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PIPER and Polarized Galactic ForegroundsIn addition to probing inflationary cosmology, PIPER will measure the polarized dust emission from the Galaxy. PIPER will be capable of full (I,0,U,V) measurement over four frequency bands ' These measurements will provide insight into the physics of dust grains and a probe of the Galactic magnetic field on large and intermediate scales.
Document ID
20090023864
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Chuss, David (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 24, 2013
Publication Date
July 1, 2009
Subject Category
Astronomy
Meeting Information
Meeting: The Path to CMBP0l: Upcoming Measurements of DMB Polarizaiton
Location: Chicago, IL
Country: United States
Start Date: July 1, 2009
End Date: July 3, 2009
Sponsors: Chicago Univ.
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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