The instrument (E2) consisted of a triaxial fluxgate magnetometer mounted on a 2.75-m boom to make magnetic field measurements up to 4 Hz. Data from each axis were first sent through a low-pass filter with the 3-dB attenuation point at 4 Hz. Depending on the telemetry format and bit rate, the data were fed either into a time-averaging computer or directly connected to telemetry. A shock identification computer triggered the storage of rapid-rate data in the spacecraft memory when there were discontinuities in the variations of the ambient magnetic field. Two measurement ranges were used, plus or minus 100 and 400 nT with resolutions of plus or minus 0.2 and 0.8 nT, respectively. The instrument was equipped with a flipper mechanism, which reoriented each sensor by 90 deg periodically. For detailed information, see p. 232 of Raumfahrtforschung, v. 19, n. 5, 1975.
Version:2.2.9
The instrument (E2) consisted of a triaxial fluxgate magnetometer mounted on a 2.75-m boom to make magnetic field measurements up to 4 Hz. Data from each axis were first sent through a low-pass filter with the 3-dB attenuation point at 4 Hz. Depending on the telemetry format and bit rate, the data were fed either into a time-averaging computer or directly connected to telemetry. A shock identification computer triggered the storage of rapid-rate data in the spacecraft memory when there were discontinuities in the variations of the ambient magnetic field. Two measurement ranges were used, plus or minus 100 and 400 nT with resolutions of plus or minus 0.2 and 0.8 nT, respectively. The instrument was equipped with a flipper mechanism, which reoriented each sensor by 90 deg periodically. For detailed information, see p. 232 of Raumfahrtforschung, v. 19, n. 5, 1975.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Fritz.M.Neubauer | |||
| 2. | CoInvestigator | spase://SMWG/Person/A.Maier |
In ASCII via FTP from SPDF
In ASCII via FTP from SPDF
YEAR OF THE DATA INTERVAL (LAST TWO DIGITS ONLY)
DAY OF THE DATA INTERVAL FROM THE FIRST DAY OF THE ABOVE YEAR, JAN. 1= DAY 1
HOUR OF THE DAY OF THE DATA INTERVAL
THE COMPONENT OF THE INTERPLANETARY MAGNETIC FIELD DIRECTED TOWARD THE SUN AND PARALLEL TO THE X-AXIS OF THE SPACECRAFT-CENTERED SOLAR ECLIPTIC (SSE) COORDINATE SYSTEM (FIELD IN NANOTELSAS).
THE COMPONENT OF THE INTERPLANETARY MAGNETIC FIELD IN THE ECLIPTIC ALONG THE SSE Y-AXIS
THE COMPONENT OF THE INTERPLANETARY MAGNETIC FIELD DIRECTED PERPENDICULAR TO AND NORTHWARD FROM THE ECLIPTIC, PARALLEL TO THE SSE Z-AXIS
AVERAGE OF FINE SCALE FIELD MAGNITUDES FOR THE INTERPLANETARY MAGNETIC FIELD VECTOR (NANOTESLAS)
ELEVATION ANGLE OF THE MAGNETIC FIELD VECTOR IN THE SSE SYSTEM (I.E., SSE LATITUDE ANGLE).
AZIMUTH ANGLE OF THE MAGNETIC FIELD VECTOR IN THE SSE SYSTEM (I.E., SSE LONGITUDE ANGLE)