Physics
Scientific paper
Feb 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jastp..72..193m&link_type=abstract
Journal of Atmospheric and Solar-Terrestrial Physics, Volume 72, Issue 2-3, p. 193-205.
Physics
3
Solar Wind, Geomagnetic Activity, Ionospheric Plasma, Total Electron Content, Zonally Traveling And Zonally Symmetric Oscillations
Scientific paper
The present paper focuses on planetary wave type responses of the thermosphere/ionosphere system to forcing from above and below during the Arctic winter of 2005/2006. The forcing from above is described by the sunspot numbers, the solar wind speed, the Bz-component of the IMF and the geomagnetic Kp-index, while the forcing from below, i.e. by upward propagating atmospheric waves, is represented by the SABER/TIMED temperatures. The observed global ionospheric zonally symmetric oscillations with periods of ~9, ~14 and ~24-27 days were approved to be of solar origin. The most persistent ~9-day oscillation is linked to a triad of solar coronal holes distributed roughly 120° apart in solar longitude. The ~18-day westward propagating wave with zonal wavenumber 1, observed in the ionospheric currents (detected by magnetometer data), and in the F-region plasma (foF2 and TEC) could be allocated to a simultaneous 18-day westward propagating planetary wave observed in the stratosphere/mesosphere/lower thermosphere region with large (~70 km) vertical wavelength.
Andonov Borislav
Borries Claudia
Jakowski Norbert
Mukhtarov Pl.
Pancheva Dora
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