Space Flight Center, NASA Greenbelt, MD 20771 USA . e-mail: Shing.F.Fung@nasa.gov
Created Sept. 2005
TIROS/NOAA SEM MEPED Data Archive This is the re-processed version of the MEPED (Medium Energy Proton Electron Detector) data archive from the TIROS/NOAA spacecraft. The raw data from the NOAA archive have been processed to 1 minute resolution; magnetic field parameters (GSM Bx, By, Bz, B/Bmin, and L) are derived in 4 magnetic field models: IGRF, Tsyganenko 89 (T89), Tsyganenko 96 (T96), Tsyganenko 01 (T01); T89, T96, and T01 magnetic field models are driven with solar wind parameters and geomagnetic indices obtained from OMNI-2 data detector counts, omni and perpendicularelectron and proton flux are archived. Details of the processing can be found from .http://radbelts.gsfc.nasa.gov. Processing was done by: Shing F. Fung, Lun C. Tan, Xi Shao Space Physics Data Facility Goddard Space Flight Center, NASA Greenbelt, MD 20771 USA . e-mail: Shing.F.Fung@nasa.gov
Created Sept. 2005
TIROS/NOAA SEM MEPED Data Archive This is the re-processed version of the MEPED (Medium Energy Proton Electron Detector) data archive from the TIROS/NOAA spacecraft. The raw data from the NOAA archive have been processed to 1 minute resolution; magnetic field parameters (GSM Bx, By, Bz, B/Bmin, and L) are derived in 4 magnetic field models: IGRF, Tsyganenko 89 (T89), Tsyganenko 96 (T96), Tsyganenko 01 (T01); T89, T96, and T01 magnetic field models are driven with solar wind parameters and geomagnetic indices obtained from OMNI-2 data detector counts, omni and perpendicularelectron and proton flux are archived. Details of the processing can be found from .http://radbelts.gsfc.nasa.gov. Processing was done by: Shing F. Fung, Lun C. Tan, Xi Shao Space Physics Data Facility Goddard Space Flight Center, NASA Greenbelt, MD 20771 USA . e-mail: Shing.F.Fung@nasa.gov
Created Sept. 2005
TIROS/NOAA SEM MEPED Data Archive This is the re-processed version of the MEPED (Medium Energy Proton Electron Detector) data archive from the TIROS/NOAA spacecraft. The raw data from the NOAA archive have been processed to 1 minute resolution; magnetic field parameters (GSM Bx, By, Bz, B/Bmin, and L) are derived in 4 magnetic field models: IGRF, Tsyganenko 89 (T89), Tsyganenko 96 (T96), Tsyganenko 01 (T01); T89, T96, and T01 magnetic field models are driven with solar wind parameters and geomagnetic indices obtained from OMNI-2 data detector counts, omni and perpendicularelectron and proton flux are archived. Details of the processing can be found from .http://radbelts.gsfc.nasa.gov. Processing was done by: Shing F. Fung, Lun C. Tan, Xi Shao Space Physics Data Facility Goddard Space Flight Center, NASA Greenbelt, MD 20771 USA . e-mail: Shing.F.Fung@nasa.gov
Created Sept. 2005
Values of Element 0 ൦-80kev_prtn(0_dg)" and Element 5 ">30kev_elec(0_dg)" are unreliable and should not be used.
Values for elements 0- 5 (൦-80kev_prtn(81_dg)" -250kev_prtn(81_dg)" 藊-800kev_prtn(81_dg)" 蟰-2500kev_prtn(81_dg)" ">2500kev_prtn(81_dg)" and ">30kev_elec(83_dg)") are not now useable
Values of Element 0 "Jperp_(>30kev_elec)" are unreliable and should not be used.
Values of Element 0-4 are unreliable and should not be used.
Values of Element 0 "Jomni (>30kev_elec)" are unreliable and should not be used.
POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.)
POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.)
POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.)
POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.)