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CDAWeb Served Heliophysics Datasets Beginning with 'N'

NEPTUNE_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
NEPTUNE_HELIO1HR_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
NEW-HORIZONS_PEPSSI_COSMIC-RAY-CORRECTED-COUNT-RATE-CRCPS: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) corrected cosmic ray count per second - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_COSMIC-RAY-CORRECTED-COUNT-RATE-CRCPS-SPECTRA: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) corrected cosmic ray count per second - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_COSMIC-RAY-CORRECTED-FLUX-CRFLUX-A: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) background corrected cosmic ray flux in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_COSMIC-RAY-CORRECTED-FLUX-CRFLUX-SPECTRA-A: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) background corrected cosmic ray flux in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_DOUBLES-COUNT-RATE-TOF-LCPS-A: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) 'Doubles' low energy events counts per second, time-of-flight (TOF) only, ~2-250 keV/nuc He+ in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_DOUBLES-COUNT-RATE-TOF-LCPS-B: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) 'Doubles' low energy events counts per second, time-of-flight (TOF) only, ~2-250 keV/nuc He+ in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_DOUBLES-COUNT-RATE-TOF-LCPS-SPECTRA-A: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) background corrected cosmic ray flux in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_DOUBLES-COUNT-RATE-TOF-LCPS-SPECTRA-B: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) background corrected cosmic ray flux in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_DOUBLES-DIFF-INTENSITY-TOF-LFLUX-A: PEPSSI>Pluto Energetic Particle Spectrometer Science Investigation suprathermal (lowest energy) particle time-of-flight (TOF) differential intensity in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_DOUBLES-DIFF-INTENSITY-TOF-LFLUX-B: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) background corrected cosmic ray flux in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_DOUBLES-DIFF-INTENSITY-TOF-LFLUX-SPECTRA-A: PEPSSI>Pluto Energetic Particle Spectrometer Science Investigation suprathermal (lowest energy) particle time-of-flight (TOF) differential intensity in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_DOUBLES-DIFF-INTENSITY-TOF-LFLUX-SPECTRA-B: PEPSSI>Pluto Energetic Particle Spectrometer Science Investigation suprathermal (lowest energy) particle time-of-flight (TOF) differential intensity in calibration regime 'A' or 'B' - Dr. Ralph L.McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_TRIPLES-COUNT-RATE-BCPS-A: New Horizons NH Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) Box-shaped slab triples count per second, time of flight (TOF) vs energy space, ~15 keV to 1 MeV, H, He, O (CNO group) in calibration regime 'A' or 'B' - Dr. Ralph L. McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_TRIPLES-COUNT-RATE-BCPS-B: New Horizons NH Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) Box-shaped slab triples count per second, time of flight (TOF) vs energy space, ~15 keV to 1 MeV, H, He, O (CNO group) in calibration regime 'A' or 'B' - Dr. Ralph L. McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_TRIPLES-COUNT-RATE-BCPS-SPECTRA-A: New Horizons NH Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) Box-shaped slab triples count per second, time of flight (TOF) vs energy space, ~15 keV to 1 MeV, H, He, O (CNO group) in calibration regime 'A' or 'B' - Dr. Ralph L. McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_TRIPLES-COUNT-RATE-BCPS-SPECTRA-B: New Horizons NH Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) Box-shaped slab triples count per second, time of flight (TOF) vs energy space, ~15 keV to 1 MeV, H, He, O (CNO group) in calibration regime 'A' or 'B' - Dr. Ralph L. McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_TRIPLES-DIFF-INTENSITY-BFLUX-A: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) Box-shaped slab triples count per second, time of flight (TOF) vs energy space, ~15 keV to 1 MeV, H, He, O (CNO group) in calibration regime 'A' or 'B' - Dr. Ralph L. McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_TRIPLES-DIFF-INTENSITY-BFLUX-B: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) Box-shaped slab triples count per second, time of flight (TOF) vs energy space, ~15 keV to 1 MeV, H, He, O (CNO group) in calibration regime 'A' or 'B' - Dr. Ralph L. McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_TRIPLES-DIFF-INTENSITY-BFLUX-SPECTRA-A: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) Box-shaped slab triples count per second, time of flight (TOF) vs energy space, ~15 keV to 1 MeV, H, He, O (CNO group) in calibration regime 'A' or 'B' - Dr. Ralph L. McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW-HORIZONS_PEPSSI_TRIPLES-DIFF-INTENSITY-BFLUX-SPECTRA-B: New Horizons Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) Box-shaped slab triples count per second, time of flight (TOF) vs energy space, ~15 keV to 1 MeV, H, He, O (CNO group) in calibration regime 'A' or 'B' - Dr. Ralph L. McNutt, Jr (Johns Hopkins University Applied Physics Laboratory)
NEW_HORIZONS_HELIO1HR_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
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_SOLAR-WIND: 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 MEPED, NOAA-05/TIROS-N/POES 5-14 Data Archive - Shing F. Fung (SPDF, GSFC/NASA)
NOAA06_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM MEPED, NOAA-05/TIROS-N/POES 5-14 Data Archive - Shing F. Fung (SPDF, GSFC/NASA)
NOAA07_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM MEPED, NOAA-05/TIROS-N/POES 5-14 Data Archive - Shing F. Fung (SPDF, GSFC/NASA)
NOAA08_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM MEPED, NOAA-05/TIROS-N/POES 5-14 Data Archive - Shing F. Fung (SPDF, GSFC/NASA)
NOAA10_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM MEPED, NOAA-05/TIROS-N/POES 5-14 Data Archive - Shing F. Fung (SPDF, GSFC/NASA)
NOAA12_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM MEPED, NOAA-05/TIROS-N/POES 5-14 Data Archive - Shing F. Fung (SPDF, GSFC/NASA)
NOAA14_MEPED1MIN_SEM: 1 minute re-processed particle count rates, fluxes, and model fields, SEM MEPED, NOAA-05/TIROS-N/POES 5-14 Data Archive - 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)
NEPTUNE_HELIO1DAY_POSITION (spase://NASA/NumericalData/Planet/Neptune/HelioWeb/Ephemeris/P1D)
Description
No TEXT global attribute value.
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEPTUNE_HELIO1HR_POSITION
Description
No TEXT global attribute value.
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW-HORIZONS_PEPSSI_COSMIC-RAY-CORRECTED-COUNT-RATE-CRCPS
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
R = Rates (Energy Only): 
1) High Energy, 
2) Initially labelled as 'Electrons' but dominated by Cosmic Rays during cruise
due to high geometry factor. 
R0 = Energy range 5-18 keV and > 735 keV 
R1 = Energy range 19-193 keV
R2 = Energy range 194-734 keV
J = general marker of Solar Wind Activity 
J00 = 'Electron' events 
J01 = 'Triples' 
where NNNN = year from 2012 to 2025
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to original datafiles: Cosmic Rays Count per
Second: 
PEPSSI_Reduced_CRCPS_NNNN.csv
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW-HORIZONS_PEPSSI_COSMIC-RAY-CORRECTED-COUNT-RATE-CRCPS-SPECTRA
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
R = Rates (Energy Only): 
1) High Energy, 
2) Initially labelled as 'Electrons' but dominated by Cosmic Rays during cruise
due to high geometry factor. 
R0 = Energy range 5-18 keV and > 735 keV 
R1 = Energy range 19-193 keV
R2 = Energy range 194-734 keV
J = general marker of Solar Wind Activity 
J00 = 'Electron' events 
J01 = 'Triples' 
where NNNN = year from 2012 to 2025
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to original datafiles: Cosmic Rays Count per
Second: 
PEPSSI_Reduced_CRCPS_NNNN.csv
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW-HORIZONS_PEPSSI_COSMIC-RAY-CORRECTED-FLUX-CRFLUX-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
R = Rates (Energy Only): 
1) High Energy, 
2) Initially labelled as 'Electrons' but dominated by Cosmic Rays during cruise
due to high geometry factor. 
R0 = Energy range 5-18 keV and > 735 keV 
R1 = Energy range 19-193 keV
R2 = Energy range 194-734 keV
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is Cosmic Rays Background Corrected Flux (differential
intensity):  related to original datafiles: 
PEPSSI_Reduced_CRFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW-HORIZONS_PEPSSI_COSMIC-RAY-CORRECTED-FLUX-CRFLUX-SPECTRA-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
R = Rates (Energy Only): 
1) High Energy, 
2) Initially labelled as 'Electrons' but dominated by Cosmic Rays during cruise
due to high geometry factor. 
R0 = Energy range 5-18 keV and > 735 keV 
R1 = Energy range 19-193 keV
R2 = Energy range 194-734 keV
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is Cosmic Rays Background Corrected Flux (differential
intensity):  related to original datafiles: 
PEPSSI_Reduced_CRFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW-HORIZONS_PEPSSI_DOUBLES-COUNT-RATE-TOF-LCPS-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
L = Low energy rates 'doubles' time-of-flight (TOF) covers the lowest energy
range particles events also overlaps with the 'triple' coincidence data
S = Detector Sector number
P = Calibrated assuming the particle is a proton
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to 'Doubles', suprathermal (low energy)
particle events counts per second, time-of-flight (TOF) only, ~2-250 keV/nuc He+
The original datafiles: 
PEPSSI_Reduced_LCPS_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_DOUBLES-COUNT-RATE-TOF-LCPS-B
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
L = Low energy rates 'doubles' time-of-flight (TOF) covers the lowest energy
range particles events also overlaps with the 'triple' coincidence data
S = Detector Sector number
P = Calibrated assuming the particle is a proton
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to 'Doubles', suprathermal (low energy)
particle events counts per second, time-of-flight (TOF) only, ~2-250 keV/nuc He+
The original datafiles: 
PEPSSI_Reduced_LCPS_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_DOUBLES-COUNT-RATE-TOF-LCPS-SPECTRA-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
L = Low energy rates 'doubles' time-of-flight (TOF) covers the lowest energy
range particles events also overlaps with the 'triple' coincidence data
S = Detector Sector number
P = Calibrated assuming the particle is a proton
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to 'Doubles', suprathermal (low energy)
particle events counts per second, time-of-flight (TOF) only, ~2-250 keV/nuc He+
The original datafiles: 
PEPSSI_Reduced_LCPS_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_DOUBLES-COUNT-RATE-TOF-LCPS-SPECTRA-B
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
L = Low energy rates 'doubles' time-of-flight (TOF) covers the lowest energy
range particles events also overlaps with the 'triple' coincidence data
S = Detector Sector number
P = Calibrated assuming the particle is a proton
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to 'Doubles', suprathermal (low energy)
particle events counts per second, time-of-flight (TOF) only, ~2-250 keV/nuc He+
The original datafiles: 
PEPSSI_Reduced_LCPS_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_DOUBLES-DIFF-INTENSITY-TOF-LFLUX-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
L = Low energy rates 'doubles' time-of-flight (TOF) covers the lowest energy
range particles events also overlaps with the 'triple' coincidence data
S = Detector Sector number
P = Calibrated assuming the particle is a proton
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to 'Doubles', suprathermal (lowest energy)
particle differential intensity time-of-flight (TOF), ~2-250 keV/nuc He+ 
The original datafiles: 
PEPSSI_Reduced_LFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_DOUBLES-DIFF-INTENSITY-TOF-LFLUX-B
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
L = Low energy rates 'doubles' time-of-flight (TOF) covers the lowest energy
range particles events also overlaps with the 'triple' coincidence data
S = Detector Sector number
P = Calibrated assuming the particle is a proton
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to 'Doubles', suprathermal (lowest energy)
particle differential intensity time-of-flight (TOF), ~2-250 keV/nuc He+ 
The original datafiles: 
PEPSSI_Reduced_LFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW-HORIZONS_PEPSSI_DOUBLES-DIFF-INTENSITY-TOF-LFLUX-SPECTRA-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
L = Low energy rates 'doubles' time-of-flight (TOF) covers the lowest energy
range particles events also overlaps with the 'triple' coincidence data
S = Detector Sector number
P = Calibrated assuming the particle is a proton
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to 'Doubles', suprathermal (lowest energy)
particle differential intensity time-of-flight (TOF), ~2-250 keV/nuc He+ 
The original datafiles: 
PEPSSI_Reduced_LFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_DOUBLES-DIFF-INTENSITY-TOF-LFLUX-SPECTRA-B
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
L = Low energy rates 'doubles' time-of-flight (TOF) covers the lowest energy
range particles events also overlaps with the 'triple' coincidence data
S = Detector Sector number
P = Calibrated assuming the particle is a proton
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to 'Doubles', suprathermal (lowest energy)
particle differential intensity time-of-flight (TOF), ~2-250 keV/nuc He+ 
The original datafiles: 
PEPSSI_Reduced_LFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW-HORIZONS_PEPSSI_TRIPLES-COUNT-RATE-BCPS-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
B = box-like slab 2D shapes, roughly polygon
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
Data type: BCPS ('Box' count per second: box-like slab 2D shape, roughly
polygon, triples counts per second, time of flight (TOF) vs energy space, ~15
keV to 1 MeV, H, He, O (CNO group) 
The original datafiles:
PEPSSI_Reduced_BCPS_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_TRIPLES-COUNT-RATE-BCPS-B
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
B = box-like slab 2D shapes, roughly polygon
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
Data type: BCPS ('Box' count per second: box-like slab 2D shape, roughly
polygon, triples counts per second, time of flight (TOF) vs energy space, ~15
keV to 1 MeV, H, He, O (CNO group) 
The original datafiles:
PEPSSI_Reduced_BCPS_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_TRIPLES-COUNT-RATE-BCPS-SPECTRA-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
B = box-like slab 2D shapes, roughly polygon
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
Data type: BCPS ('Box' count per second: box-like slab 2D shape, roughly
polygon, triples counts per second, time of flight (TOF) vs energy space, ~15
keV to 1 MeV, H, He, O (CNO group) 
The original datafiles:
PEPSSI_Reduced_BCPS_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_TRIPLES-COUNT-RATE-BCPS-SPECTRA-B
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
B = box-like slab 2D shapes, roughly polygon
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
Data type: BCPS ('Box' count per second: box-like slab 2D shape, roughly
polygon, triples counts per second, time of flight (TOF) vs energy space, ~15
keV to 1 MeV, H, He, O (CNO group) 
The original datafiles:
PEPSSI_Reduced_BCPS_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'a' or 'b' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_TRIPLES-DIFF-INTENSITY-BFLUX-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
B = box-like slab 2D shapes, roughly polygon
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
The original datafiles:
PEPSSI_Reduced_BFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_TRIPLES-DIFF-INTENSITY-BFLUX-B
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
B = box-like slab 2D shapes, roughly polygon
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
The original datafiles:
PEPSSI_Reduced_BFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_TRIPLES-DIFF-INTENSITY-BFLUX-SPECTRA-A
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
B = box-like slab 2D shapes, roughly polygon
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to PEPSSI B (box-like slab 2D shape, roughly
polygon) Triples Flux [or differential intensity, which is physically calibrated
data with units of 1/(cm^2 sr s keV)] ~15 keV to 1 MeV, 
The original datafiles:
PEPSSI_Reduced_BFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
Back to top
NEW-HORIZONS_PEPSSI_TRIPLES-DIFF-INTENSITY-BFLUX-SPECTRA-B
Description
The New Horizons mission's Pluto Energetic Particle Spectrometer Science
Investigation (PEPSSI) is made up of a time-of-flight (TOF)/mass spectrometer
and the associated science investigation. The PEPSSI instrument is designed to
measure pick-up ions, electrons, and other energetic ions energized by processes
such as charge exchange of Pluto's escaping atmospheric neutrals with solar ions
and photonsand by the expected bow shock resulting from the interaction between
the solar wind plasma and the atmosphere. In addition to measurements in the
Pluto/Charon system (closest approach planned for 14 July 2015), PEPSSI makes
observations of energetic particles in the solar wind during the cruise to
Pluto, and in 2007 made the most extensive energetic particle measurements in
Jupiter's magnetotail as the spacecraft traveled over 1 AU down the tail. 
B = box-like slab 2D shapes, roughly polygon
S = Detector Sector
Main publication: McNutt et al. 2008: The Pluto Energetic Particle Spectrometer
Science Investigation (PEPSSI) on the New Horizons Mission
Published: 25 October 2008
Volume 140, pages 315-385, (2008)
https://doi.org/10.1007/s11214-008-9436-y
https://doi.org/10.1007/s11214-008-9436-y
This particular dataset is related to PEPSSI B (box-like slab 2D shape, roughly
polygon) Triples Flux [or differential intensity, which is physically calibrated
data with units of 1/(cm^2 sr s keV)] ~15 keV to 1 MeV, 
The original datafiles:
PEPSSI_Reduced_BFLUX_NNNN_M.csv
where NNNN = year from 2012 to 2025, and 
M = 'A' or 'B' is a calibration regime
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW_HORIZONS_HELIO1HR_POSITION doi:10.48322/hfg9-qk78
Proper citations should include the "Accessed on date" in the form .
Description
No TEXT global attribute value.
Dataset in CDAWeb
Data Access Code Examples written in Python and IDL®.
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NEW_HORIZONS_SWAP_PICKUP-IONS doi:10.48322/d4g8-sm25
Description
Data from New Horizons Solar Wind Around Pluto instrument.
Elliott, H. A., D. J. McComas, Zirnstein, E. J., Randol, B. M., Delamere, P. A.,
Livadiotis, G., et al. (2019). Slowing of the Solar Wind in the Outer
Heliosphere. Astrophysical Journal, 885(2). DOI
10.3847/1538-4357/ab3e49.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
Data Access Code Examples written in Python and IDL®.
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NEW_HORIZONS_SWAP_PICKUP-IONS-HISTOGRAM doi:10.48322/z274-yv24
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
Data Access Code Examples written in Python and IDL®.
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NEW_HORIZONS_SWAP_SOLAR-WIND
Description
Data from New Horizons Solar Wind Around Pluto instrument.
Elliott, H. A., D. J. McComas, Zirnstein, E. J., Randol, B. M., Delamere, P. A.,
Livadiotis, G., et al. (2019). Slowing of the Solar Wind in the Outer
Heliosphere. Astrophysical Journal, 885(2). DOI
10.3847/1538-4357/ab3e49.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
Data Access Code Examples written in Python and IDL®.
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NOAA05_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/5/SPM/MEPED/KeyParameter/PT1M)
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
Data Access Code Examples written in Python and IDL®.
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NOAA06_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/6/SEM/MEPED/KeyParameter/PT1M)
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
Data Access Code Examples written in Python and IDL®.
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NOAA07_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/7/SEM/MEPED/KeyParameter/PT1M)
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
Data Access Code Examples written in Python and IDL®.
Back to top
NOAA08_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/8/SEM/MEPED/KeyParameter/PT1M)
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
Data Access Code Examples written in Python and IDL®.
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NOAA10_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/10/SEM/MEPED/KeyParameter/PT1M)
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
Data Access Code Examples written in Python and IDL®.
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NOAA12_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/12/SEM/MEPED/KeyParameter/PT1M)
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
Data Access Code Examples written in Python and IDL®.
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NOAA14_MEPED1MIN_SEM (spase://NOAA/NumericalData/POES/14/SEM/MEPED/KeyParameter/PT1M)
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
Data Access Code Examples written in Python and IDL®.
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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
Data Access Code Examples written in Python and IDL®.
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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
Data Access Code Examples written in Python and IDL®.
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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
Data Access Code Examples written in Python and IDL®.
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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
Data Access Code Examples written in Python and IDL®.
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