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},
{
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},
{
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{
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},
{
"orgName": "Goddard Institute for Space Studies (GISS)",
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},
{
"orgName": "Mesoscale Atmospheric Processes Laboratory",
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}
},
{
"orgName": "Climate and Radiation Laboratory",
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}
},
{
"orgName": "Atmospheric Chemistry and Dynamics Laboratory",
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}
},
{
"orgName": "Cryospheric Sciences Laboratory",
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"secondary": "cryosphere"
}
},
{
"orgName": "Ocean Ecology Laboratory",
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"secondary": "oceanecology"
}
},
{
"orgName": "Hydrological Sciences Laboratory",
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}
},
{
"orgName": "Biospheric Sciences Laboratory",
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},
{
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},
{
"orgName": "Geodesy and Geophysics Laboratory",
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},
{
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}
},
{
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},
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},
{
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}
},
{
"orgName": "Astroparticle Physics Laboratory",
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"secondary": "astroparticles"
}
},
{
"orgName": "X-ray Astrophysics Laboratory",
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}
},
{
"orgName": "Gravitational Astrophysics Laboratory",
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}
},
{
"orgName": "Observational Cosmology Laboratory",
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}
},
{
"orgName": "Exoplanets and Stellar Astrophysics Laboratory",
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}
},
{
"orgName": "Heliophysics Science Division",
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}
},
{
"orgName": "Solar Physics Laboratory",
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"secondary": "solar"
}
},
{
"orgName": "Heliospheric Physics Laboratory ",
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"secondary": "heliospheric"
}
},
{
"orgName": "Geospace Physics Laboratory",
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"router": {
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"secondary": "geospace"
}
},
{
"orgName": "Space Weather Laboratory",
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"secondary": "spaceweather"
}
},
{
"orgName": "Ionospheric, Thermospheric, Mesospheric (ITM) Physics Laboratory",
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"parentOrgCode": "670",
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}
},
{
"orgName": "Solar System Exploration Division",
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"router": {
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"secondary": null
}
},
{
"orgName": "Solar System Exploration Data Services Office",
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"secondary": "dataarchives"
}
},
{
"orgName": "Astrochemistry Laboratory",
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"router": {
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"secondary": "astrochemistry"
}
},
{
"orgName": "Planetary Systems Lab",
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"router": {
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}
},
{
"orgName": "Planetary Magnetospheres Lab",
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"secondary": "magnetospheres"
}
},
{
"orgName": "Planetary Geology, Geophysics & Geochemistry Lab",
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"router": {
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"secondary": "p3g"
}
},
{
"orgName": "Planetary Environments Laboratory ",
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"router": {
"primary": "solarsystem",
"secondary": "atmosenvironments"
}
}
]
Wilkinson Microwave Anisotropy Probe (WMAP)
The Wilkinson Microwave Anisotropy Probe (WMAP) created a map of temperature fluctuations in the cosmic background radiation -- the remnant afterglow of the hot young universe -- at much higher resolution, sensitivity, and accuracy than its predecessor, the Cosmic Background Explorer (COBE). WMAP observations shed light on several key questions in cosmology, including the structure and physical parameters of the universe. WMAP was launched into orbit in 2001. Observations formally concluded in October 2010, although analysis of the data continues.
The Wilkinson Microwave Anisotropy Probe (WMAP) created a map of temperature fluctuations in the cosmic background radiation -- the remnant afterglow of the hot young universe -- at much higher resolution, sensitivity, and accuracy than its predecessor, the Cosmic Background Explorer (COBE). WMAP observations shed light on several key questions in cosmology, including the structure and physical parameters of the universe. WMAP was launched into orbit in 2001. Observations formally concluded in October 2010, although analysis of the data continues.