On heliophysical and geophysical phenomena during October-November 2003

Czasopismo : Acta Geophysica
Tytuł artykułu : On heliophysical and geophysical phenomena during October-November 2003

Autorzy :
Yamasaki, K.
Department of Earth and Planetary Sciences, Faculty of Science, Kobe University, Nada, Kobe, Japan, yk2000@kobe-u.ac.jp,
Teisseyre, R.
Institute of Geophysics, Polish Academy of Sciences, Warszawa, Poland, rt@igf.edu.pl,
Herak, M.
University of Zagreb, Faculty of Science and Mathematics, Department of Geophysics, Zagreb, Croatia, herak@irb.hr,
Rosyidi, S. A. P.
Department of Civil Engineering, Muhammadiyah University of Yogyakarta, Yogyakarta, Indonesia, atmaja_sri@umy.ac.id,
Moustafa, S. S. R.
Department of Seismology, National Research Institute of Astronomy and Geophysics, Helwan, Cairo, Egypt, sri@umy.ac.id,
Tenzer, R.
School of Surveying, Faculty of Sciences, University of Otago, Dunedin, New Zealand, robert.tenzer@surveying.otago.ac.nz,
Rabeh, T.
National Research Institute of Astronomy and Geophysics, Cairo, Egypt; Center of Geophysics, Faculty of Science IGIDL, Lisbon University, Lisbon, Portugal, taharabeh@yahoo.com,
Węglarczyk, S.
Cracow University of Technology, Faculty of Environmental Engineering, Kraków, Poland, sweglar@pk.edu.pl,
Huo, Y.
China University of Geosciences, Beijing, China, hyuany@gmail.com,
Shemang, E. M.
Department of Geology, University of Botswana, Gaborone, Botswana, shemae@mopipi.ub.bw,
Meyer, Z.
Department of Geotechnics, West Pomeranian University of Technology, Szczecin, Poland, meyer@ps.pl,
Iwański, R.
Satellite Remote Sensing Centre, Institute of Meteorology and Water Management, Kraków, Poland, rafal.iwanski@imgw.pl,
Chukwuma, V. U.
Department of Physics, Olabisi Onabanjo University, Ago-Iwoye, Nigeria, victorchukwuma@yahoo.com,
Abstrakty : A study of the geomagnetic storm of November 20-21, 2003, is presented using Solar X-rays data, solar wind parameters and magnetic index, Dst. The results suggest that very large X class flares may not cause very intense geomagnetic storms, as flares of M importance would do. Furthermore, the results suggest that the solar wind structure that was responsible for this storm is of the shock-driver gas configuration in which the sheath is the most geoeffective element. Presently it is shown that an intense storm can be driven by two successive southward Bz structures without a resultant “double dip” at the boundary of these structures within the corresponding interval of the main phase. Furthermore, this study confirms earlier results that show that pressure enhancement does not cause the direct injection of new particles into the ring current region; rather it causes a local adiabatic energization of the particles already within the ring current region.

Słowa kluczowe : heliophysical and geophysical phenomena, solar activity, magnetospheric processes, geomagnetic storm,
Wydawnictwo : Instytut Geofizyki PAN
Rocznik : 2009
Numer : Vol. 57, no. 3
Strony : 778 – 800
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DOI :
Cytuj : Yamasaki, K. ,Teisseyre, R. ,Herak, M. ,Rosyidi, S. A. P. ,Moustafa, S. S. R. ,Tenzer, R. ,Rabeh, T. ,Węglarczyk, S. ,Huo, Y. ,Shemang, E. M. ,Meyer, Z. ,Iwański, R. ,Chukwuma, V. U. , On heliophysical and geophysical phenomena during October-November 2003. Acta Geophysica Vol. 57, no. 3/2009
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