Version:2.2.9
NumericalData
ResourceID
spase://NASA/NumericalData/AMPTE-UKS/FGM/PT5S
ResourceHeader
ResourceName
AMPTE-UKS Magnetic Field Data
ReleaseDate
2020-07-07 21:14:16Z
Description
AMPTE-UKS 5-second (spin) averaged magnetic field measurements
Acknowledgement
UKS-IRM Prime Parameters, UKS/IRM High Resolution Data, or products derived from them may NOT be published or shown in any form without the consent of the Principal Investigators concerned. Acknowledgements to the PI and the UK CDHF would
be appropriate in any published work; full-authorship may be required
in some cases.
Scientists intending to embark on studies involving AMPTE UKS/IRM data
products are advised to contact the relevant Principal Investigator(s)
early in order to ensure that the data is suitable for the study, that
the project does not infringe on other ongoing work, and that the
Principal Investigator in general consents to the intended use of the
data. PIs can provide this support only on a best efforts basis, so please
be as precise and succinct as possible, and please be patient when awaiting
a PI response.
Contacts
InformationURL
Name
AMPTE documents
URL
Description
An overview of the AMPTE missions with some descriptions of instruments
PriorIDs
spase://VMO/NumericalData/AMPTE_UKS/FGM/PT5S
spase://VMO/NumericalData/AMPTE-UKS/FGM/PT5S
spase://VSPO/NumericalData/AMPTE-UKS/FGM/PT5S
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
AMPTE/UKS Data
URL
Description
A web-accessible directory hosting AMPTE/UKS spin-averaged magnetic field data.
Format
Text
Encoding
ASCII
InstrumentIDs
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
1984-08-21 08:24:42.5Z
StopDate
1985-01-15 08:01:02.5Z
Cadence
PT5S
ObservedRegion
Earth.Magnetosheath
ObservedRegion
Earth.Magnetosphere
ObservedRegion
Earth.Magnetosphere.Magnetotail
ObservedRegion
Heliosphere.NearEarth
Caveats
The time tags represent the start times of accumulation intervals (spin). UKS times are UT stamped on board while IRM time stamps are UT at time of ground receipt. Thus for time-critical science, the IRM times need to be corrected by subtracting the light travel time from the spacecraft to the ground-station (at Weilheim in Germany apart special events requiring NASA DSN). For the transmission frequencies used, the vacuum light speed is appropriate. At apogee, this correction is more than a third of a second. There are no other known time delays.
Parameter #1
Name
Epoch
ParameterKey
Column 1
Description
The start of the accumulation time interval for the data point, in DA/MO/YR HR:MI:SS.MS format.
Support
Parameter #2
Name
Bm
ParameterKey
Column 2
Description
Units
nT
UnitsConversion
1e-9>T
FillValue
-1e31
Field
Qualifier
Magnitude
Qualifier
Scalar
FieldQuantity
Magnetic
Parameter #3
Name
B
Description
Units
nT
UnitsConversion
1e-9>T
CoordinateSystem
CoordinateRepresentation
Cartesian
CoordinateSystemName
GSE
Structure
Size
3
Element
Name
Bx
Qualifier
Component.I
Index
1
ParameterKey
Column 3
Element
Name
By
Qualifier
Component.J
Index
2
ParameterKey
Column 4
Element
Name
Bz
Qualifier
Component.K
Index
3
ParameterKey
Column 5
FillValue
-1e31
Field
Qualifier
Vector
FieldQuantity
Magnetic