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CDAWeb Served Heliophysics Datasets Beginning with 'N'
- NEW_HORIZONS_SWAP_PICKUP-IONS: Data from New Horizons SWAP instrument - David J. McComas (Princeton)
- NEW_HORIZONS_SWAP_PICKUP-IONS-HISTOGRAM: Data from New Horizons SWAP instrument - David J. McComas (Princeton)
- NEW_HORIZONS_SWAP_VALIDSUM: Validated Summary (VS) data from New Horizons SWAP instrument - David J. McComas (Princeton)
- NOAA05_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM-1 MEPED, NOAA-05/TIROS-N - Shing F. Fung (SPDF, GSFC/NASA)
- NOAA06_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM-1 MEPED, NOAA-06 - Shing F. Fung (SPDF, GSFC/NASA)
- NOAA07_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM-1 MEPED, NOAA-07 - Shing F. Fung (SPDF, GSFC/NASA)
- NOAA08_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM-1 MEPED, NOAA-08 - Shing F. Fung (SPDF, GSFC/NASA)
- NOAA10_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM-1 MEPED, NOAA-10 - Shing F. Fung (SPDF, GSFC/NASA)
- NOAA12_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM-1 MEPED, NOAA-12 - Shing F. Fung (SPDF, GSFC/NASA)
- NOAA14_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM-1 MEPED, NOAA-14 - Shing F. Fung (SPDF, GSFC/NASA)
- NOAA15_POES-SEM2_FLUXES-2SEC: NOAA15 POES-SEM2 2-second Particle Precipitation Data [Important: these data have known contamination problems: please consult Rob Redmon (sem.poes@noaa.gov) for usage recommendations.] - NGDC and SWPC (NOAA)
- NOAA16_POES-SEM2_FLUXES-2SEC: NOAA16 POES-SEM2 2-second Particle Precipitation Data [Important: these data have known contamination problems: please consult Rob Redmon (sem.poes@noaa.gov) for usage recommendations.] - NGDC and SWPC (NOAA)
- NOAA18_POES-SEM2_FLUXES-2SEC: NOAA18 POES-SEM2 2-second Particle Precipitation Data [Important: these data have known contamination problems: please consult Rob Redmon (sem.poes@noaa.gov) for usage recommendations.] - NGDC and SWPC (NOAA)
- NOAA19_POES-SEM2_FLUXES-2SEC: NOAA19 POES-SEM2 2-second Particle Precipitation Data [Important: these data have known contamination problems: please consult Rob Redmon (sem.poes@noaa.gov) for usage recommendations.] - NGDC and SWPC (NOAA)
- NEW_HORIZONS_SWAP_PICKUP-IONS (spase://VSPO/NumericalData/NewHorizons/SWAP/PickupIon/ValidatedSummary/P1D)
- Description
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.
Dataset in CDAWeb
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- NEW_HORIZONS_SWAP_PICKUP-IONS-HISTOGRAM (spase://VSPO/NumericalData/NewHorizons/SWAP/PickupIonHistogram/ValidatedSummary/P1D)
- Description
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.
- Caveats
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).
Dataset in CDAWeb
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- NEW_HORIZONS_SWAP_VALIDSUM (spase://VSPO/NumericalData/NewHorizons/SWAP/ProtonMoments/ValidatedSummary/PT64S)
- Description
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.
Dataset in CDAWeb
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- NOAA05_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/5/SEM/MEPED/PT60S)
- Description
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
- Modification History
Created Sept. 2005
Dataset in CDAWeb
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- NOAA06_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/6/SEM/MEPED/PT60S)
- Description
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
- Modification History
Created Sept. 2005
Dataset in CDAWeb
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- NOAA07_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/7/SEM/MEPED/PT60S)
- Description
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
- Modification History
Created Sept. 2005
Dataset in CDAWeb
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- NOAA08_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/8/SEM/MEPED/PT60S)
- Description
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
- Modification History
Created Sept. 2005
Dataset in CDAWeb
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- NOAA10_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/10/SEM/MEPED/PT60S)
- Description
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
- Modification History
Created Sept. 2005
Dataset in CDAWeb
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- NOAA12_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/12/SEM/MEPED/PT60S)
- Description
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
- Modification History
Created Sept. 2005
Dataset in CDAWeb
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- NOAA14_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/14/SEM/MEPED/PT60S)
- Description
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
- Modification History
Created Sept. 2005
- Variable Notes
- MEPED Count Rates for 0 Deg. telescopes, 4 proton and 2 electron energy bands (counts_0dg)
Values of Element 0 ൦-80kev_prtn(0_dg)" and Element 5 ">30kev_elec(0_dg)" are unreliable and should not be used.
- MEPED Count Rates for 81/83 Deg. telescopes, 2 electron energy bands (counts_90dg)
Values for elements 0- 5 (൦-80kev_prtn(81_dg)" -250kev_prtn(81_dg) 250-800kev_prtn(81_dg)" 蟰-2500kev_prtn(81_dg)" ">2500kev_prtn(81_dg)" and >30kev_elec(83_dg)") are not now useable
- MEPED calculated omnidirectional electron flux, 2 energy bands from 0/83 telescopes
Values of Element 0 "Jomni (>30kev_elec)" are unreliable and should not be used.
- MEPED calculated omnidirectional proton flux, 3 energy bands from omni telescopes
Values of Element 0-4 are unreliable and should not be used.
- MEPED calculated perpendicular electron flux, 2 energy bands (Jperp_e)
Values of Element 0 "Jperp_(>30kev_elec)" are unreliable and should not be used.
- [NOT NOW USEABLE] MEPED calculated perpendicular proton flux, 5 energy bands (Jperp_p)
Values are unreliable and should not be used.
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- NOAA15_POES-SEM2_FLUXES-2SEC (spase://NOAA/NumericalData/POES/15/SEM-2/CDF/PT2S)
- Description
POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.)
Dataset in CDAWeb
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- NOAA16_POES-SEM2_FLUXES-2SEC (spase://NOAA/NumericalData/POES/16/SEM-2/CDF/PT2S)
- Description
POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.)
Dataset in CDAWeb
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- NOAA18_POES-SEM2_FLUXES-2SEC (spase://NOAA/NumericalData/POES/18/SEM-2/CDF/PT2S)
- Description
POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.)
Dataset in CDAWeb
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- NOAA19_POES-SEM2_FLUXES-2SEC (spase://NOAA/NumericalData/POES/19/SEM-2/CDF/PT2S)
- Description
POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.)
Dataset in CDAWeb
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- NASA Official: Robert M. Candey (301)286-6707, Robert.M.Candey@nasa.gov
- Curator: Tami Kovalick
- Last Modified: