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  List of Accepted Contributions - ST5.5 Inter-hemispheric similarities and asymmetries in geospace phenomena

Please, click Abstract Number to find the corresponding abstract as PDF file; if necessary, download Adobe Acrobat Reader 4.0 first to open the file. Any abstract may be freely reproduced for non-commercial, scientific purposes; however, the moral right of the author(s) to be identified as the author(s) of such abstracts is asserted.

EGU06-A-00297
Shirochkov, A. V.
Significant North – South and East – West Asymmetries in the ionospheric Effects of the intense geomagnetic Storms and Superstorms

EGU06-A-00957
Farrugia, C.; Sandholt, P E.
Structure of the reconnecting magnetosphere under a strongly eastward-pointing IMF (but Bz < 0): Simultaneous Observations in both hemispheres under near-equinox conditions

EGU06-A-01201
Sato, N; Kadokura, A; Ebihara, Y; Deguchi, H; Saemundsson, T
Conjugate and non-conjugate auroras observed with TV cameras on the ground

EGU06-A-01211
Lukianova, R; Christiansen, F
Modeling of the global Distribution of ionospheric electric Fields based on realistic Maps of field-aligned Currents

EGU06-A-01472
Ostgaard, N; Mende, S. B.; Frey, H. U.; Sigwarth, J. B.; Aasnes, A.
Substorm onset asymmetries derived from conjugate auroral imaging

EGU06-A-01525
Alfonsi, L.; De Franceschi, G.; Cilliers, P.J.; Materassi, M.; Mitchell, C.N.; Romano, V.; Skone, S.; Spalla, P.; Wernik, A.W.
UAMPY: a contribution to the ICESTAR/IHY activities for the International Polar Year 2007-2008

EGU06-A-03387
Kozlovsky, A.; Meurant, M.; Turunen, T.
The motion of auroral oval caused by a solar wind pressure pulse and associated interplanetary magnetic field disturbances

EGU06-A-05154
Liou, K.
The non-conjugate aspect of large-scale aurora: A review of optical and particle observations

EGU06-A-09178
Fillingim, M. O.; Parks, G. K.; Mende, S. B.
Inter-hemispheric similarities and asymmetries of the afternoon aurora: an indicator of solar wind-magnetosphere energy transfer

EGU06-A-09763
Ridley, A.; Gombosi, T.
Interhemispheric differences in the ionospheric potential


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