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Related papers: He-D3 Polarization observed in Prominences

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A large set of high precision full-Stokes spectropolarimetric observations of prominences in He-D3, Halpha and Hbeta lines has been recorded with the ZIMPOL polarimeter at the Gregory-Coude Telescope in Locarno. The observational technique…

Solar and Stellar Astrophysics · Physics 2009-06-15 R. Ramelli , M. Bianda , J. Trujillo Bueno , L. Merenda , J. O. Stenflo

A large set of high precision full-Stokes spectropolarimetric observations of the He-D3 line in spicules has been recorded with the ZIMPOL polarimeter at the Gregory-Coude Telescope in Locarno. The observational technique allow us to obtain…

Solar and Stellar Astrophysics · Physics 2010-11-26 R. Ramelli , M. Bianda , L. Merenda , J. Trujillo Bueno

We analyze the observations of a quiescent prominence acquired by the Telescope Heliographique pour l'Etude du Magnetisme et des Instabilites Solaires (THEMIS) in the He I 5876 A (He I D3) multiplet aiming to measure the spectral…

Solar and Stellar Astrophysics · Physics 2017-12-27 J. Koza , J. Rybák , P. Gömöry , M. Kozák , A. López Ariste

Stellar prominences detected in rapidly rotating stars serve as probes of the magnetism in the corona of cool stars. We have synthesized the temporal evolution of the Stokes profiles generated in the He I 10830 and 5876 A triplets during…

Solar and Stellar Astrophysics · Physics 2016-12-21 T. Felipe , M. J. Martínez González , A. Asensio Ramos

Prominences are cool overdensities of plasma supported by magnetic fields that levitate in the solar corona. The physical characterization of these structures is key for understanding the magnetic field in the corona. Our work attempts to…

Solar and Stellar Astrophysics · Physics 2025-03-06 S. Esteban Pozuelo , A. Asensio Ramos , J. Trujillo Bueno , R. Ramelli , F. Zeuner , M. Bianda

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 datasets of synthetic Stokes profiles for the case of quiescent…

Instrumentation and Methods for Astrophysics · Physics 2009-09-28 R. Casini , A. Lopez Ariste , F. Paletou , L. Leger

Spectropolarimetric observations of solar flares in the He I D$_3$ line at 5876 {\AA} are extremely rare, and their diagnostic potential remains largely unexplored. We report the first unambiguous detection of linear polarization in He I…

The diagnosis of new high-resolution spectropolarimetric observations of solar prominences made in the visible and near-infrared mainly, requires a radiative modelling taking into account for both multi-dimensional geometry and complex…

Astrophysics · Physics 2015-05-13 L. Leger , F. Paletou

We determine an optimal width and shape of the narrow-band filter centered around the He\,{\sc i} D$_{3}$ line for prominence and coronal mass ejection (CME) observations with the ASPIICS ({\it Association of Spacecraft for Polarimetric and…

Solar and Stellar Astrophysics · Physics 2018-07-03 S. Jejčič , P. Heinzel , N. Labrosse , A. N. Zhukov , A. Bemporad , S. Fineschi , S. Gunár

We present new spectropolarimetric observations of the chromospheric He I 10830 {\AA} multiplet observed in a filament during its phase of activity. The data were recorded with the new Tenerife Infrared Polarimeter (TIP-II) at the German…

Solar and Stellar Astrophysics · Physics 2011-02-09 C. Sasso , A. Lagg , S. K. Solanki

We study the formation of the Stokes profiles of the He I multiplet at 10830 A when relaxing two of the approximations that are often considered in the modeling of this multiplet, namely the lack of self-consistent radiation transfer and…

Solar and Stellar Astrophysics · Physics 2023-07-05 Andres Vicente Arevalo , Jiri Stepan , Tanausu del Pino Aleman , Maria Jesus Martinez Gonzalez

Full Stokes spectropolarimetric data (in the 10830 A region) of an active region filament were obtained in July 2005 using the Tenerife Infrared Polarimeter instrument. The polarization profiles in the filament show Zeeman-like signatures.…

Solar and Stellar Astrophysics · Physics 2010-01-15 C. Kuckein , R. Centeno , V. Martinez Pillet

We present preliminary results of 2D radiative modelling of He I lines in solar prominences, using a new numerical code developed by us (Leger, Chevallier and Paletou 2007). It treats self-consistently the radiation transfer and the non-LTE…

Astrophysics · Physics 2008-07-11 L. Leger , F. Paletou

We show preliminary results of an ongoing investigation aimed at determining the configuration of the magnetic field vector in the threads of a quiescent hedgerow solar prominence using high-spatial resolution spectropolarimetric…

Solar and Stellar Astrophysics · Physics 2019-08-19 D. Orozco Suarez , A. Asensio Ramos , J. Trujillo Bueno

We report Stokes vector observations of solar spicules and a prominence in the He I 1083 nm multiplet carried out with the Tenerife Infrared Polarimeter. The observations show linear polarization profiles that are produced by scattering…

Solar and Stellar Astrophysics · Physics 2015-06-11 M. J. Martínez González , A. Asensio Ramos , R. Manso Sainz , C. Beck , L. Belluzzi

Measurements of polarized neutron--polarized $^3$He scattering are reported. The target consisted of cryogenically-polarized solid $^3$He, thickness 0.04 atom/b and polarization 40%. The longitudinal and transverse total cross-section…

Nuclear Experiment · Physics 2009-10-30 C. D. Keith , C. R. Gould , D. G. Haase , M. L. Seely , P. R. Huffman , N. R. Roberson , W. Tornow , W. S. Wilburn

Stellar activity remains one of the primary challenges in the detection and characterization of low-mass exoplanets, as it can induce radial velocity (RV) variations that mask or mimic planetary signals. Identifying reliable activity…

This thesis is dedicated to a study of a spin-isospin structure of the polarized ${}^3\mathrm{He}$. First, an introduction to the spin structure of ${}^3\mathrm{He}$ is given, followed by a brief overview of past experiments. The main focus…

Nuclear Experiment · Physics 2012-08-06 Miha Mihovilovic

For about a decade, spectro-polarimetry of HeI 10830 has been applied to the magnetic diagnostics of the solar chromosphere. This resonance line is very versatile, as it is visible both on disk and in off-limb structures, and it has a good…

Astrophysics · Physics 2011-02-11 R. Casini , R. Manso Sainz , B. C. Low

We describe the neutron polarimeter NPOL3 for the measurement of polarization transfer observables $D_{ij}$ with a typical high resolution of $\sim$300 keV at $T_n$ $\simeq$ 200 MeV. The NPOL3 system consists of three planes of neutron…

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