This data set contains high resolution samples at about one-second
intervals of the interplanetary magnetic field measured by the Ulysses
Magnetic Field experiment. Field vector components are given in units of
nanoteslas and in RTN coordinates, where R is the sun-s/c axis, T is the
cross product of the solar rotation axis and R, and T is the cross product
of R and T. The field magnitudes in nT are averages of scalar magnitudes
at higher time resolution. Times are computed at the mid-point of each
averaging interval and expressed in Spacecraft Event Time - UT (SCET-UT).
Data gaps have not been flagged in any way - if there were no available
data in a particular hour then there is no data record for that hour. No
data from the Feb. 1992 encounter with Jupiter are included. Each file
includes one day of data. Parameter key information given below is specific
to the data version at nssdcftp and at the ESA Research and Scientific Support
Department site identified below. Further details on the magnetic field
measurements can be found in the following reference: Balogh, A., et al.,
Astron. Astrophys. Suppl. Ser., 92(2), 221, 1992.
Version:2.4.1
This data set contains high resolution samples at about one-second
intervals of the interplanetary magnetic field measured by the Ulysses
Magnetic Field experiment. Field vector components are given in units of
nanoteslas and in RTN coordinates, where R is the sun-s/c axis, T is the
cross product of the solar rotation axis and R, and T is the cross product
of R and T. The field magnitudes in nT are averages of scalar magnitudes
at higher time resolution. Times are computed at the mid-point of each
averaging interval and expressed in Spacecraft Event Time - UT (SCET-UT).
Data gaps have not been flagged in any way - if there were no available
data in a particular hour then there is no data record for that hour. No
data from the Feb. 1992 encounter with Jupiter are included. Each file
includes one day of data. Parameter key information given below is specific
to the data version at nssdcftp and at the ESA Research and Scientific Support
Department site identified below. Further details on the magnetic field
measurements can be found in the following reference: Balogh, A., et al.,
Astron. Astrophys. Suppl. Ser., 92(2), 221, 1992.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Andre.Balogh | |||
| 2. | TechnicalContact | spase://SMWG/Person/Joyce.E.Wolf |
Site hosting instrument information, data and plots for Ulysses magnetometer
Web Service to this product using the HAPI interface.
Access to Data via CDPP/AMDA Web application.
Scalar magnitude of the magnetic field in nT
Magnetic field phi angle
Magnetic field theta angle