International audienceThe aim of the present work is twofold: a) to validate the Milne-Eddington UNNOFIT inversion by comparing its results with those of the SIR inversion, which is in LTE but does not assumes the Milne-Eddington atmosphere; b) to present a decrease of the network local average magnetic field strength in the vicinity of a filament/prominence, observed before its disppearance, suggesting that the disappearance results from a weakening of the magnetic support
Context. The design of modern instruments does not only imply thorough studies of instrumental effec...
International audienceThe magnetic field vector of the quiet Sun has been first determined by usual ...
International audienceContext. Direct magnetic field measurements in solar prominences occur infrequ...
International audienceThe aim of the present work is twofold: a) to validate the Milne-Eddington UNN...
International audienceAims:We inverted a spectropolarimetric scan of an active region and a filament...
International audienceThe magnetic field vector was measured in a prominence by interpretation of th...
International audienceThis paper presents the inversion of a spectro-polarimetric scan (240 arcsec×3...
Aims.We inverted a spectropolarimetric scan of an active region and a filament ($240\times 340$ arcs...
International audienceContext. Magnetic field vector measurements are always ambiguous, that is, two...
Context. The design of modern instruments does not only imply thorough studies of instrumental effec...
International audienceThe magnetic field vector of the quiet Sun has been first determined by usual ...
International audienceContext. Direct magnetic field measurements in solar prominences occur infrequ...
International audienceThe aim of the present work is twofold: a) to validate the Milne-Eddington UNN...
International audienceAims:We inverted a spectropolarimetric scan of an active region and a filament...
International audienceThe magnetic field vector was measured in a prominence by interpretation of th...
International audienceThis paper presents the inversion of a spectro-polarimetric scan (240 arcsec×3...
Aims.We inverted a spectropolarimetric scan of an active region and a filament ($240\times 340$ arcs...
International audienceContext. Magnetic field vector measurements are always ambiguous, that is, two...
Context. The design of modern instruments does not only imply thorough studies of instrumental effec...
International audienceThe magnetic field vector of the quiet Sun has been first determined by usual ...
International audienceContext. Direct magnetic field measurements in solar prominences occur infrequ...