activity
20102022
most citedPrevalence of Small-scale Jets from the Networks of the Solar Transition Region and Chromosphere

335 citations · 759 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2022★ 99 cited

The European Solar Telescope

C. Quintero Noda, R. Schlichenmaier, L. R. Bellot Rubio +14

The European Solar Telescope (EST) is a project aimed at studying the magnetic connectivity of the solar atmosphere, from the deep photosphere to the upper chromosphere. Its design…

astro-ph.SR2014★ 153 cited

On the prevalence of small-scale twist in the solar chromosphere and transition region

B. De Pontieu, L. Rouppe van der Voort, S. W. McIntosh +21

The solar chromosphere and transition region (TR) form an interface between the Sun's surface and its hot outer atmosphere. Here most of the non-thermal energy that powers the sola…

astro-ph.SR2014★ 335 cited

Prevalence of Small-scale Jets from the Networks of the Solar Transition Region and Chromosphere

H. Tian, E. E. DeLuca, S. R. Cranmer +24

As the interface between the Sun's photosphere and corona, the chromosphere and transition region play a key role in the formation and acceleration of the solar wind. Observations…

astro-ph.SR2014★ 88 cited

Observations of Subarcsecond Bright Dots in the Transition Region above Sunspots with the Interface Region Imaging Spectrograph

H. Tian, L. Kleint, H. Peter +5

Observations with the Interface Region Imaging Spectrograph (IRIS) have revealed numerous sub-arcsecond bright dots in the transition region above sunspots. These bright dots are s…

astro-ph.SR2014★ 84 cited

Detection of supersonic downflows and associated heating events in the transition region above sunspots

L. Kleint, P. Antolin, H. Tian +18

IRIS data allow us to study the solar transition region (TR) with an unprecedented spatial resolution of 0.33 arcsec. On 2013 August 30, we observed bursts of high Doppler shifts s…

astro-ph.SR2010

Turbulent magnetic fields in the quiet Sun: A search for cyclic variations

L. Kleint, S. V. Berdyugina, A. I. Shapiro +1

Turbulent magnetic fields fill most of the volume of the solar atmosphere. However, their spatial and temporal variations are still unknown. Since 2007, during the current solar mi…