The Hunt for Perpendicular Magnetic Field Measurements in Plasma

被引:0
|
作者
Jensen, Elizabeth A. [1 ,3 ]
Rahmani, Yaser [2 ]
Simpson, Jamesina J. [2 ]
机构
[1] Planetary Sci Inst, 1700 East Ft Lowell,Suite 106, Tucson, AZ 85719 USA
[2] Univ Utah, 50 S Cent Campus Dr, Salt Lake City, UT 84112 USA
[3] ACS Engn & Safety, Spring, TX 77373 USA
来源
ASTROPHYSICAL JOURNAL | 2024年 / 963卷 / 01期
关键词
SOLAR; RADIO;
D O I
10.3847/1538-4357/ad2347
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 portion of the vector that is perpendicular using a modified measurement. Isolating this electromagnetic propagation wave mode to measure the magnetic field enables us to (i) study more about the magnetic field vector in plasma, (ii) reduce error in total electron content measurements, and (iii) discover 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 gyrofrequency, 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.
引用
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页数:6
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