Spectral Lines in FUV and EUV for Diagnosing Coronal Magnetic Field

The diagnostic capabilities of spectral lines in the far-ultraviolet (FUV) and extreme-ultraviolet (EUV) wavelength ranges are explored in terms of their Hanle and Zeeman sensitivity to probe the vector magnetic fields in the solar corona. The temperature range covered is log ( 10 T ) = 5.5 – 6.3....

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Veröffentlicht in:	Solar physics 2022-07, Vol.297 (7), Article 96
Hauptverfasser:	Khan, Raveena, Nagaraju, K.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics and Astroparticles Atmospheric Sciences Corona Coronal magnetic fields Field strength Line spectra Linear polarization Magnetic fields Physics Physics and Astronomy Polarization Sensitivity Solar corona Solar magnetic field Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Wavelengths Zeeman effect
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