Specific features of the generation of long-periodic geomagnetic pulsations in the event on June 25, 2008

The event of the generation of long-periodic geomagnetic Pc5 pulsations occurring on June 25, 2008 under undisturbed geomagnetic conditions is considered using data from ground-based and satellite observations. Two maxima in the frequency bands 1.9–2.2 and 2.9–3.3 mHz are revealed in the spectra of oscillations in the interplanetary medium, magnetosphere, and on the Earth. Pulsations with frequency 1.9–2.2 mHz were detected in all time sectors from low to high latitudes. The maximum amplitude of the oscillations was recorded in the longitude sector coinciding with position of the ion foreshock region. It is assumed that the event under consideration was caused both by variations of the solar wind dynamic pressure (amplified by the foreshock region) and by the direct penetration of ultra-low-frequency waves from solar wind to the magnetosphere.

[1]  A. Potapov,et al.  Relationship between the fluxes of relativistic electrons at geosynchronous orbit and the level of ULF activity on the Earth’s surface and in the solar wind during the 23rd solar activity cycle , 2012 .

[2]  K. Glassmeier,et al.  Ground-based and satellite observations of traveling magnetospheric convection twin vortices , 1989 .

[3]  Desheng Han,et al.  Coupling of perturbations in the solar wind density to global Pi3 pulsations: A case study , 2007 .

[4]  A. Hasegawa Drift Mirror Instability in the Magnetosphere , 1969 .

[5]  Kazue Takahashi,et al.  Ion flux oscillations associated with a radially polarized transverse Pc 5 magnetic pulsation , 1990 .

[6]  D. Sibeck A model for the transient magnetospheric response to sudden solar wind dynamic pressure variations , 1990 .

[7]  N. Kleimenova,et al.  Geomagnetic pulsations and magnetic disturbances during the initial phase of a strong magnetic storm of May 15, 2005 , 2007 .

[8]  V. Angelopoulos,et al.  The role of transient ion foreshock phenomena in driving Pc5 ULF wave activity , 2013 .

[9]  L. Burlaga,et al.  Magnetic holes in the solar wind , 1976 .

[10]  C. Russell,et al.  Magnetic field orientation and suprathermal ion streams in the earth's foreshock , 1980 .

[11]  C. Russell,et al.  Ogo 5 observations of Pc 5 waves: Particle flux modulations , 1977 .

[12]  V. Parkhomov,et al.  Long-period geomagnetic pulsations caused by the solar wind negative pressure impulse on 22 March 1979 (CDAW-6) , 1998 .

[13]  H. Spence,et al.  Observations of discrete, global magnetospheric oscillations directly driven by solar wind density variations , 2003 .

[14]  A. Du,et al.  Experimental evidence of direct penetration of upstream ULF waves from the solar wind into the magnetosphere during the strong magnetic storm of November 9, 2004 , 2010 .

[15]  D. Constantinescu,et al.  Magnetosheath and heliosheath mirror mode structures, interplanetary magnetic decreases, and linear magnetic decreases: Differences and distinguishing features , 2011 .

[16]  Wolfgang Baumjohann,et al.  The Magnetospheric Response to 8-Minute Period Strong-Amplitude Upstream Pressure Variations , 1989 .