Abstract. A large set of high precision full-Stokes spectropolarimetric obser-vations of prominences in He-D3, H and H lines has been recorded with the ZIMPOL polarimeter at the Gregory-Coude Telescope in Locarno. The obser-vational technique allows us to obtain measurements free from seeing induced spurious eects. The instrumental polarization is well under control and taken into account in the data analysis. We present our observational results for each of the above-mentioned lines. Of particular interest is that most of our H mea-surements show anti-symmetric V proles that are a characteristic signature of the Zeeman eect in the prominence plasma. A Stokes inversion technique based on the quantum theory of the Hanle and Zeeman eects is...
International audienceThe magnetic field vector was measured in a prominence by interpretation of th...
Magnetic fields can be measured, in solar prominences, by means of two different basic mechanisms th...
International audienceOver 1,000 polarization measurements pertaining to about 90 distinct solar pro...
Abstract. Over the last few years a large set of spectropolarimetric observations of prominences and...
International audienceWe report on first spectropolarimetric observations of solar prominences made ...
International audienceWe report on spectropolarimetric observations of Halpha in prominences made wi...
Spectro-polarimetric measurements of the D3-HeI 5876 A line profile in 35 prominences have been perf...
Context. Narrowband imaging spectropolarimetry is one of the most powerful tools available to infer ...
We report on first spectropolarimetric observations of solar prominences made at THEMIS. Hereafter w...
In recent times there has been a strong revival of interest in spectropolarimetric observations of s...
Context. Determining the magnetic field vector in quiescent solar prominences is possible by interpr...
International audienceHanle-effect vector-magnetic-field measurements in the unresolved 5876-A D3 li...
We present spectropolarimetric observations in the He I 1083.0 nm multiplet of a quiescent, hedgerow...
We present novel spectropolarimetric observations of the hydrogen Hα line taken with the Zürich Imag...
International audienceThe magnetic field vector was measured in a prominence by interpretation of th...
Magnetic fields can be measured, in solar prominences, by means of two different basic mechanisms th...
International audienceOver 1,000 polarization measurements pertaining to about 90 distinct solar pro...
Abstract. Over the last few years a large set of spectropolarimetric observations of prominences and...
International audienceWe report on first spectropolarimetric observations of solar prominences made ...
International audienceWe report on spectropolarimetric observations of Halpha in prominences made wi...
Spectro-polarimetric measurements of the D3-HeI 5876 A line profile in 35 prominences have been perf...
Context. Narrowband imaging spectropolarimetry is one of the most powerful tools available to infer ...
We report on first spectropolarimetric observations of solar prominences made at THEMIS. Hereafter w...
In recent times there has been a strong revival of interest in spectropolarimetric observations of s...
Context. Determining the magnetic field vector in quiescent solar prominences is possible by interpr...
International audienceHanle-effect vector-magnetic-field measurements in the unresolved 5876-A D3 li...
We present spectropolarimetric observations in the He I 1083.0 nm multiplet of a quiescent, hedgerow...
We present novel spectropolarimetric observations of the hydrogen Hα line taken with the Zürich Imag...
International audienceThe magnetic field vector was measured in a prominence by interpretation of th...
Magnetic fields can be measured, in solar prominences, by means of two different basic mechanisms th...
International audienceOver 1,000 polarization measurements pertaining to about 90 distinct solar pro...