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:2.6.0
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 |
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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