20.02.2013 Views

PROBLEMS OF GEOCOSMOS

PROBLEMS OF GEOCOSMOS

PROBLEMS OF GEOCOSMOS

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Proceedings of the 7th International Conference "Problems of Geocosmos" (St. Petersburg, Russia, 26-30 May 2008)<br />

c. The relation Z/H is used in an attempt to predict the earthquakes.<br />

Here E and H are the horizontal components of the electric and magnetic fields, Z is the vertical<br />

component of the magnetic field, and θ is the phase angle between the E and Z oscillations.<br />

In addition we would like to mention a new approach to study the ULF geoelectromagnetic field<br />

(Guglielmi et al., 2007). This is the spectral-polarization method which rests on the evaluation of the Stokes<br />

parameters at a given point on the earth’s surface. It allows estimating of the Alfvén resonant frequency by<br />

using the ground-based observation of the Pc3-4 magnetospheric oscillations. The spectral-polarization<br />

method is scheduled to use in the Geophysical Observatory Borok (Φ = 54.05 o , Λ = 119.44 o , L = 2.9) in the<br />

frame of BARS project (“Study of the Alfvén Resonances in Borok”). It has been elaborated the special<br />

equipment, the appropriate software support, and the field test of the method has been provided. The result<br />

shows that the spectral-polarization method may be apparently used for the estimating of the Alfvén resonant<br />

frequencies. We have made the special attention to the study of anharmonicity of the Pc3-4 waves.<br />

4. SYNCHRONOUS DETECTION<br />

The theory of the finite-amplitude standing Alfvén waves predicts the phenomenon of frequency<br />

doubling. It has been found by use of both numerical simulations (Rankin et al., 1994) and perturbation<br />

theory in the second (lowest) order of nonlinearity (Dmitrienko, 2005). However, as we know, the magnetic<br />

observations of the frequency doubling were absent hitherto. The goal of our work in the frame of BARS<br />

project is to fill this gap by using the method of synchronous detection method which allows to identify a<br />

weak signal against the background of interferences (Guglielmi and Zotov, 2007). It is not easy to observe<br />

the phenomenon since the spectrum of Alfvén oscillations of the magnetosphere is non-equidistant, and<br />

therefore the nonlinear oscillations at a frequency twice than the frequency of pumping oscillations are out of<br />

resonance. Oscillogram and Fourier-spectrum do not show the effect of frequency doubling. To overcome<br />

this specific difficulty we have used the synchronous detection method which allows us to identify the<br />

desired weak signal against the background of interferences.<br />

Fig. 3. Spectrum of oscillations (left panel) and synchronous detection of the frequency doubling<br />

(right panel).<br />

As an example let us consider Fig. 3. The Pc3 oscillations have been registered on 9 April 2007, at<br />

10-12 UT at GO Borok. In Fig. 3 we see that the spectrum (left panel) has the pronounced maximum at the<br />

frequency of 50 mHz. We see also that the spectral analysis does not allow us to detect the effect of<br />

frequency doubling. In contrast, the application of the synchronous detection method (right panel in Fig. 3)<br />

leads to conclusion that the oscillations with frequency of 100 mHz are really generated. We believe that this<br />

is the nonlinear effect of frequency doubling because the spectrum of linear oscillations of the<br />

magnetosphere is evidently non-equidistant.<br />

The key innovation here is as follows: By using the method of synchronous detection it has been<br />

established that the effect of frequency doubling may be clearly detected. Even being small, effect of the 2 nd<br />

harmonic generation will has important geophysical consequences, e.g., for the development of nonlinear<br />

hydromagnetic spectroscopy of the space plasma.<br />

94

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!