Spectro-polarimetric measurements of the D3-HeI 5876 A line profile in 35 prominences have been performed in 2003 with the Gregory-Coud\'e Telescope in Locarno. Two different experimental techniques (ZIMPOL and Beam-exchange method) have been successfully employed to determine all four Stokes components. Both give compatible results. The preliminary results as well as the measurement techniques are reported
We present spectropolarimetric observations in the He I 1083.0 nm multiplet of a quiescent, hedgerow...
Context. Polarimetric observations taken with ground- or space-based telescopes usually need to be c...
We present a summary of data obtained with the 350 μm polarimeter, Hertz, at the Caltech Submillimet...
Abstract. A large set of high precision full-Stokes spectropolarimetric obser-vations of prominences...
International audienceOver 1,000 polarization measurements pertaining to about 90 distinct solar pro...
International audienceWe report on first spectropolarimetric observations of solar prominences made ...
We outline the theory and practice of measuring the four Stokes parameters of spectral lines in emis...
Abstract. Over the last few years a large set of spectropolarimetric observations of prominences and...
We present novel spectropolarimetric observations of the hydrogen Hα line taken with the Zürich Imag...
International audienceHanle-effect vector-magnetic-field measurements in the unresolved 5876-A D3 li...
Context. Narrowband imaging spectropolarimetry is one of the most powerful tools available to infer ...
Metis, the space coronagraph on board the Solar Orbiter, offers us new capabilities for studying eru...
High resolution ( 0.15 Å/pixel ) spectropolarimetry across the Hβ emission line of the Be star γ Cas...
XPOL, the first correlation polarimeter at a large millimeter telescope, uses a flexible digital cor...
Metis on board Solar Orbiter is the space coronagraph developed by an Italian–German–Czech consortiu...
We present spectropolarimetric observations in the He I 1083.0 nm multiplet of a quiescent, hedgerow...
Context. Polarimetric observations taken with ground- or space-based telescopes usually need to be c...
We present a summary of data obtained with the 350 μm polarimeter, Hertz, at the Caltech Submillimet...
Abstract. A large set of high precision full-Stokes spectropolarimetric obser-vations of prominences...
International audienceOver 1,000 polarization measurements pertaining to about 90 distinct solar pro...
International audienceWe report on first spectropolarimetric observations of solar prominences made ...
We outline the theory and practice of measuring the four Stokes parameters of spectral lines in emis...
Abstract. Over the last few years a large set of spectropolarimetric observations of prominences and...
We present novel spectropolarimetric observations of the hydrogen Hα line taken with the Zürich Imag...
International audienceHanle-effect vector-magnetic-field measurements in the unresolved 5876-A D3 li...
Context. Narrowband imaging spectropolarimetry is one of the most powerful tools available to infer ...
Metis, the space coronagraph on board the Solar Orbiter, offers us new capabilities for studying eru...
High resolution ( 0.15 Å/pixel ) spectropolarimetry across the Hβ emission line of the Be star γ Cas...
XPOL, the first correlation polarimeter at a large millimeter telescope, uses a flexible digital cor...
Metis on board Solar Orbiter is the space coronagraph developed by an Italian–German–Czech consortiu...
We present spectropolarimetric observations in the He I 1083.0 nm multiplet of a quiescent, hedgerow...
Context. Polarimetric observations taken with ground- or space-based telescopes usually need to be c...
We present a summary of data obtained with the 350 μm polarimeter, Hertz, at the Caltech Submillimet...