activity
20022026
most citedPhysics of Solar Prominences: I - Spectral Diagnostics and Non-LTE Modelling

435 citations · 671 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.IM2026

White paper on the relevance of the European Solar Telescope (EST) for the French heliophysics

E. Pariat, Q. Noraz, B. Perri +61

The project of the European Solar Telescope aims to provide a state-of-the art infrastructure to study the Sun and its interactions with Earth and the heliosphere. This 4.2m apertu…

astro-ph.SR2025

Multiwavelength spectroscopic observations of a quiescent prominence

Jianchao Xue, Ping Zhang, Jean-Claude Vial +5

In this paper we focus on the analysis of the multiwavelength spectroscopic observations of a quiescent prominence. The spectral and geometrical parameters in the prominence were d…

astro-ph.IM2019★ 1 cited

The Solar Orbiter SPICE instrument -- An extreme UV imaging spectrometer

The SPICE Consortium, :, M. Anderson +88

The Spectral Imaging of the Coronal Environment (SPICE) instrument is a high-resolution imaging spectrometer operating at extreme ultraviolet (EUV) wavelengths. In this paper, we p…

astro-ph.SR2018★ 32 cited

IRIS Observations of Spicules and Structures Near the Solar Limb

C. E. Alissandrakis, J. -C. Vial, A. Koukras +2

We have analyzed IRIS spectral and slit-jaw observations of a quiet region near the South Pole. In this article we present an overview of the observations, the corrections, and the…

astro-ph.SR2013★ 27 cited

Solar source of energetic particles in interplanetary space during the 2006 December 13 event

C. Li, Y. Dai, J. -C. Vial +5

An X3.4 solar flare and a fast halo coronal mass ejection (CME) occurred on 2006 December 13, accompanied by a high flux of energetic particles recorded both in near-Earth space an…

astro-ph.SR2012★ 32 cited

Kinematics and helicity evolution of a loop-like eruptive prominence

K. Koleva, M. S. Madjarska, P. Duchlev +4

We aim at investigating the morphology, kinematic and helicity evolution of a loop-like prominence during its eruption. We use multi-instrument observations from AIA/SDO, EUVI/STER…

astro-ph.SR2011★ 38 cited

Solar magnetism eXplorer (SolmeX)

H. Peter, L. Abbo, V. Andretta +36

The magnetic field plays a pivotal role in many fields of Astrophysics. This is especially true for the physics of the solar atmosphere. Measuring the magnetic field in the upper s…

astro-ph.SR2010★ 435 cited

Physics of Solar Prominences: I - Spectral Diagnostics and Non-LTE Modelling

N. Labrosse, P. Heinzel, J. -C. Vial +5

This review paper outlines background information and covers recent advances made via the analysis of spectra and images of prominence plasma and the increased sophistication of no…

astro-ph.SR2009★ 16 cited

Hanle signatures of the coronal magnetic field in the linear polarization of the hydrogen LyAlpha line

M. Derouich, F. Auchere, J. C. Vial +1

This paper is dedicated to the assessment of the validity of future coronal spectro-polarimetric observations and to prepare their interpretation in terms of the magnetic field vec…

astro-ph.SR2009★ 8 cited

Electron density in the quiet solar coronal transition region from SoHO/SUMER measurements of S VI line radiance and opacity

E. Buchlin, J. -C. Vial

Context: The sharp temperature and density gradients in the coronal transition region are a challenge for models and observations. Aims: We set out to get linearly- and quadratical…

astro-ph2008★ 20 cited

A Time-Evolving 3D Method Dedicated to the Reconstruction of Solar plumes and Results Using Extreme Ultra-Violet Data

Nicolas Barbey, Frédéric Auchère, Thomas Rodet +1

An important issue in the tomographic reconstruction of the solar poles is the relatively rapid evolution of the polar plumes. We demonstrate that it is possible to take into accou…

astro-ph2007★ 34 cited

Flare magnetic reconnection and relativistic particles in the 2003 October 28 event

C. Li, Y. H. Tang, Y. Dai +2

An X17.2 solar flare occurred on 2003 October 28, accompanied by multi-wavelength emissions and a high flux of relativistic particles observed at 1AU. We present the analytic resul…

astro-ph2002★ 28 cited

A simplified numerical model of coronal energy dissipation based on reduced MHD

E. Buchlin, V. Aletti, S. Galtier +3

A 3D model intermediate between cellular automata (CA) models and the reduced magnetohydrodynamic (RMHD) equations is presented to simulate solar impulsive events generated along a…