activity
20042026
most citedSunrise: instrument, mission, data and first results

328 citations · 4k across the 98 of their papers we have counts for

collaborators
Showing 2016Show all

10 papers · 1 filter

astro-ph.SR2016★ 23 cited

Morphological properties of slender Ca II H fibrils observed by SUNRISE II

R. Gafeira, A. Lagg, Sami K Solanki +12

We use seeing-free high spatial resolution Ca II H data obtained by the SUNRISE observatory to determine properties of slender fibrils in the lower solar chromosphere. In this work…

astro-ph.SR2016★ 8 cited

Spectropolarimetric evidence for a siphon flow along an emerging magnetic flux tube

Iker S. Requerey, B. Ruiz Cobo, J. C. Del Toro Iniesta +12

We study the dynamics and topology of an emerging magnetic flux concentration using high spatial resolution spectropolarimetric data acquired with the Imaging Magnetograph eXperime…

astro-ph.SR2016★ 29 cited

A new MHD-assisted Stokes inversion technique

T. L. Riethmüller, S. K. Solanki, P. Barthol +10

We present a new method of Stokes inversion of spectropolarimetric data and evaluate it by taking the example of a SUNRISE/IMaX observation. An archive of synthetic Stokes profiles…

astro-ph.SR2016★ 41 cited

A Tale of Two Emergences: Sunrise II Observations of Emergence Sites in a Solar Active Region

Rebecca Centeno, Julian Blanco Rodriguez, Jose Carlos Del Toro Iniesta +11

In June 2013, the two scientific instruments onboard the second Sunrise mission witnessed, in detail, a small-scale magnetic flux emergence event as part of the birth of an active…

astro-ph.SR2016★ 16 cited

Kinematics of Magnetic Bright Features in the Solar Photosphere

Shahin Jafarzadeh, S. K. Solanki, R. H. Cameron +12

Convective flows are known as the prime means of transporting magnetic fields on the solar surface. Thus, small magnetic structures are good tracers of the turbulent flows. We stud…

astro-ph.SR2016★ 85 cited

Solar Coronal Loops Associated with Small-scale Mixed Polarity Surface Magnetic Fields

L. P. Chitta, H. Peter, S. K. Solanki +12

How and where are coronal loops rooted in the solar lower atmosphere? The details of the magnetic environment and its evolution at the footpoints of coronal loops are crucial to un…