DEFINITION OF THE ALFVÉN MODE IN INHOMOGENEOUS MAGNETIC FIELD

Journal Title: Solar-Terrestrial Physics - Year 2023, Vol 9, Issue 1

Abstract

The article is methodological and defines the concept of the linear Alfvén mode. There are two definitions — electrodynamic and hydrodynamic. In the former, the Alfvén mode is considered a wave with a potential transverse electric field. In the latter, waves are more often identified with the Alfvén mode, plasma motion in which is purely vortex. While these definitions are equivalent for homogeneous plasma, they are incompatible if the field line curvature is taken into account: if the transverse electric field is purely potential, the plasma speed has not only a vortex component, but also a potential one, and vice versa. The electrodynamic and hydrodynamic definitions are equivalent only if the wave electric field completely lacks a component along the binormal to the external magnetic field. However, such waves do not exist in nature.

Authors and Affiliations

Klimushkin D. Y. , Mager P. N.

Keywords

Related Articles

COHERENT MICROWAVE EMISSION AS AN INDICATOR OF NON-THERMAL ENERGY RELEASE AT A CORONAL X-RAY POINT

A response has been found in a narrow band 5–7 GHz of microwave emission to the appearance of a coronal X-ray point. The emission source is a short X-ray loop located in the tail part of an active region and occurring wh...

Information Abstract Text Hysteresis effect between geomagnetic activity indices (Ap, Dst) and interplanetary medium parameters in solar activity cycles 21–24

We have studied the relationship of geomagnetic activity indices (Ap, Dst) on time intervals, equal to solar cycles (∼11 years), with solar activity indicators and heliospheric parameters. It is shown that the plots of t...

FEATURES OF DISTRIBUTION OF SEISMIC ACTIVITY IN DIFFERENT REGIONS OF EARTH OVER PHASES OF THE 11-YEAR SOLAR CYCLE

We discuss the relationship of solar activity with the seismicity of Earth and reasons for the differences in the results of studies of various authors. Using the epoch superposition method, we analyze the differences in...

INTERACTION BETWEEN LONG-PERIOD ULF WAVES AND CHARGED PARTICLE IN THE MAGNETOSPHERE: THEORY AND OBSERVATIONS (OVERVIEW)

The paper reviews the current state of the problem of interaction between long-period ultra-low-frequency (ULF) waves and high-energy particles. We consider elements of the theory of energy exchange between waves and par...

DIAGNOSTICS OF AURORAL OVAL BOUNDARIES ON THE BASIS OF THE MAGNETOGRAM INVERSION TECHNIQUE

It is shown that the convection reversal boundary is a fundamental parameter of the magnetosphere-ionosphere coupling, which determines a strong analogy between the electrostatic potential of the ionosphere and the equiv...

Download PDF file
  • EP ID EP714640
  • DOI 10.12737/stp-91202304
  • Views 43
  • Downloads 0

How To Cite

Klimushkin D. Y. , Mager P. N. (2023). DEFINITION OF THE ALFVÉN MODE IN INHOMOGENEOUS MAGNETIC FIELD. Solar-Terrestrial Physics, 9(1), -. https://europub.co.uk/articles/-A-714640