most citedSolar prominences with Na and Mg emissions and centrally reversed Balmer line

9 citations · 15 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR20122 cited

On the Branching in the Emission Relations of Ca II lines in Solar Prominences

G. Stellmacher, E. Wiehr

We observe simultaneously the Ca II K, Ca II 8542 and H-beta emissions in solar prominences at high spatial and spectral resolution. We confirm a branching in the emission relation…

astro-ph.SR2012

Dependence of the He/H8 emission ratio on brightness, temperature, and structuring of prominences

G. Stellmacher, E. Wiehr

We investigate the dependence of the He/H8 emission ratio on kinetic temperature and total Balmer brightness. The line pair He\,{\sc i}\,3888\,Å and H\,3889 has been observed s…

astro-ph.SR20123 cited

Observation of an Instability in a 'Quiescent' Prominence

G. Stellmacher, E. Wiehr

We present the detection of a bubble-like cavity traveling through a quiescent prominence. The H-alpha emission in the cavity is >16 times smaller than in its surroundings. The cav…

astro-ph.SR2012

The Infrared Ca II lines in Sunspot Umbrae

W. Kollatschny, G. Stellmacher, E. Wiehr +1

We present an empirical working model for sunspot umbrae which equally describes observed continuum intensities and line profiles. The wings of the infrared Ca II lines depend sens…

astro-ph.SR20129 cited

Solar prominences with Na and Mg emissions and centrally reversed Balmer line

G. Stellmacher, E. Wiehr

We study spectral lines in exceptionally bright solar limb prominences with pronounced sodium and magnesium emission. We find that most prominences with significant NaD2 and Mgb2 e…

astro-ph.SR20121 cited

On the Origin of the Balmer and Lyman Emission Lines

G. Stellmacher, E. Wiehr

We show how the observed hydrogen Balmer and Lyman emission lines constrain the modeling of quiescent solar prominences. We compare space observations of Lyman lines with ground-ba…