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Effects of IMF B z reversals on the Ionospheric Critical Frequencies (f 0 F2) between 1975 and 1986. Yurdanur Tulunay Tolga Yapıcı Department of Aerospace Engineering, Middle East Technical University. Content. Introduction Objectives Datasets Criteria for “ Superposed Epoch” Results
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Effects of IMF Bz reversals on the Ionospheric Critical Frequencies (f0F2) between 1975 and 1986 Yurdanur Tulunay Tolga Yapıcı Department of Aerospace Engineering, Middle East Technical University COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Content • Introduction • Objectives • Datasets • Criteria for “Superposed Epoch” • Results • Conclusion • Future Work COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Introduction IMF Bz component Most of the features of the Earth’s magnetosphere and high latitude ionosphere COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Objectives • Investigate the probable effects of IMF Bz on f0F2, • Search the role of geomagnetic conjugacy, • To validate the previously published results. COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Datasets • Ionospheric Critical Frequencies: AZ163 - KG24R, SO166 • Geomagnetic Index: Kp • Interplanetary Magnetic Field COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Criteria for “SuperPosed Epoch” • The Geomagnetically quiet times:3 Hour Planetary Kp Index • Kp≤2+ • Event Definition: IMF Bz • Southward polarity change, • | ΔIMF Bz | > 11 nT, • Polarity should be same for 3 hours before the event • Polarity should be same for 3 hours after the event COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Results – I [Davis et al., 1997] COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Results – II [Davis et al., 1997] COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Results – III(Control Curves) [Tulunay et al., 2001] COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Results – IV(f0F2 distributions AZ163) COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Results – V(f0F2 distributions KG24R) COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Results –VI(f0F2 distributions SO166) COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Results – IV (AZ163) COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Results – V(SO166) COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Conclusion • f0F2 variabilitydue to IMF Bz reversals have been studied. • Due to events, tendency of ~1 MHz decrease in δ(f0F2). COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Discussion – I COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Discussion – II COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Future Work • Develop a model of the ionospheric variability under the IMF By and IMF Bz dynamics. COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
Acknowledgement • Thanks to; • TÜBİTAK ÇAYDAG • COST 724 • Matthew Wild at the World Data Center COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
References • Tulunay, Y., “Interplanetary magnetic field and its possible effects on the mid-latitude ionosphere II”, Annali di Geofisica, 37/2, (1994) • Tulunay, Y., “Interplanetary magnetic field and its possible effects on the mid-latitude ionosphere III”, Annali di Geofisica, 39/4 (1996) • Davis, J. D., Wild, M. N., Lockwood, M., Tulunay, Y., “Ionospheric and geomagnetic responses to changes in IMF Bz: a superposed epoch study”, Annales Geophysicae, 15, 217-230 (1997) • O. A. Troshichev, “Plasma pressure and the field aligned currents in the magnetosphere”, Advances in Space Sciences, 33, 729-736 (2005) • Nelson C. Maynard, “Coupling The Solar-Wind/IMF To The Ionosphere Through The High Latitude Cusps”, Surveys in Geophysics, 26: 255–280 (2005) • J. Merka, J. Safrankova, Z. Nemecek and J. Sımunek, “Magion-4 High-Altitude Cusp Study”, Surveys in Geophysics, 26: 57–69 (2005) • For Data: • http://spidr.ngdc.noaa.gov/spidr/index.jsp • World Data Centre at Rutherford • Matthew Wild COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
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