activity
20022019
most citedSunrise: instrument, mission, data and first results

328 citations · 2.4k across the 25 of their papers we have counts for

collaborators
Showing 2010Show all

14 papers · 1 filter

astro-ph.SR2010★ 69 cited

Detection of large acoustic energy flux in the solar atmosphere

N. Bello González, M. Franz, V. Martínez Pillet +9

We study the energy flux carried by acoustic waves excited by convective motions at sub-photospheric levels. The analysis of high-resolution spectropolarimetric data taken with IMa…

astro-ph.SR2010★ 28 cited

Surface waves in solar granulation observed with {\sc Sunrise}

M. Roth, M. Franz, N. Bello González +10

Solar oscillations are expected to be excited by turbulent flows in the intergranular lanes near the solar surface. Time series recorded by the IMaX instrument aboard the {\sc Sunr…

astro-ph.SR2010★ 136 cited

SUNRISE/IMaX observations of convectively driven vortex flows in the Sun

J. A. Bonet, I. Marquez, J. Sanchez Almeida +10

We characterize the observational properties of the convectively driven vortex flows recently discovered on the quiet Sun, using magnetograms, Dopplergrams and images obtained with…

astro-ph.SR2010★ 64 cited

Bright points in the quiet Sun as observed in the visible and near-UV by the balloon-borne observatory Sunrise

T. L. Riethmueller, S. K. Solanki, V. Martínez Pillet +13

Bright points (BPs) are manifestations of small magnetic elements in the solar photosphere. Their brightness contrast not only gives insight into the thermal state of the photosphe…

astro-ph.SR2010★ 35 cited

Supersonic Magnetic Upflows in Granular Cells Observed with Sunrise/IMaX

J. M. Borrero, V. Martinez Pillet, R. Schlichenmaier +8

Using the IMaX instrument on-board the Sunrise stratospheric balloon-telescope we have detected extremely shifted polarization signals around the Fe I 5250.217 Å spectral line with…

astro-ph.SR2010★ 134 cited

Fully resolved quiet-Sun magnetic flux tube observed with the Sunrise IMaX instrument

A. Lagg, S. K. Solanki, T. L. Riethmueller +14

Until today, the small size of magnetic elements in quiet Sun areas has required the application of indirect methods, such as the line-ratio technique or multi-component inversions…