Sun-like stars produce superflares roughly once per century
por: Vasilyev, Valeriy, et al.
Publicado: (2024)

Molecular hydrogen controls the temperatures of flares on TRAPPIST-1
por: Solanki, Alexander I. Shapiro Nadiia Kostogryz Sara Seager Veronika Witzke Julien de Wit Valeriy Vasilyev Astrid M. Veronig Robert Cameron Hardi Peter Sami K.
Publicado: (2026)

Testing MURaM and MPS-ATLAS against the quiet solar spectrum
por: Witzke, Veronika, et al.
Publicado: (2023)

Low-latitude magnetic flux emergence on rapidly rotating solar-type stars
por: Işık, Emre, et al.
Publicado: (2024)

Stellar Surface Magnetic Fields Impact Limb Darkening
por: Kostogryz, Nadiia M., et al.
Publicado: (2024)

Solar variability in the Mg II h and k lines
por: Sowmya, K., et al.
Publicado: (2025)

First Calculations of Starspot Spectra based on 3D Radiative Magnetohydrodynamics Simulations
por: Smitha, H. N., et al.
Publicado: (2024)

Decoding the Radial Velocity Signatures of Solar Faculae with 3D MHD Simulations
por: Kröll, Florian, et al.
Publicado: (2026)

The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates
por: Isik, Emre, et al.
Publicado: (2025)

Synthetic disk-integrated absorption lines isolating stellar granulation for high-precision RV studies
por: Frame, Ginger, et al.
Publicado: (2026)

Towards understanding stellar variability at the sub m/s level: Isolating granulation signals in synthetic spectral lines
por: Frame, Ginger, et al.
Publicado: (2025)

Small-scale Dynamo in Cool Stars III. Changes in the photospheres of F3V to M0V stars
por: Bhatia, Tanayveer S., et al.
Publicado: (2023)

The mean solar butterfly diagram and poloidal field generation rate at the surface of the Sun
por: Cloutier, Simon, et al.
Publicado: (2024)

A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy
por: Vasilyev, Valeriy, et al.
Publicado: (2026)

Detectability of Solar Rotation Period Across Various Wavelengths
por: Vasilyev, Valeriy, et al.
Publicado: (2025)

Flares on TRAPPIST-1 reveal the spectrum of magnetic features on its surface
por: Vasilyev, Valeriy, et al.
Publicado: (2025)

The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes
por: Bekki, Yuto, et al.
Publicado: (2024)

Non-thermal broadening of coronal lines in a 3D MHD loop model
por: Breu, C. A., et al.
Publicado: (2024)

Reliable Transmission Spectrum Extraction with a Three-Parameter Limb Darkening Law
por: Keers, Rosa E., et al.
Publicado: (2024)

$\texttt{globin}$: A spectropolarimetric inversion code for the coupled inference of atomic line parameters
por: Vukadinović, D., et al.
Publicado: (2024)

Hydrogen Ionization Inside the Sun
por: Baturin, V. A., et al.
Publicado: (2024)

3D Radiative MHD Simulations of Starspots II: Large-scale Structure
por: Bhatia, Tanayveer Singh, et al.
Publicado: (2024)

Mg II h&k spectral line properties computed using 3D radiative transfer in an enhanced network region simulated with the MURaM-ChE code
por: Ondratschek, P., et al.
Publicado: (2026)

Non-LTE abundances of nitrogen in the Sun and reference A-F type stars
por: Mashonkina, L. I., et al.
Publicado: (2024)

Diversity of morphology of type II spicules in MURaM-ChE simulations
por: Chandra, Sanghita, et al.
Publicado: (2026)

Coriolis force acting on near-surface horizontal flows during simulations of flux emergence produces a tilt angle consistent with Joy's law on the Sun
por: Roland-Batty, William, et al.
Publicado: (2025)

A flux-independent increase in outflows prior to the emergence of active regions on the Sun
por: Schunker, Hannah, et al.
Publicado: (2024)

Overestimated Pressure Broadening Misleads Model Spectra in Cool M Dwarf Stars
por: Glidden, Ana, et al.
Publicado: (2026)

The rush to the poles and the role of magnetic buoyancy in the solar dynamo
por: Cloutier, Simon, et al.
Publicado: (2024)

Radial velocities of narrow emission line components in the spectra of T Tauri stars
por: Kiryukhina, V. A., et al.
Publicado: (2024)

How well does surface magnetism represent deep Sun-like star dynamo action?
por: Finley, Adam J., et al.
Publicado: (2024)

Behaviors of Ca II K line in A-type stars
por: Takeda, Yoichi
Publicado: (2020)

Dynamical mass determination and partial eclipses of the heartbeat star HD 181793
por: Uronen, Laura E., et al.
Publicado: (2024)

A single frequency approach to nonequilibrium modeling of the chromosphere
por: Ruan, W., et al.
Publicado: (2026)

Influence of departures from LTE on determinations of the sulfur abundances in A-K type stars
por: Korotin, S. A., et al.
Publicado: (2025)

Asymmetry of the spectral lines of the coronal hole and quiet Sun in the transition region
por: Hosseini, Razieh, et al.
Publicado: (2024)