This data set, held in CDAWeb as ISEE1_H0_FE, contains electron moments from the Vector Electron Spectrometer (VES), and spacecraft position vectors, at 9s or 18s resolution, depending on spacecraft telemetry rate. The data set also holds 1-min averages of the measured magnetic field vector. Electron moments include density, flow velocity, temperature and its anisotropy, and heat flux vector. Also given are the pressure tensor, its diagonalizing eigenvector, and the angle between its principal axis and the ambient magnetic field vector. These parameters are based on distributions accumulated in 3 sec but telemetered over 9s or 18s. Ancillary information given includes the spacecraft spin period, the spacecraft potential, the energy channels above this potential on which the moments for this record were based, and on/off flags for the Harvey and Mozer experiments.
Version:2.6.0
This data set, held in CDAWeb as ISEE1_H0_FE, contains electron moments from the Vector Electron Spectrometer (VES), and spacecraft position vectors, at 9s or 18s resolution, depending on spacecraft telemetry rate. The data set also holds 1-min averages of the measured magnetic field vector. Electron moments include density, flow velocity, temperature and its anisotropy, and heat flux vector. Also given are the pressure tensor, its diagonalizing eigenvector, and the angle between its principal axis and the ambient magnetic field vector. These parameters are based on distributions accumulated in 3 sec but telemetered over 9s or 18s. Ancillary information given includes the spacecraft spin period, the spacecraft potential, the energy channels above this potential on which the moments for this record were based, and on/off flags for the Harvey and Mozer experiments.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Keith.W.Ogilvie | |||
| 2. | GeneralContact | spase://SMWG/Person/Adolfo.Figueroa-Vinas | |||
| 3. | MetadataContact | spase://SMWG/Person/Lee.Frost.Bargatze |
For ftp retrieval of daily CDF files
In CDF via HTTP from SPDF
For CDAWeb subset, plot and list capabilities
Web Service to this product using the HAPI interface.
DD-MON-YY HH:MM:SS.SSS
This density is determined from a distribution obtained during 0.5s, for one 60 deg sector of one spacecraft spin.
This density is determined from a full-spin (3 sec) electron distribution.
The GSE X, Y, Z components of the bulk velocity vector
The GSE XX, XY, XZ, YX, YY, YZ, ZX, ZY, ZZ elements of the pressure tensor P. Pij = Pji.
The GSE X, Y, Z components of the heat flux vector
Electron temperature is 1/3rd of the trace of the diagonalized pressure tensor
Electron temperature anisotropy is T-parallel/T-perpendicular.
Normalized gyrotropy is the difference between perpendicular eigenvalues of the pressure tensor, divided by the electron temperature
Bx(GSE), 1 minute average
By(GSE), 1 minute average
Bz(GSE), 1 minute average
GSE X component of spacecraft position vector
GSE Y component of spacecraft position vector
GSE Z component of spacecraft position vector