NASA Logo, National Aeronautics and Space Administration
CDAWeb
+ FEEDBACK
CDAWeb banner

CDAWeb Served Heliophysics Datasets Beginning with 'N'

NEW_HORIZONS_HELIO1DAY_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_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_HELIO1DAY_POSITION
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
Back to top
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
Back to top
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
Back to top
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
Back to top
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
Back to top
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
Back to top
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
Back to top
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
Back to top
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
Back to top
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
Back to top
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
 
Dataset in CDAWeb
Back to top
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
Back to top
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
Back to top
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
Back to top
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
Back to top
NASA Logo - nasa.gov