Radio Emission from Solar System "Bodies"
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
{'SignBlockName': 'Vernon Pankonin', 'PO_EMAI': None, 'PO_PHON': None}
Radio wavelength observations of objects in the Solar System give               information on their physical and chemical structure and the                    structure of their magnetospheres and atmospheres.  The                         magnetospheric studies use observations of the synchrotron                      radiation from relativistic electrons trapped in a magnetosphere                to map out the particle distributions and magnetic field                        topologies.  Atmospheric studies use radio data to probe levels                 in the atmosphere deeper than those which are probed with                       observations at other wavelengths.                                                                                                                              Dr. De Pater will use this grant to continue her studies of                     objects in the Solar System at centimeter and millimeter                        wavelengths.  The objects to be investigated include the gaseous                giant planets Jupiter, Saturn, Uranus, and Neptune; the Earth-                  like planets Venus, Mars, and Mercury; the galilean satellites;                 and various new and periodic comets which come close to the Sun.
{'FirstName': 'Imke', 'LastName': 'de Pater', 'PI_MID_INIT': None, 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Imke de Pater', 'EmailAddress': 'imke@berkeley.edu', 'NSF_ID': '000423096', 'StartDate': '06/01/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
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{'Code': '1214', 'Text': 'PLANETARY ASTRONOMY'}
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