Collection Information
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IDENTIFIER |
urn:nasa:pds:mercury-simulation:data::1.0
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NAME |
Do we need to consider electrons' kinetic effects to properly model a planetary magnetosphere: the case of Mercury - simulation data collection
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TYPE |
Data
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DESCRIPTION |
This collection contains the results from the simulation study presented in Lapenta, G.; Schriver, D.; Walker, R. J.; Berchem, J.;
Echterling, N. F.; El Alaoui, M.; Travnicek, P., Do we need to consider electrons' kinetic effects to properly model a planetary
magnetosphere: the case of Mercury, JGR, 2022. (https://doi.org/*************)
The data includes fully kinetic global PIC simulations of Mercury's magnetosphere that include both ion and electron kinetic effects along with MESSENGER data. The energy conserving version of the
ipic3D simulation code (ECSIM) (Lapenta, 2017 doi:10.1016/j.jcp.2017.01.002) was used to study the evolution of Mercury's magnetosphere.
This work was funded by NASA grants HSR 80NSSC19K0841 and HSR 80NSSC19K0846 and NASA SSW 80NSSC19K0789 and 80NSSC21K0053. Resources supporting this work were
provided by the NASA High-End Computing (HEC) program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center and
NCCS at NASA Goddard Space Flight Center.
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SEARCH/ACCESS DATA |
Do we need to consider electrons' kinetic effects to properly model a planetary magnetosphere: the case of Mercury - simulation data bundle Online
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|
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Citation |
DIGITAL OBJECT IDENTIFIER (DOI) |
10.17189/krn5-0r32 (from parent bundle)
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AUTHOR LIST |
Lapenta, G.; Schriver, D.; Walker, R. J.; Berchem, J.; Echterling, N. F.; El Alaoui, M.; Travnicek, P.
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EDITOR LIST |
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PUBLICATION YEAR |
2022
|
DESCRIPTION |
This collection contains the results from the simulation study presented in Lapenta, G.; Schriver, D.; Walker, R. J.; Berchem, J.;
Echterling, N. F.; El Alaoui, M.; Travnicek, P., Do we need to consider electrons' kinetic effects to properly model a planetary
magnetosphere: the case of Mercury, JGR, 2022. (https://doi.org/*************)
The data includes fully kinetic global PIC simulations of Mercury's magnetosphere that include both ion and electron kinetic effects along with MESSENGER data. The energy conserving version of the
ipic3D simulation code (ECSIM) (Lapenta, 2017 doi:10.1016/j.jcp.2017.01.002) was used to study the evolution of Mercury's magnetosphere.
This work was funded by NASA grants HSR 80NSSC19K0841 and HSR 80NSSC19K0846 and NASA SSW 80NSSC19K0789 and 80NSSC21K0053. Resources supporting this work were
provided by the NASA High-End Computing (HEC) program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center and
NCCS at NASA Goddard Space Flight Center.
|
|
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Context |
START DATE TIME |
1965-01-01T12:00:00.000Z
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STOP DATE TIME |
N/A (ongoing)
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LOCAL MEAN SOLAR TIME |
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LOCAL TRUE SOLAR TIME |
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SOLAR LONGITUDE |
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PRIMARY RESULT PURPOSE |
SCIENCE
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PRIMARY RESULT PROCESSING LEVEL |
Derived
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PRIMARY RESULT DESCRIPTION |
This is simulation data
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PRIMARY RESULT WAVELENGTH RANGE |
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PRIMARY RESULT DOMAIN |
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PRIMARY RESULT DISCIPLINE NAME |
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INVESTIGATION |
MESSENGER
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OBSERVING SYSTEM |
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OBSERVING SYSTEM COMPONENT |
MESSENGER
Computer
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TARGET |
MERCURY
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REFERENCES |
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