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Analysis of a Permo-Triassic polarity transition in different absolute reconstructions of Pangaea,considering a model with features of the present Earth magnetic field
Permo-Triassic Pangaea absolute reconstruction Earth magnetic field polarity transition
2015/9/2
The main objective of this paper is to show that the distribution of transitional palaeomagnetic data recorded at 250 Ma are in agreement with simulated data that depend on the sampling site, using a ...
Repeat station data compared to a global geomagnetic field model
Geomagnetic repeat station data crustal bias
2015/8/26
Geomagnetic repeat station surveys with local variometers for improved data reductions have been carried out in Germany for about ten years. For nearly the same time interval the satellites Ørste...
Candidates for multiple impact craters?: Popigai and Chicxulub as seen by the global high resolution gravitational field model EGM2008
Candidates for multiple impact craters Popigai and Chicxulub global high resolution gravitational field model EGM2008
2014/12/31
In 2008 the new Earth Gravitational Model (EGM2008) was released. It contains a complete set of spherical harmonic coefficients of the Earth's gravitational potential (Stokes parameters) to degree 219...
Analytical Model to Study the Behaviour of Auroral Particles in a Local Region of the Magnetotail at the Onset of a Magnetospheric Substorm
Auroral Particles Region Onset Magnetospheric Substorm
2009/6/16
Analytical Model to Study the Behaviour of Auroral Particles in a Local Region of the Magnetotail at the Onset of a Magnetospheric Substorm.
Global Geomagnetic Secular Variation from 1956 to 1976 as Described by a Four-Dipole Model
Global Geomagnetic Secular Variation Four-Dipole Model
2009/6/15
Global Geomagnetic Secular Variation from 1956 to 1976 as Described by a Four-Dipole Model.
The Cosmic Ray Asymptotic Directions for Station Oulu in the Magnetic Field of the Tsyganenko 1989 Model
cosmic rays magnetospheric magnetic field asymptotic directions geomagnetic disturbance level
2009/6/10
Using the magnetospheric field model developed by Tsyganenko (1989) the asymptotic directions
were calculated for cosmic ray particles entering the top of the atmosphere at Oulu (65.°06N, 25.°47E).Th...