HPDE.io

flyby Giacobini-Zinner

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/ICE/ice-mag-p21

Description

The coordinate resolution for the magnetic field components is the
I,S coordinate system, defined by the JPL group before launch. I is
the unit vector in the direction of the ICE spin axis (positive in
the northward direction), and S is the unit vector from the space-
craft to the Sun. The Z-axis ia equal to I, the Y-axis to the nor-
malized cross-product I x S, and the x-axis to Y x Z. The I,S co-
ordinate system us approximately the same as the Solar Ecliptic (SE)
system since the spacecraft Z-axis is maintained within half a degree
of perpendicular to the Ecliptic plane. (SE is defined the same way
as GSE, but with the spacecraft [point of observation] substituted
for Earth).

View XML | View JSON | Edit

Details

Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/ICE/ice-mag-p21
ResourceHeader
ResourceName
flyby Giacobini-Zinner
ReleaseDate
2014-07-20 11:40:50Z
Description

The coordinate resolution for the magnetic field components is the
I,S coordinate system, defined by the JPL group before launch. I is
the unit vector in the direction of the ICE spin axis (positive in
the northward direction), and S is the unit vector from the space-
craft to the Sun. The Z-axis ia equal to I, the Y-axis to the nor-
malized cross-product I x S, and the x-axis to Y x Z. The I,S co-
ordinate system us approximately the same as the Solar Ecliptic (SE)
system since the spacecraft Z-axis is maintained within half a degree
of perpendicular to the Ecliptic plane. (SE is defined the same way
as GSE, but with the spacecraft [point of observation] substituted
for Earth).

Contacts
RolePersonStartDateStopDateNote
1.TechnicalContactspase://SMWG/Person/Elena.Budnik
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
Description

Web Service to this product using the HAPI interface.

Format
CSV
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA Web application
URL
Description

Access to Data via CDPP/AMDA Web application.

Format
CSV
Format
VOTable
Format
CDF
Format
PNG
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.
ProviderName
PDS
ProviderResourceName
ICE-C-MAG-3-RDR-GIACOBIN-ZIN-V1.0
InstrumentIDs
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
1985-09-10 00:00:00Z
StopDate
1985-09-14 20:51:15Z
Cadence
PT0.16S
ObservedRegion
Heliosphere.NearEarth
Parameter #1
Name
b_cse
ParameterKey
ice_b_cse
UCD
phys.magField
Units
nT
RenderingHints
DisplayType
TimeSeries
Structure
Size
3
Element
Name
bx
Index
1
ParameterKey
ice_b_cse(0)
Element
Name
by
Index
1
ParameterKey
ice_b_cse(1)
Element
Name
bz
Index
1
ParameterKey
ice_b_cse(2)
Field
Qualifier
Vector
FieldQuantity
Magnetic
Parameter #2
Name
|b|
ParameterKey
ice_b_tot
Description

Magnetic Field Magnitude

UCD
phys.magField
Units
nT
RenderingHints
DisplayType
TimeSeries
Field
Qualifier
Magnitude
FieldQuantity
Magnetic