Field-perpendicular and field-aligned plasma flows observed by EISCAT during a prolonged period of northward IMF

• Published in: Journal of Atmospheric and Terrestrial Physics
• Main Authors: Farmer, A.D, Lockwood, Mike, Horne, R.B, Bromage, B.J.I, Freeman, K.S.C
• Format: Article in Journal/Newspaper
• Language: unknown
• Published: 1984
• Subjects: EISCAT; Tromsø
• Online Access: https://centaur.reading.ac.uk/38919/; https://doi.org/10.1016/0021-9169(84)90066-7

The effect of a prolonged period of strongly northward Interplanetary Magnetic Field (IMF) on the high-latitude F-region is studied using data from the EISCAT Common Programme Zero mode of operation on 11–12 August 1982. The analysis of the raw autocorrelation functions is kept to the directly derived parameters Ne, Te, Ti and velocity, and limits are defined for the errors introduced by assumptions about ion composition and by changes in the transmitted power and system constant. Simple data-cleaning criteria are employed to eliminate problems due to coherent signals and large background noise levels. The observed variations in plasma densities, temperatures and velocities are interpreted in terms of supporting data from ISEE-3 and local riometers and magnetometers. Both field-aligned and field-perpendicular plasma flows at Tromsø showed effects of the northward IMF: convection was slow and irregular and field-aligned flow profiles were characteristic of steady-state polar wind outflow with flux of order 1012 m−2 s−1. This period followed a strongly southward IMF which had triggered a substorm. The substorm gave enhanced convection, with a swing to equatorward flow and large (5 × 1012 m−2 s−1), steady-state field-aligned fluxes, leading to the possibility of O+ escape into the magnetosphere. The apparent influence of the IMF over both field-perpendicular and field-aligned flows is explained in terms of the cross-cap potential difference and the location of the auroral oval.