Code for: The Hunt for Perpendicular Magnetic Field Measurements in Plasma

Abstract (updated 2024 January 31): The one consistent technique for remotely estimating the magnetic field in plasma has been Faraday rotation. It is only sensitive to the portion of the vector parallel to the propagation path. We show how to remotely detect the the portion of the vector that is perpendicular using a modified measurement. Isolating this electromagnetic propagation wave mode to measure the magnetic field enables studying (i) more about the magnetic field vector in plasma, (ii) reducing error in total electron content measurements, and (iii) discovering new magnetic field information from archived data sets. The Appleton-Hartree equation is used to verify a new approach to calculating the phase change to an electromagnetic wave propagating through a plasma at frequencies larger than the gryofrequency, the cyclotron frequency, and the upper hybrid frequency. Focusing on the perpendicular propagation modes, the simplified equation for the integrated path effect from a perpendicular magnetic field is calculated. The direction of the perpendicular component is unknown, because the magnetic field is squared. Isolating the magnetic term in the equation with dual frequency waves is shown. We also show how to eliminate the magnetic field contribution to total electron content measurements with a similar approach. In combination with Faraday rotation, the degeneracy of the magnetic field vector direction is reduced to a cone configuration.

 

The MATLAB code provided here produces the figures shown in the pre-print paper: https://doi.org/10.22541/essoar.169724944.44406502/v1

 

This is to be run in MATLAB (tested) or Octave (not tested) by typing

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