Global-scale observations of ionospheric convection variation in response to sudden increases in the solar wind dynamic pressure

Details Global-scale observations of ionospheric convection variation in response to sudden increases in the solar wind dynamic pressure Global-scale observations of ionospheric convection variation in response to sudden increases in the solar wind dynamic pressure

Apr 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012jgra..11704209g&link_type=abstract

Journal of Geophysical Research, Volume 117, Issue A4, CiteID A04209

Physics

Interplanetary Physics: Interplanetary Shocks, Ionosphere: Plasma Convection (2760), Space Weather: Geomagnetically Induced Currents, Space Weather: Solar Effects

Scientific paper

We have used a superposed epoch analysis to study 205 sudden commencement (SC) events detected with ground-based magnetometers between the years 2000 and 2007. The strength of the SC events was clearly correlated to the magnitude of the jump in the solar wind dynamic pressure, regardless of whether or not the SC events were followed by a magnetic storm. Data from the Super Dual Auroral Radar Network (SuperDARN) demonstrated that both the ionospheric plasma drift speed and the number of echoes increased in the noon sector in response to the increase in solar wind dynamic pressure. In contrast, the number of SuperDARN echoes in the midnight sector decreased as the solar wind dynamic pressure increased, even though the average drift speed in the midnight sector also increased. We also uncovered that the ionosphere and ring current evolve differently in response to the pressure pulses. The SYM-H index, which represents changes in both the magnetopause and ring currents, responded immediately and either rapidly returned to pre-SC values or progressed into the main phase of a geomagnetic storm. In contrast, the ionospheric convection data were affected for a much longer time. The implication is that the ring current reacts to a sudden compression of the magnetosphere on a time scale of 10 min, while the convection pattern itself is affected for as long as the increase in solar wind dynamic pressure is sustained, or until a geomagnetic storm was triggered, as is the case in the sudden storm commencement (SSC) subset of events.

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