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}
},
{
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}
},
{
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}
},
{
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},
{
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},
{
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}
},
{
"orgName": "Scientific Visualization Studio",
"orgShortName": "Scientific Visualization Studio Group",
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}
},
{
"orgName": "Earth Sciences Division",
"orgShortName": "Earth Sciences Division",
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}
},
{
"orgCode": "610AT",
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}
},
{
"orgCode": "610HBG",
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}
},
{
"orgName": "Global Modeling and Assimilation Office ",
"orgShortName": "Global Modeling and Assimilation Office",
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}
},
{
"orgName": "Goddard Institute for Space Studies (GISS)",
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}
},
{
"orgName": "Mesoscale Atmospheric Processes Laboratory",
"orgShortName": "Mesoscale Atmospheric Processes",
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}
},
{
"orgName": "Climate and Radiation Laboratory",
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"router": {
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"secondary": "climate"
}
},
{
"orgName": "Atmospheric Chemistry and Dynamics Laboratory",
"orgShortName": "Atmospheric Chemistry and Dynamics",
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"router": {
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}
},
{
"orgName": "Cryospheric Sciences Laboratory",
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"secondary": "cryosphere"
}
},
{
"orgName": "Ocean Ecology Laboratory",
"orgShortName": "Ocean Ecology",
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"parentOrgCode": "610",
"router": {
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"secondary": "oceanecology"
}
},
{
"orgName": "Hydrological Sciences Laboratory",
"orgShortName": "Hydrological Sciences",
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"secondary": "hydrology"
}
},
{
"orgName": "Biospheric Sciences Laboratory",
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"secondary": "biosphere"
}
},
{
"orgName": "Terrestrial Information Systems Laboratory",
"orgShortName": "Terrestrial Information Systems",
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"router": {
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"secondary": "terrestrialinfo"
}
},
{
"orgName": "Geodesy and Geophysics Laboratory",
"orgShortName": "Geodesy and Geophysics Laboratory",
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}
},
{
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}
},
{
"orgName": "High Energy Astrophysics Science Archive Research Center (HEASARC) Office",
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}
},
{
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}
},
{
"orgName": "Instrument Development Group",
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}
},
{
"orgName": "Astroparticle Physics Laboratory",
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"parentOrgCode": "660",
"router": {
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"secondary": "astroparticles"
}
},
{
"orgName": "X-ray Astrophysics Laboratory",
"orgShortName": "X-ray Astrophysics Laboratory",
"orgCode": "662",
"parentOrgCode": "660",
"router": {
"primary": "astrophysics",
"secondary": "xray"
}
},
{
"orgName": "Gravitational Astrophysics Laboratory",
"orgShortName": "Gravitational Astrophysics Laboratory",
"orgCode": "663",
"parentOrgCode": "660",
"router": {
"primary": "astrophysics",
"secondary": "gravity"
}
},
{
"orgName": "Observational Cosmology Laboratory",
"orgShortName": "Observational Cosmology Laboratory",
"orgCode": "665",
"parentOrgCode": "660",
"router": {
"primary": "astrophysics",
"secondary": "cosmology"
}
},
{
"orgName": "Exoplanets and Stellar Astrophysics Laboratory",
"orgShortName": "Exoplanets and Stellar Astrophysics Laboratory",
"orgCode": "667",
"parentOrgCode": "660",
"router": {
"primary": "astrophysics",
"secondary": "exoplanets"
}
},
{
"orgName": "Heliophysics Science Division",
"orgShortName": "Heliophysics Science Division",
"orgCode": "670",
"parentOrgCode": "600",
"router": {
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"secondary": null
}
},
{
"orgName": "Solar Physics Laboratory",
"orgShortName": "Solar Physics Laboratory",
"orgCode": "671",
"parentOrgCode": "670",
"router": {
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"secondary": "solar"
}
},
{
"orgName": "Heliospheric Physics Laboratory ",
"orgShortName": "Heliospheric Physics Laboratory",
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"parentOrgCode": "670",
"router": {
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"secondary": "heliospheric"
}
},
{
"orgName": "Geospace Physics Laboratory",
"orgShortName": "Geospace Physics Laboratory",
"orgCode": "673",
"parentOrgCode": "670",
"router": {
"primary": "heliophysics",
"secondary": "geospace"
}
},
{
"orgName": "Space Weather Laboratory",
"orgShortName": "Space Weather Laboratory",
"orgCode": "674",
"parentOrgCode": "670",
"router": {
"primary": "heliophysics",
"secondary": "spaceweather"
}
},
{
"orgName": "Ionospheric, Thermospheric, Mesospheric (ITM) Physics Laboratory",
"orgShortName": "ITM Physics Laboratory",
"orgCode": "675",
"parentOrgCode": "670",
"router": {
"primary": "heliophysics",
"secondary": "itmphysics"
}
},
{
"orgName": "Solar System Exploration Division",
"orgShortName": "Solar System Exploration Division",
"orgCode": "690",
"parentOrgCode": "600",
"router": {
"primary": "solarsystem",
"secondary": null
}
},
{
"orgName": "Solar System Exploration Data Services Office",
"orgShortName": "Solar System Exploration Data Services Office",
"orgCode": "690.1",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "dataarchives"
}
},
{
"orgName": "Astrochemistry Laboratory",
"orgShortName": "Astrochemistry Laboratory",
"orgCode": "691",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "astrochemistry"
}
},
{
"orgName": "Planetary Systems Lab",
"orgShortName": "Planetary Systems Laboratory",
"orgCode": "693",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "planetarysystems"
}
},
{
"orgName": "Planetary Magnetospheres Lab",
"orgShortName": "Planetary Magnetospheres Laboratory",
"orgCode": "695",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "magnetospheres"
}
},
{
"orgName": "Planetary Geology, Geophysics & Geochemistry Lab",
"orgShortName": "Planetary Geology, Geophysics & Geochemistry Lab",
"orgCode": "698",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "p3g"
}
},
{
"orgName": "Planetary Environments Laboratory ",
"orgShortName": "Planetary Environments Laboratory",
"orgCode": "699",
"parentOrgCode": "690",
"router": {
"primary": "solarsystem",
"secondary": "atmosenvironments"
}
}
]
Wind Solar Wind Experiment (SWE)
The Solar Wind Experiment (SWE) will measure ions and electrons in the solar wind and the foreshock regions (particles whose energies are in the kiloelectronvolt range).
The Solar Wind Experiment (SWE) will measure ions and electrons in the solar wind and the foreshock regions (particles whose energies are in the kiloelectronvolt range). From these measurements, the solar wind velocity, density, temperature and heat flux can be deduced. Electron and ion velocity distributions should reveal properties of the following plasmas and their pivotal role in the transfer of mass, momentum, and energy from the Sun to the Earth. Measurements made in the foreshock region will contribute to understanding the structure of the bow shock.
Related Publications
2025. "First Detection of Low-frequency Striae in Interplanetary Type III Radio Bursts.", The Astrophysical Journal Letters, 985 (2): L27 [10.3847/2041-8213/add688] [Journal Article/Letter]
2019. "Unraveling the Internal Magnetic Field Structure of the Earth-directed Interplanetary Coronal Mass Ejections During 1995 – 2015.", Solar Physics, 294 (7): 89 [10.1007/s11207-019-1477-8] [Journal Article/Letter]