The spectroscopic determinations of the solar magnetic fields are based on the Zeeman effect observed in relation to a number of absorption lines of the solar...
Magnetic Discontinuity in the Upper Solar Chromosphere Associated with Coronal Loop Brightening Revealed by the CLASP2.1 Observation
We have developed an advanced ultraviolet (UV) spectropolarimeter called Chromospheric Layer SpectroPolarimeter (CLASP2), designed to explore the magnetic...
Magnetic field diagnostics through the second solar spectrum: a spectroscopic analysis of the most polarizing atomic lines
Detailed observations of the second solar spectrum have shown a complex phenomenology whose detailed interpretation is still in a preliminary phase. The only...
Magnetic field inversions from Stokes profiles generated by MHD simulations
We report tests of inversion methods applied to complex Stokes spectra generated by realistic MHD simulations. The average magnetic field strength of the...
Techniques involved in measurements of solar magnetic field are based on the observation and interpretation of the polarization signal in suitable Fraunhofer...
Magnetic Field Morphology Studied by Multi-scale Polarimetry in and around the Filamentary Dark Cloud GF-9
We present a summary of results obtained by Poidevin & Bastien (2006) in the GF-9 core region. Multi-scale analysis is used and suggests that an original...
Magnetic field oscillations in sunspots and active regions
In order to investigate the oscillatory behaviour of the magnetic field in sunspots and pores, full Stokes measurements of 1.56 μm iron lines have been...