HDPWS

MESSENGER - Analytical Models - KT17 model

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-model

Description
Magnetic field along Mercury orbit is being real-time calculated. S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user. KT17 magnetic field model (Korth et al., 2017) model is used in calculations.

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Details

Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-model
ResourceHeader
ResourceName
MESSENGER - Analytical Models - KT17 model
AlternateName
KT17 mercury magnetic field model
ReleaseDate
2016-04-04 18:53:40Z
Description
Magnetic field along Mercury orbit is being real-time calculated. S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user. KT17 magnetic field model (Korth et al., 2017) model is used in calculations.
Acknowledgement
James, M. K. - KT17 (v1.0.0) - https://github.com/mattkjames7/KT17/releases/tag/v1.0.0
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/Haje.Korth
2. TechnicalContact spase://CNES/Person/CDPP-AMDA/M.K.James

InformationURL
Name
Korth, H., Johnson, C. L., Philpott, L., Tsyganenko, N. A., Anderson, B. J. (2017). A dynamic model of Mercury's magnetospheric magnetic field. Geophysical Research Letters, 44, 10,147– 10,154.
URL
Description
Model description
InformationURL
Name
James, M. K. - KT17 (v1.0.0)
URL
Description
Software
InformationURL
Name
Anderson, B. J., Johnson, C. L., and Korth, H. (2013), A magnetic disturbance index for Mercury's magnetic field derived from MESSENGER Magnetometer data, Geochem. Geophys. Geosyst., 14, 3875– 3886
URL
Description
Disturbance index description
PriorIDs
mes-orb-orb
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
mes-kt17-model
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 https://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 https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
ProviderName
IRAP
InstrumentIDs
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
2011-03-04 00:00:00Z
StopDate
2015-04-29 23:59:00Z
Cadence
PT1M
ObservedRegion
Mercury
Parameter #1
Name
b msm
ParameterKey
b_kt17_model_60_0.427_50_mes_xyz_orbmso
Units
nT
Structure
Size
3
Element
Name
bx
Qualifier
Component.I
Index
1
ParameterKey
b_kt17_model_60_0.427_50_mes_xyz_orbmso(0)
Element
Name
by
Qualifier
Component.J
Index
2
ParameterKey
b_kt17_model_60_0.427_50_mes_xyz_orbmso(1)
Element
Name
bz
Qualifier
Component.K
Index
3
ParameterKey
b_kt17_model_60_0.427_50_mes_xyz_orbmso(2)
Field
FieldQuantity
Magnetic
Parameter #2
Name
|b|
ParameterKey
b_kt17_model_tot_60_0.427_50_mes_xyz_orbmso
Description
Scalar magnitude of the magnetic field in nT
UCD
phys.magField
Units
nT
UnitsConversion
1e-9>T
RenderingHints
DisplayType
TimeSeries
Field
Qualifier
Magnitude
FieldQuantity
Magnetic