activity
20062026
most citedThe Interface Region Imaging Spectrograph (IRIS)

1.4k citations · 7.3k across the 99 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.SR2016★ 35 cited

Observations of Ellerman bomb emission features in He I D3 and He I 10830 Å

Tine Libbrecht, Jayant Joshi, Jaime de la Cruz Rodríguez +2

Context. Ellerman bombs (EBs) are short-lived emission features, characterized by extended wing emission in hydrogen Balmer lines. Until now, no distinct signature of EBs has been…

astro-ph.SR2016★ 34 cited

Formation of the helium EUV resonance lines

Thomas Peter Golding, Jorrit Leenaarts, Mats Carlsson

Context: While classical models successfully reproduce intensities of many transition region lines, they predict helium EUV line intensities roughly an order of magnitude lower tha…

astro-ph.SR2016★ 103 cited

Non-LTE inversions of the Mg II h&k and UV triplet lines

Jaime de la Cruz Rodríguez, Jorrit Leenaarts, Andrés Asensio Ramos

The Mg II h&k lines are powerful diagnostics for studying the solar chromosphere. They have become particularly popular with the launch of the IRIS satellite, and a number of studi…

astro-ph.SR2016★ 87 cited

3D NLTE analysis of the most iron-deficient star, SMSS0313-6708

Thomas Nordlander, Anish M. Amarsi, Karin Lind +5

Models of star formation in the early universe depend on the details of accretion, fragmentation and radiative feedback. Different simulations predict different initial mass functi…

astro-ph.SR2016★ 40 cited

The cause of spatial structure in solar He I 1083 nm multiplet images

Jorrit Leenaarts, Thomas Golding, Mats Carlsson +2

Context. The He i 1083 nm is a powerful diagnostic for inferring properties of the upper solar chromosphere, in particular for the magnetic field. The basic formation of the line i…

astro-ph.SR2016★ 63 cited

Partial redistribution in 3D non-LTE radiative transfer in solar atmosphere models

Andrii V. Sukhorukov, Jorrit Leenaarts

Resonance spectral lines such as H I Ly α, Mg II h&k, and Ca II H&K that form in the solar chromosphere are influenced by the effects of 3D radiative transfer as well as partial re…