activity
20062026
most citedPhysics of Solar Prominences: I - Spectral Diagnostics and Non-LTE Modelling

435 citations · 1.4k across the 49 of their papers we have counts for

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7 papers · 1 filter

astro-ph2008★ 10 cited

Diagnostics of active and eruptive prominences through hydrogen and helium lines modelling

Nicolas Labrosse, Jean-Claude Vial, Pierre Gouttebroze

In this study we show how hydrogen and helium lines modelling can be used to make a diagnostic of active and eruptive prominences. One motivation for this work is to identify the p…

astro-ph2006

O VI and H_2 Lines in Sunspots

Nicolas Labrosse, Huw Morgan, Shadia Rifai Habbal +1

Sunspots are locations on the Sun where unique atmospheric conditions prevail. In particular, the very low temperatures found above sunspots allow the emission of H_2 lines. In thi…

astro-ph2006★ 1 cited

Spectral Diagnostics of Active Prominences

Nicolas Labrosse, Pierre Gouttebroze, Jean-Claude Vial

Active prominences exhibit plasma motions, resulting in difficulties with the interpretation of spectroscopic observations. These solar features being strongly influenced by the ra…

astro-ph2006★ 2 cited

Plasma diagnostic of a solar prominence from hydrogen and helium resonance lines

N. Labrosse, J. -C. Vial, P. Gouttebroze

We present the first comparison of profiles of H et He resonance lines observed by SUMER with theoretical profiles computed with our non-LTE radiative transfer code. We use the H I…

astro-ph2006★ 1 cited

The Helium spectrum in erupting solar prominences

Nicolas Labrosse, Pierre Gouttebroze, Jean-Claude Vial

Even quiescent solar prominences may become active and sometimes erupt. These events are occasionally linked to coronal mass ejections. However we know very little about the plasma…

astro-ph2006★ 24 cited

Effect of motions in prominences on the helium resonance lines in the extreme ultraviolet

Nicolas Labrosse, Pierre Gouttebroze, Jean-Claude Vial

We aim at studying the effect of radial motions on the spectrum emitted by moving prominences in the helium resonance lines and at facilitating the interpretation of observations,…