Yurdanur Tulunay Tolga Yapıcı
description
Transcript of Yurdanur Tulunay Tolga Yapıcı
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
1
Effects of IMF Bz reversals on the Ionospheric Critical Frequencies (f0F2)
between 1975 and 1986
Yurdanur TulunayTolga Yapıcı
Department of Aerospace Engineering, Middle East Technical University
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
2
Content
Introduction Objectives Datasets Criteria for “Superposed Epoch” Results Conclusion Future Work
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
3
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
4
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
5
Datasets
Ionospheric Critical Frequencies:
AZ163 - KG24R,AZ163 - KG24R,
SO166SO166
Geomagnetic Index:
KpKp
Interplanetary Magnetic Field
Name CodeGeom. Lat.
Geom. Long.
Arkangelsk AZ163 60.38 N 117.54 E
Kerguelen Islands
KG24R 58.47 S 121.83 E
Sodankyla SO166 63.74 N 107.68 E
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
6
Criteria for “SuperPosed Epoch”“SuperPosed Epoch”
The Geomagnetically quiet times:3 Hour Planetary Kp Index3 Hour Planetary Kp Index
1. Kp≤2+
Event Definition:IMF BIMF Bzz
1. Southward polarity change,2. | ΔIMF Bz | > 11 nT,3. Polarity should be same for 3 hours before the event4. Polarity should be same for 3 hours after the event
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
7
Results – I
[Davis et al., 1997]
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
8
Results – II
[Davis et al., 1997]
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
9
Results – III (Control Curves)
[Tulunay et al., 2001]
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
10
Results – IV (f0F2 distributions AZ163)
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
11
Results – V (f0F2 distributions KG24R)
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
12
Results –VI (f0F2 distributions SO166)
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
13
Results – IV (AZ163)
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
14
Results – V (SO166)
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
15
Conclusion
ff00F2 variabilityF2 variability due to IMF BIMF Bzz reversals reversals have been studied.
Due to events, tendency of ~1 MHz~1 MHz decrease in δ(f0F2).
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
16
Discussion – I
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
17
Discussion – II
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
18
Future Work
Develop a modelmodel of the ionospheric variabilityvariability under the IMF BIMF Byy and IMF B and IMF Bzz
dynamicsdynamics.
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
19
Acknowledgement
Thanks to;
– TÜBİTAK ÇAYDAG– COST 724– Matthew Wild at the World Data Center
COST 724 MCM, Antalya, TURKEY, 27-30/03/2006
20
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
21
Thanks for listening...