Studies of the Large Scale Structure of the Sun's Corona andMeter-Decameter Bursts
{'Code': '06020203', 'Directorate': {'Abbreviation': 'GEO', 'LongName': 'Directorate For Geosciences'}, 'Division': {'Abbreviation': 'AGS', 'LongName': 'Div Atmospheric & Geospace Sciences'}}
{'SignBlockName': 'Sherry O. Farwell', 'PO_EMAI': None, 'PO_PHON': None}
Using high spatial- and temporal-resolution images acquired                with the Clark Lake multifrequency radioheliograph, we will study               meter-decameter radio sources in the solar corona.  Radio                       synoptic charts and quiet Sun maps will be used to study and                    model large-scale structures such as streamers and coronal holes.               Impulsive burst observations will be used in conjunction with                   soft X-ray data to study several aspects of coronal mass                        ejections, including structure and plasma parameters, height-time               evolution, the relationship of CME's, flare and shocks, and                     acceleration of particles at slow shocks.  The overall aim is to                use already existing data to elucidate the nature of impulsive                  ejections from the sun which ultimately impact the earth.
{'FirstName': 'Mukul', 'LastName': 'Kundu', 'PI_MID_INIT': 'R', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Mukul R Kundu', 'EmailAddress': 'kundu@astro.umd.edu', 'NSF_ID': '000329815', 'StartDate': '01/15/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'University of Maryland, College Park', 'CityName': 'COLLEGE PARK', 'ZipCode': '207425100', 'PhoneNumber': '3014056269', 'StreetAddress': '3112 LEE BUILDING', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'Maryland', 'StateCode': 'MD', 'CONGRESSDISTRICT': '04', 'CONGRESS_DISTRICT_ORG': 'MD04', 'ORG_UEI_NUM': 'NPU8ULVAAS23', 'ORG_LGL_BUS_NAME': 'UNIVERSITY OF MARYLAND, COLLEGE PARK', 'ORG_PRNT_UEI_NUM': 'NPU8ULVAAS23'}
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{'Code': '1523', 'Text': 'SOLAR-TERRESTRIAL'}
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