South Pole Studies of the Cosmic Background Radiation
{'Code': '01020302', 'Directorate': {'Abbreviation': 'O/D', 'LongName': 'Office Of The Director'}, 'Division': {'Abbreviation': 'OPP', 'LongName': 'Office of Polar Programs'}}
{'SignBlockName': 'John T. Lynch', 'PO_EMAI': None, 'PO_PHON': None}
This project will map the southern sky in the Cosmic Microwave                  Background Radiation (CMBR) at a wavelength of 3mm and with                     angular resolution from 0.5 - 10 degrees.  The purpose is to look               for deviations from isotropy and therefore fluctuations in the                  distribution of mass in the early universe.  The instrument to be               used is a modified balloon payload that will take advantage of the              low atmospheric temperature and humidity at the South Pole, the                 quiet radio environment, and the circumpolar motion of features in              the sky.  The experiment addresses one of the outstanding                       questions of cosmology.
{'FirstName': 'Philip', 'LastName': 'Lubin', 'PI_MID_INIT': 'M', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Philip M Lubin', 'EmailAddress': 'lubin@deepspace.ucsb.edu', 'NSF_ID': '000461401', 'StartDate': '01/01/1988', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'University of California-Santa Barbara', 'CityName': 'SANTA BARBARA', 'ZipCode': '931060001', 'PhoneNumber': '8058934188', 'StreetAddress': '3227 CHEADLE HALL', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'California', 'StateCode': 'CA', 'CONGRESSDISTRICT': '24', 'CONGRESS_DISTRICT_ORG': 'CA24', 'ORG_UEI_NUM': 'G9QBQDH39DF4', 'ORG_LGL_BUS_NAME': 'UNIVERSITY OF CALIFORNIA, SANTA BARBARA', 'ORG_PRNT_UEI_NUM': None}
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[{'Code': '511500', 'Text': 'ANT Astrophys & Geospace Sci'}, {'Code': '912000', 'Text': 'CROSS-DIRECTORATE PROGRAMS'}]
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