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During magnetic storms, there is a strong response in the ionosphere and thermosphere which occurs at polar latitudes. Energy input in the form of Poynting flux and energetic particle precipitation, and energy output in the form of heated ions and neutrals have been detected at different altitudes and all local times. We have analyzed a number of storms, using satellite data from the Defense Meteorological Satellite Program (DMSP), the Gravity Recovery and Climate Experiment (GRACE), Gravity field and steady-state Ocean C ...
Published by: Journal of Space Weather and Space Climate Published on: 01/2016
YEAR: 2016   DOI: 10.1051/swsc/2015041
The equatorial ionosphere under conditions of deep solar minimum exhibits structuring due to tidal forces. Data from instruments carried by the Communication/Navigation Outage Forecasting System (C/NOFS) which was launched in April 2008 have been analyzed for the first 2 years following launch. The Planar Langmuir Probe (PLP), Ion Velocity Meter (IVM) and Vector Electric Field Investigation (VEFI) all detect periodic structures during the 2008\textendash2010 period which appear to be tides. However when the tidal features ...
Published by: Journal of Atmospheric and Solar-Terrestrial Physics Published on: 10/2013
YEAR: 2013   DOI: 10.1016/j.jastp.2012.11.009
Published by: Journal of Geophysical Research Published on: Jan-01-2011
YEAR: 2011   DOI: 10.1029/2010JA016164