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U.S. Department of Energy
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Two-dimensional mapping of dayside convection

Technical Report ·
OSTI ID:7242156
Millstone Hill radar azimuth scans were used to map the large-scale features of the ionospheric convection pattern in the vicinity of the cusp and cleft. Each scan covers 5 hours of MLT and 20 deg of invariant latitude with 30 minute temporal resolution Individual snapshots of the convection pattern for disturbed conditions on 31 January 1982 span the entire region of convection convergence near noon and compare favorably with average model representations of the dayside region. The characteristic features of ion and electron precipitation observed during satellite overflights of the radar field of view are used to identify the cusp and cleft and to relate the location of these magnetospheric features to the pattern of ionospheric convection electric field. Cusp precipitation is seen at 70 deg lat. and 09 MLT at the sunward/anti-sunward convection reversal immediately after a sudden turning of interplanetary magnetic field (IMF) B sub y from -5 nT to +5 nT while IMF B sub z was -10 nT.
Research Organization:
Massachusetts Inst. of Tech., Cambridge, MA (USA)
OSTI ID:
7242156
Report Number(s):
AD-A-214541/5/XAB
Country of Publication:
United States
Language:
English