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ULF-Sounding of Magnetosphere and Earth

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 353))

The investigation of the pulsation spatial structure was based on the solution of direct problems of MHD-wave propagation. In this chapter, we shall show how the developed concepts can be adapted to the inverse problems, to determine the magnetospheric cold plasma distribution and to study the Earth's crust conductivity by using either ground or satellite ULF-observations.

We will consider a method of ground-based magnetospheric plasma monitoring based on the FLR-theory (see Chapter 6). In this method the distribution of Alfvén velocity and, thus, plasma density, along a field line is obtained from the FLR-frequencies. To this end, the inverse problem is reduced to a spectral problem. The FLR-frequencies are found from the geomagnetic pulsations.

The Earth's crust conductivity is determined by methods known as magnetotelluric sounding (MTS)([10], [32]). The method is based on simultaneous measuring of electric and magnetic fields in the ULF-range. Numerous papers and monographs have been devoted to this topic. However, little attention has been devoted to the influence of magnetospheric peculiarities of MHD-wave propagation and excitation. We shall study the role of resonance magnetic shells in interpreting data of ground-based MTS as well as the possibility of an above ionosphere MTS from low-orbit satellites.

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(2007). ULF-Sounding of Magnetosphere and Earth. In: Hydromagnetic Waves in the Magnetosphere and the Ionosphere. Astrophysics and Space Science Library, vol 353. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-6637-5_11

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