405 citations · 551 across the 9 of their papers we have counts for
9 papers
The Effect of Stellar Contamination on Low-resolution Transmission Spectroscopy: Needs Identified by NASA's Exoplanet Exploration Program Study Analysis Group 21
Benjamin V. Rackham, Néstor Espinoza, Svetlana V. Berdyugina +58
Study Analysis Group 21 (SAG21) of NASA's Exoplanet Exploration Program Analysis Group (ExoPAG) was organized to study the effect of stellar contamination on space-based transmissi…
High-frequency Oscillations in Small Magnetic Elements Observed with Sunrise/SuFI
Shahin Jafarzadeh, S. K. Solanki, M. Stangalini +3
We characterize waves in small magnetic elements and investigate their propagation in the lower solar atmosphere from observations at high spatial and temporal resolution. We use t…
Chromospheric and Coronal Wave Generation in a Magnetic Flux Sheath
Yoshiaki Kato, Osker Steiner, Viggo Hansteen +3
Using radiation magnetohydrodynamic simulations of the solar atmospheric layers from the upper convection zone to the lower corona, we investigate the self-consistent excitation of…
Recent Advances in the Exploration of the Small-Scale Structure of the Quiet Solar Atmosphere: Vortex Flows, the Horizontal Magnetic Field, and the Stokes-V Line-Ratio Method
O. Steiner, R. Rezaei
We review (i) observations and numerical simulations of vortical flows in the solar atmosphere and (ii) measurements of the horizontal magnetic field in quiet Sun regions. First, w…
Simulations of stellar convection with CO5BOLD
Bernd Freytag, Matthias Steffen, Hans-Günter Ludwig +3
High-resolution images of the solar surface show a granulation pattern of hot rising and cooler downward-sinking material -- the top of the deep-reaching solar convection zone. Con…
The Horizontal Magnetic Field of the Quiet Sun: Numerical Simulations in Comparison to Observations with Hinode
O. Steiner, R. Rezaei, R. Schlichenmaier +2
Three-dimensional magnetohydrodynamic simulations of the surface layers of the Sun intrinsically produce a predominantly horizontal magnetic field in the photosphere. This is a rob…