Relationship of O+ field-aligned flows and densities to convection speed in the polar cap at 5000 km altitude
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Atmospheric Science,Geophysics
Reference18 articles.
1. EXOS E(Akebono) suprathermal mass spectometer observations of the polar wind;Abe;J. Geophys. Res.,1993
2. Observations of downward moving O+ in the polar topside ionosphere;Chandler;J. Geophys. Res.,1995
3. The polar wind;Ganguli;Rev. Geophys.,1996
4. Dynamics of the H+ and O+ polar wind in the transition region as influenced by ionospheric convection and electron heating;Ho;J. Geophys. Res.,1997
5. The cleft ion fountain: a two-dimensional kinetic model;Horwitz;J. Geophys. Res.,1985
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1. Storm-time electron density enhancement in the cleft ion fountain;Journal of Geophysical Research: Space Physics;2012-11
2. Polar cap electron density distribution from IMAGE radio plasma imager measurements: Empirical model with the effects of solar illumination and geomagnetic activity;Journal of Geophysical Research: Space Physics;2008-01
3. First tomographic image of ionospheric outflows;Geophysical Research Letters;2006-10-19
4. The correlation of plasma density distributions over 5000 km with solar illumination of the ionosphere: Solar cycle and zenith angle observations;Geophysical Research Letters;2003-12
5. Near-simultaneous Polar and DMSP measurements of topside ionospheric field-aligned flows at high latitudes;Journal of Geophysical Research: Space Physics;2001-12-01
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