Long term studies of equatorial spread F using the JULIA radar at Jicamarca

By D. Hysell, J. Burcham. 2002

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Thermospheric responses to gravity waves: Influences of increasing viscosity and thermal diffusivity (2005, background): “The prediction of larger GW amplitudes near 200 km at solar minimum appears to correlate with stronger ESF and plasma bubble activity observed under these conditions [Hysell and Burcham, 2002].”
Occurrence characteristics of plasma bubble derived from global ground‐based GPS receiver networks (2007, methodology): “[43] The difference of apex altitudes on the solar activity agrees with study of solar cycle dependence of plasma bubble with a Jicamarca unattended long term investigations of the ionosphere and atmosphere (JULIA) radar [ Hysell and Burcham, 2002 ].”
On the enigma of day‐to‐day variability in equatorial spread F (2005, background): “The problem is perplexing because, climatologically, ESF is closely related to the appearance of an eastward electric field (~E) during post-sunset rise (PSSR) of the F layer [Fejer et al., 1999; Hysell and Burcham, 2002]; yet, on a given evening, the two phenomena can appear unrelated.”