492 citations
- W. Schmidt2 profiles80 · h 35
- A. Gandorfer62 · h 32
- S. Solanki3 profiles57 · h 78
- J. C. del Toro Iniesta55 · h 22
- S. Berdyugina2 profiles46 · h 28
- T. Berkefeld2 profiles46 · h 28
- A. Feller2 profiles43 · h 23
- R. Schlichenmaier43 · h 29
- V. Pillet39 · h 38
- J. Hirzberger2 profiles35 · h 31
- J. Borrero33 · h 24
- P. Barthol2 profiles32 · h 25
- Instituto de Astrofísica de CanariasES144 papers
- Max Planck Institute for Solar System ResearchDE129 papers
- Universidad de La LagunaES103 papers
- Instituto de Astrofísica de AndalucíaES83 papers
- Centre National de la Recherche ScientifiqueFR68 papers
- Leibniz Institute for Astrophysics PotsdamDE62 papers
- Kyung Hee UniversityKR61 papers
- NSF NCAR High Altitude ObservatoryUS61 papers
- National Solar ObservatoryUS60 papers
- Istituto Ricerche Solari LocarnoCH56 papers
- Czech Academy of Sciences, Astronomical InstituteCZ54 papers
- University of GöttingenDE47 papers
46 papers · 1 filter
Internal Gravity Waves in the Magnetized Solar Atmosphere. I. Magnetic Field Effects
G. Vigeesh, J. Jackiewicz, O. Steiner
Observations of the solar atmosphere show that internal gravity waves are generated by overshooting convection, but are suppressed at locations of magnetic flux, which is thought t…
Non-magnetic photospheric bright points in 3D simulations of the solar atmosphere
Flavio Calvo, Oskar Steiner, Bernd Freytag
Context. Small-scale bright features in the photosphere of the Sun, such as faculae or G-band bright points, appear in connection with small-scale magnetic flux concentrations. Aim…
A distinct magnetic property of the inner penumbral boundary. II. Formation of a penumbra at the expense of a pore
Jan Jurcak, Nazaret Bello Gonzalez, Rolf Schlichenmaier +1
We recently presented evidence that stable umbra-penumbra boundaries are characterised by a distinct canonical value of the vertical component of the magnetic field, $B^{\rm stable…
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…
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…
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…