Geoscience Reference
In-Depth Information
be carefully monitored. Thermosphere-ionosphere models such as the present UAM
should be combined with global MHD models of the magnetosphere, taking into
account the plasma sheet not frozen in ions. And last, in the near future both the
“space weather” and the usual weather and climate models should be combined
in some way. Nowadays, computer techniques and technology permit us to realize
these tasks.
Acknowledgments Work at GFZ Potsdam (M.F. and B.P.) was supported by Deutsche
Forschungsgemeinschaft (DFG). We thank the ACE SWEPAM and MAG instrument teams and the
ACE Science Center for providing the data, and the World Data Center for Geomagnetism, Kyoto,
for the D st , ASYM, and AE indices. The CHAMP mission is sponsored by the Space Agency
of the German Aerospace Center (DLR) through funds of the Federal Ministry of Economics
and Technology, following a decision of the German Federal Parliament (grant code 50EE0944).
The data retrieval and operation of the CHAMP satellite by the German Space Operations Center
(GSOC) of DLR is acknowledged.
The authors (A.N. and O.Z.) acknowledge (1) NOAA National Geophysical Data
Center/NGDC and the World Data Center for Geomagnetism, Kyoto, for the Ap, Kp, and
D st indexes data ( http://spidr.ngdc.noaa.gov/spidr/ ) ; (2) U.S. Geological Survey and National
Earthquake Information Center for the earthquake data, URL: http://earthquake.usgs.gov/
earthquakes/ ; (3) IGS community and Crustal Dynamics Data Information System (CDDIS)
for the TEC Global Ionosphere Maps (Noll et al. 2009 ;Noll 2010 ); and (4) University of Hawaii
for Generic Mapping Tools (Wessel and Smith 1998 ).
References
Akhoondzadeh M, Saradjian MR (2011) TEC variations analysis concerning Haiti (January 12,
2010) and Samoa (September 29, 2009) earthquakes. Adv Space Res 47(1):94-104
Amm O, Aruliah A, Buchert SC, Fujii R, Gjerloev JW, Ieda A, Matsuo T, Stolle C, Vanhamaki H,
Yoshikawa A (2008) Towards understanding the electrodynamics of the 3-dimensional
high-latitude ionosphere: present and future. Ann Geophys 26:3913-3932. doi: 10.5194/an-
geo-26-3913-2008
Aruliah AL, Griffins EM, McWhirter I et al (2004) First tristatic studies of meso-scale ion-neutral
dynamics and energetics in the high-latitude upper atmosphere using collocated FPIs and
EISCAT radar ionosphere. Geophys Res Lett 31(L03802):1-4. doi: 10.1029/2003GL018469
Banks PM (1972) Magnetospheric processes and the behavior of the neutral atmosphere. Space
Res 12:1051-1067
Brunelli BE, Namgaladze AA (1988) Fizika ionosfery. Nauka, Moscow, 527 p (in Russian)
Chmyrev VM, Isaev NV, Bilichenko SV, Stanev GA (1989) Observation by space-borne detectors
of electric fields and hydromagnetic waves in the ionosphere over on earthquake center. Phys
Earth Planet Interiors 57:110-114
Coroniti FV, Kennel CF (1973) Can the ionosphere regulate magnetospheric convection? J
Geophys Res 78:2837-2851
Depueva AKh, Ruzhin YuYa (1995) Seismoionospheric fountain-effect as analogue of active space
experiment. Adv Space Res 15(N 12):151-154
Depueva AKh, Mikhailov AV, Devi M, Barbara AK (2007) Spatial and time variations in critical
frequencies of the ionospheric F region above the zone of equatorial earthquake preparation.
Geomagn Aeron 47(N. 1):129-133. doi: 10.1134/S0016793207010197
 
Search WWH ::




Custom Search