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تسجيل مستخدم جديدHanle signatures of the coronal magnetic field in the linear polarization of the hydrogen LyAlpha line
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M. Derouich
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This paper is dedicated to the assessment of the validity of future coronal spectro-polarimetric observations and to prepare their interpretation in terms of the magnetic field vector.
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Magnetic field measurements in the upper chromosphere and above, where the gas-to-magnetic pressure ratio $beta$ is lower than unity, are essential for understanding the thermal structure and dynamical activity of the solar atmosphere. Recent develop
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