activity
20052026
most citedMulti-line Stokes inversion for prominence magnetic-field diagnostics

40 citations · 142 across the 12 of their papers we have counts for

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6 papers · 1 filter

astro-ph.IM2026

Error Propagation from Integral Moments and Spectral Derivatives of Stokes Profiles to Magnetic Observables

Roberto Casini

We aim to derive convenient analytic estimations of magnetic inference errors, which can be used to inform and facilitate the creation of the science-traceability matrix of a polar…

astro-ph.IM2026★ 1 cited

Image instabilities and polarization cross-talk

Roberto Casini, Alfred G. de Wijn

We expand on our previous study of the impact of atmospheric seeing on polarization cross-talk, and show how the formalism that was developed in that work can be applied to treat t…

astro-ph.IM2026

Optimal polarization modulation and calibration schemes

Roberto Casini, David M. Harrington, Alfred G. de Wijn

We review the algebraic definition of the efficiency of a polarization modulation scheme, which is commonly adopted for solar and stellar spectro-polarimetry applications, and gene…

astro-ph.IM2013★ 9 cited

Improved search of PCA databases for spectro-polarimetric inversion

R. Casini, A. Asensio Ramos, B. W. Lites +1

We describe a simple technique for the acceleration of spectro-polarimetric inversions based on principal component analysis (PCA) of Stokes profiles. This technique involves the i…

astro-ph.IM2011★ 27 cited

Analysis of Seeing-Induced Polarization Cross-Talk and Modulation Scheme Performance

Roberto Casini, Alfred G. de Wijn, Philip G. Judge

We analyze the generation of polarization cross-talk in Stokes polarimeters by atmospheric seeing, and its effects on the noise statistics of spectropolarimetric measurements for b…

astro-ph.IM2009★ 40 cited

Multi-line Stokes inversion for prominence magnetic-field diagnostics

R. Casini, A. Lopez Ariste, F. Paletou +1

We present test results on the simultaneous inversion of the Stokes profiles of the He I lines at 587.6 nm (D_3) and 1083.0 nm in prominences (90-deg scattering). We created datase…