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...
Magnetic field strength in solar coronal waveguides
We applied Bayesian techniques to the problem of inferring the magnetic field strength in transversely oscillating solar coronal loops from observed periods and...
Magnetic field structures associated with chromospheric heating in a plage region
The strongest quasi-steady heating in the solar atmosphere occurs in the active chromosphere and in particular within plage regions. Our aim is to investigate...
Magnetic fields not only provide a basic tool for observing galaxies but constitute an important clue to interpret many dynamic processes taking place in them...
Magnetic Fields of the Quiet Sun: A New Quantitative Perspective From Hinode
This article summarizes results of studies presented in two papers already published: Lites et al. (2007a); Lites et al. (2007b). Please see these for further...