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Thermal-ion upwelling in the high-latitude ionosphere

Thesis/Dissertation ·
OSTI ID:7206160
High latitude observations of thermal ion outflows, traditionally known as the polar wind,' and heavy ion upwellings, consisting chiefly of heated O{sup +}, suggest that the terrestrial ionosphere acts as an important, and at times, dominant source of ions for the magnetosphere. The topside ionospheric processes responsible for modulating both types of polar ion flows were examined to quantify the magnitudes and compositional variability of steady-state polar wind flows and to identify the role of low-altitude frictional heating in transient heavy ion (O{sup +}) upwellings. Theoretical and experimental approaches were used to elucidate the high-latitude processes that influence ionospheric source strength and transient behavior. A time-dependent hydrodynamic model was used to examine solar cycle and seasonal dependencies under steady-state assumptions. The role of low-altitude ion frictional heating was examined by coupling the National Center for Atmospheric Research-Thermosphere/Ionosphere General Circulation Model (NCAR-TIGCM) to the polar wind model to specify time-dependent frictional heating during a period of observed high-altitude O{sup +} outflow. Preferential O{sup +} heating resulted in a factor of four increase in modeled O{sup +} fluxes, which coincides in both space and time with the observed heavy ion outflows. Finally, the role of frictional heating and global heating morphology was related to observations of high-altitude ion outflows using Dynamics Explorer-2 satellite data and incoherent scatter radar observations.
Research Organization:
Michigan Univ., Ann Arbor, MI (United States)
OSTI ID:
7206160
Country of Publication:
United States
Language:
English