This data set contains data from the LECP instrument on the Voyager 2 spacecraft. Each record in a file contains 1-day (24-hour) scan-averaged fluxes and flux uncertainties of electrons in two contiguous energy channels that cover the energy range 22-61 keV. The period 2006/001 through 2018/304 includes electrons measured upstream of the termination shock and in the heliosheath up to heliopause crossing. The voyager 2 LECP instrument steps through eight, 45 deg full-angle sectors, spending 192 sec in each sector, yielding a full scan through 360 deg every 25.6 min. The LECP scan plane is nearly parallel to RT-plane of the heliospheric RTN coordinate system. The electron data are averaged over the seven active sectors S1-S7; S8 is behind the sun-shield and not included in the average.
-- Electron channels designated EB01 and EB02
-- Data have been corrected to remove background due to penetrating cosmic ray ions
-- Electron fluxes and uncertainties (one st. dev.) in units: (cm^2 s sr MeV)^-1
-- Data are 5-point running averages of daily values
-- Values -9.900e+01 used for missing or nonphysical data
-- Negative year indicates filled data for the associated doy
Version:2.7.1
Version:2.7.1
This data set contains data from the LECP instrument on the Voyager 2 spacecraft. Each record in a file contains 1-day (24-hour) scan-averaged fluxes and flux uncertainties of electrons in two contiguous energy channels that cover the energy range 22-61 keV. The period 2006/001 through 2018/304 includes electrons measured upstream of the termination shock and in the heliosheath up to heliopause crossing. The voyager 2 LECP instrument steps through eight, 45 deg full-angle sectors, spending 192 sec in each sector, yielding a full scan through 360 deg every 25.6 min. The LECP scan plane is nearly parallel to RT-plane of the heliospheric RTN coordinate system. The electron data are averaged over the seven active sectors S1-S7; S8 is behind the sun-shield and not included in the average.
-- Electron channels designated EB01 and EB02
-- Data have been corrected to remove background due to penetrating cosmic ray ions
-- Electron fluxes and uncertainties (one st. dev.) in units: (cm^2 s sr MeV)^-1
-- Data are 5-point running averages of daily values
-- Values -9.900e+01 used for missing or nonphysical data
-- Negative year indicates filled data for the associated doy
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Stamatios.M.Krimigis | |||
| 2. | DeputyPI | spase://SMWG/Person/Matthew.Hill | |||
| 3. | CoInvestigator | spase://SMWG/Person/Robert.B.Decker | |||
| 4. | CoInvestigator | spase://SMWG/Person/Jerry.W.Manweiler | |||
| 5. | MetadataContact | spase://SMWG/Person/Robert.M.Candey | |||
| 6. | MetadataContact | spase://SMWG/Person/Andriy.Koval |
The HelioData dataset page provides an overview of the dataset with access links, associated variables, and more.
Access to Data in CDF Format via ftps from SPDF
Access to Data in CDF Format via https from SPDF
Access to ASCII, CDF, and Plots via NASA/GSFC CDAWeb
Web Service to this product using the HAPI interface.
Time, beginning of interval
4-digit year
Day of year (1-365 or 366)
Decimal year = year + (doy - 1)/dpy (dpy=365 or 366)
Flux, electrons 22-35 keV
Stat. unc. of EB01_fav
Flux, electrons 35-61 keV
Stat. unc. of EB02_fav