Steve Milan
0000-0001-5050-9604
University of Leicester
259 papers found
Refreshing results…
The orientation and current density of the magnetotail current sheet: A statistical study of the effect of geomagnetic conditions
Dynamics of the region 1 Birkeland current oval derived from the Active Magnetosphere and Planetary Electrodynamics Response Experiment (AMPERE)
Simultaneous ground-satellite observations of meso-scale auroral arc undulations
Comparison between SuperDARN flow vectors and equivalent ionospheric currents from ground magnetometer arrays
A quantitative deconstruction of the morphology of high-latitude ionospheric convection
Global-scale observations of ionospheric convection variation in response to sudden increases in the solar wind dynamic pressure
AXIOM: Advanced X-ray imaging of the magnetosheath
Seasonal and clock angle control of the location of flux transfer event signatures at the magnetopause
Relationship between interplanetary parameters and the magnetopause reconnection rate quantified from observations of the expanding polar cap
The IMF dependence of the local time of transpolar arcs: Implications for formation mechanism
Storm and substorm effects on magnetotail current sheet motion
Alfvén: magnetosphere—ionosphere connection explorers
An assessment of the length and variability of Mercury's magnetotail
Global-scale observations of ionospheric convection during geomagnetic storms
Winds and tides in the mid-latitude Southern Hemisphere upper mesosphere recorded with the Falkland Islands SuperDARN radar
Bifurcations of the main auroral ring at Saturn: ionospheric signatures of consecutive reconnection events at the magnetopause
Dynamic subauroral ionospheric electric fields observed by the Falkland Islands radar during the course of a geomagnetic storm
Geomagnetic storms over the last solar cycle: A superposed epoch analysis
IMPALAS: Investigation of MagnetoPause Activity using Longitudinally-Aligned Satellites—a mission concept proposed for the ESA M3 2020/2022 launch
Tracking corotating interaction regions from the Sun through to the orbit of Mars using ACE, MEX, VEX, and STEREO
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