Radio Observations and Modeling of Supernova Remnants
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
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Supernova remnants result when the ejecta of a supernova expands                into the ambient interstellar medium, compresses it, and mixes                  with it.  This expansion and mixing are extraordi.narily complex.               The Principal Investigator proposes to observe and map nearby                   supernova remnants and to model them computa.tionally.  The goal                is to increase our understanding of the physical processes taking               place in them, in particular to find out how and where                          synchrotron radio emission takes place in them and how this                     emission varies with time.
{'FirstName': 'John', 'LastName': 'Dickel', 'PI_MID_INIT': 'R', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'John R Dickel', 'EmailAddress': 'johnd@astro.uiuc.edu', 'PI_PHON': '2173335532', 'NSF_ID': '000088649', 'StartDate': '01/01/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'University of Illinois at Urbana-Champaign', 'CityName': 'URBANA', 'ZipCode': '618013620', 'PhoneNumber': '2173332187', 'StreetAddress': '506 S WRIGHT ST', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'Illinois', 'StateCode': 'IL', 'CONGRESSDISTRICT': '13', 'CONGRESS_DISTRICT_ORG': 'IL13', 'ORG_UEI_NUM': 'Y8CWNJRCNN91', 'ORG_LGL_BUS_NAME': 'UNIVERSITY OF ILLINOIS', 'ORG_PRNT_UEI_NUM': None}
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