Studying the connection between the ionosphere and plasmasphere using GPS observations

Physics

Scientific paper

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0994 Instruments And Techniques, 2431 Ionosphere/Magnetosphere Interactions (2736), 2730 Magnetosphere: Inner, 2768 Plasmasphere

Scientific paper

Studying plasmaspheric dynamics during and after magnetic storms provides information on how the plasmasphere responds to and influences storm evolution, and provides insight into magnetosphere-ionosphere coupling. Understanding the source and loss processes of ring current and radiation belt particles requires a dynamic picture of the plasmaspheric mass density, which modifies those populations by particle-particle and indirectly by wave-particle interactions. Studies using plasmaspheric measurements from the IMAGE satellite and ionospheric total electron content measurements from ground-based GPS receivers have demonstrated a striking correlation between stormtime density enhancements in the ionosphere and plasmaspheric drainage plume structure caused by enhanced magnetospheric convection. We describe how the continuous dual-frequency L-band transmissions from 27 Global Positioning Satellites (1.2 and 1.5 GHz), orbiting at about 4 Earth radii, are important observational tools for studying the plasmasphere and ionosphere as a coupled system. Total electron content measurements from ground-based GPS receiver networks are complementary to measurements obtained from zenith-viewing GPS receivers in low-Earth orbit, currently available from a variety of altitudes both within and above the ionosphere. We will report on observed trends such as the plasmaspheric content versus latitude, how this evolves over several hours during a magnetic storm, apparent refilling of the plasmasphere after a storm, and how the plasmasphere structure correlates with ground and space-based GPS measurements of the ionosphere. Since GPS measurements of the plasmasphere are fairly new, we will discuss the measurement system itself, limitations and possible new directions.

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