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Voyager 2 1-hr Averaged Triaxial Fluxgate Magnetometer (MAG) Interplanetary Magnetic Field in ASCII Format
var authors='Ness, Norman F.; Burlaga, Leonard F.';
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(2025).
Voyager 2 1-hr Averaged Triaxial Fluxgate Magnetometer (MAG) Interplanetary Magnetic Field in ASCII Format.
[Data set].
Space Physics Data Facility; Planetary Data System.
https://doi.org/10.48322/7chv-fq03. Accessed on document.write(currentDateStr);.
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ResourceID
spase://NASA/NumericalData/Voyager2/MAG/ASCII/PT1H
Description
This data set contains hour averages of the interplanetary magnetic
field (IMF) measurements obtained by the triaxial fluxgate magnetometer
experiment on Voyager 1. Identical instruments on Voyager 1 and 2 were
designed to measure the IMF between Earth and Saturn (10 AU) during the
primary Voyager mission. The design and performance yielded absolute
accuracies to better than < 0.1 nT. In general, each component of the
hourly average has an uncertainty of up to (+/- 0.05 nT) in the region
beyond 10 AU. More accurate measurements can be obtained by special
processing of the data, but it was not feasible to do this for the
entire data set included here. The magnetic field magnitude in nT is
provided along with angles of the field vector in the spacecraft-
centered Heliographic (HG) coordinate system, also known as RTN.
Coordinate System
=================
Interplanetary magnetic field studies make use of two important
coordinate systems, the Inertial Heliographic (IHG) coordinate system
and the Heliographic (HG) coordinate system.
The IHG coordinate system is use to define the spacecraft's position.
The IHG system is defined with its origin at the Sun. There are three
orthogonal axes, X(IHG), Y(IHG), and Z(IHG). The Z(IHG) axis points
northward along the Sun's spin axis. The X(IHG) - Y(IHG) plane lays in
the solar equatorial plane. The intersection of the solar equatorial
plane with the ecliptic plane defines a line, the longitude of the
ascending node, which is taken to be the X(IHG) axis. The X(IHG) axis
drifts slowly with time, approximately one degree per 72 years.
Magnetic field orientation is defined in relation to the spacecraft.
Drawing a line from the Sun's center (IHG origin) to the spacecraft
defines the X axis of the HG coordinate system. The HG coordinate
system is defined with its origin centered at the spacecraft. Three
orthogonal axes are defined, X(HG), Y(HG), and Z(HG). The X(HG) axis
points radially away from the Sun and the Y(HG) axis is parallel to the
solar equatorial plane and therefore parallel to the X(IHG)-Y(IHG) plane
too. The Z(HG) axis is chosen to complete the orthonormal triad.
An excellent reference guide with diagrams explaining the IHG and HG
systems may be found in Space and Science Reviews, Volume 39 (1984),
pages 255-316, MHD Processes in the Outer Heliosphere, L. F. Burlaga
[BURLAGA1984].
Metadata Rights
CC0-1.0:
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions. The actual data/software may be subject to a different license.
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Details
Version:2.7.1
NumericalData
ResourceID
spase://NASA/NumericalData/Voyager2/MAG/ASCII/PT1H
NamingAuthority
NASA
ResourceType
NumericalData
ResourceHeader
ResourceName
Voyager 2 1-hr Averaged Triaxial Fluxgate Magnetometer (MAG) Interplanetary Magnetic Field in ASCII Format
DOI
https://doi.org/10.48322/7chv-fq03
ReleaseDate
2026-06-26 13:31:22Z
RevisionHistory
RevisionEvent
ReleaseDate
2020-07-07 21:15:58Z
Note
Only known prior ReleaseDate of the metadata
RevisionEvent
ReleaseDate
2025-11-14 16:01:55Z
Note
Added PublicationInfo. Added ResourceType and NamingAuthority. Changed http to https in top-level schemaLocation attribute. Fixed version number separator in top-level schemaLocation attribute. Matched version number in schemaLocation attribute to updated value in Version tag. ZCB
RevisionEvent
ReleaseDate
2025-12-04 13:32:37Z
Note
Added MetadataRightsList and RightsList(s). Updated to 2.7.1. ZCB
RevisionEvent
ReleaseDate
2026-02-17 18:48:03Z
Note
Added DOI. TLK
RevisionEvent
ReleaseDate
2026-06-26 13:31:22Z
Note
Add 'Z' to TemporalDescription:TimeSpan:StartDate, TemporalDescription:TimeSpan:StopDate. ZCB
Description
This data set contains hour averages of the interplanetary magnetic
field (IMF) measurements obtained by the triaxial fluxgate magnetometer
experiment on Voyager 1. Identical instruments on Voyager 1 and 2 were
designed to measure the IMF between Earth and Saturn (10 AU) during the
primary Voyager mission. The design and performance yielded absolute
accuracies to better than < 0.1 nT. In general, each component of the
hourly average has an uncertainty of up to (+/- 0.05 nT) in the region
beyond 10 AU. More accurate measurements can be obtained by special
processing of the data, but it was not feasible to do this for the
entire data set included here. The magnetic field magnitude in nT is
provided along with angles of the field vector in the spacecraft-
centered Heliographic (HG) coordinate system, also known as RTN.
Coordinate System
=================
Interplanetary magnetic field studies make use of two important
coordinate systems, the Inertial Heliographic (IHG) coordinate system
and the Heliographic (HG) coordinate system.
The IHG coordinate system is use to define the spacecraft's position.
The IHG system is defined with its origin at the Sun. There are three
orthogonal axes, X(IHG), Y(IHG), and Z(IHG). The Z(IHG) axis points
northward along the Sun's spin axis. The X(IHG) - Y(IHG) plane lays in
the solar equatorial plane. The intersection of the solar equatorial
plane with the ecliptic plane defines a line, the longitude of the
ascending node, which is taken to be the X(IHG) axis. The X(IHG) axis
drifts slowly with time, approximately one degree per 72 years.
Magnetic field orientation is defined in relation to the spacecraft.
Drawing a line from the Sun's center (IHG origin) to the spacecraft
defines the X axis of the HG coordinate system. The HG coordinate
system is defined with its origin centered at the spacecraft. Three
orthogonal axes are defined, X(HG), Y(HG), and Z(HG). The X(HG) axis
points radially away from the Sun and the Y(HG) axis is parallel to the
solar equatorial plane and therefore parallel to the X(IHG)-Y(IHG) plane
too. The Z(HG) axis is chosen to complete the orthonormal triad.
An excellent reference guide with diagrams explaining the IHG and HG
systems may be found in Space and Science Reviews, Volume 39 (1984),
pages 255-316, MHD Processes in the Outer Heliosphere, L. F. Burlaga
[BURLAGA1984].
PublicationInfo
Authors
Ness, Norman F.; Burlaga, Leonard F.
PublicationDate
2025-11-14 16:01:55Z
PublishedBy
Space Physics Data Facility; Planetary Data System
Contacts
Role
Person
StartDate
StopDate
Note
1.
PrincipalInvestigator
spase://SMWG/Person/Norman.F.Ness
2.
CoInvestigator
spase://SMWG/Person/Leonard.F.Burlaga
3.
MetadataContact
spase://SMWG/Person/Todd.A.King
PriorIDs
spase://VSPO/NumericalData/P_VOYAGER2_HDR_MAG_1HR_ASC
spase://VSPO/NumericalData/Voyager2/MAG/PT1H
spase://VSPO/NumericalData/Voyager2/MAG/ASCII/PT1H
AccessInformation
RepositoryID
spase://SMWG/Repository/NASA/GSFC/SPDF
Availability
Online
AccessRights
Open
RightsList
Rights
SchemeURI
https://spdx.org/licenses/
RightsIdentifierScheme
SPDX
RightsIdentifier
CC0-1.0
RightsURI
https://spdx.org/licenses/CC0-1.0.html
RightsName
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products
AccessURL
Name
FTPS from SPDF (not with most browsers)
URL
ftps://spdf.gsfc.nasa.gov/pub/data/voyager/voyager2/magnetic_fields/ip_1hour_ascii/
Description
The data set format and description are in vy2mag_1h_fmt.txt
AccessURL
Name
HTTPS from SPDF
URL
https://spdf.gsfc.nasa.gov/pub/data/voyager/voyager2/magnetic_fields/ip_1hour_ascii/
Description
The data set format and description are in vy2mag_1h_fmt.txt
Format
Text
AccessInformation
RepositoryID
spase://SMWG/Repository/PDS/PPI
Availability
Online
AccessRights
Open
AccessURL
Name
PDS/PPI
URL
https://pds-ppi.igpp.ucla.edu/search/view/?f=yes&id=pds://PPI/VG2-SW-MAG-4-SUMM-HGCOORDS-1HR-V1.0
ProductKey
VG2-SW-MAG-4-SUMM-HGCOORDS-1HR-V1.0
Description
This collection is archived with NASA's Planetary Data System.
Language
En
Format
Text.ASCII
Acknowledgement
NASA's Planetary Plasma Interactions (PPI) Node of the Planetary Data System (PDS) and the P.I. for the data.
ProviderProcessingLevel
CALIBRATED
InstrumentIDs
spase://SMWG/Instrument/Voyager2/MAG
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
1977-08-20 00:00:00Z
StopDate
1989-08-25 00:00:00Z
Cadence
PT1H
ObservedRegion
Heliosphere.Outer