Simulations of facular magnetic fields on cool stars I: Main sequence stars with solar metallicity

Sensitivity of spectral lines to granulation: from the Sun to K-type stars
by: Vasilyev, V., et al.
Published: (2026)

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

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

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

Self-consistent numerical simulations for the formation and dynamics of solar prominences
by: Zessner, Lisa-Marie, et al.
Published: (2026)

Statistical properties of spicules in MURaM-ChE
by: Chandra, Sanghita, et al.
Published: (2025)

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

Magnetograms underestimate even unipolar magnetic flux nearly everywhere on the solar disk
by: Sinjan, Jonas, et al.
Published: (2024)

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

Probing chromospheric fine structures with a Hα proxy using MURaM-ChE
by: Chandra, Sanghita, et al.
Published: (2025)

Variations in the magnetic field strength of pre-main-sequence stars, solar-type main-sequence stars, and the Sun
by: Yamashita, Mai, et al.
Published: (2025)

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

The effect of stellar magnetic activity on measurements of morning and evening asymmetry of planetary terminator
by: Kostogryz, N., et al.
Published: (2025)

Modeling HMI observables for the study of solar oscillations
by: Fournier, D., et al.
Published: (2025)

Structure and dynamics of the internetwork solar chromosphere: results of a small-scale dynamo simulation
by: Przybylski, D., et al.
Published: (2025)

Sensitivity of spectral lines to granulation: The Sun
by: Sowmya, K., et al.
Published: (2025)

SiO maser polarization and magnetic field in evolved cool stars
by: Marinho, L., et al.
Published: (2024)

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

Surface activity of a Rossby sequence of cool Hyades stars
by: Strassmeier, K. G., et al.
Published: (2025)

Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution
by: Santos, A. R. G., et al.
Published: (2024)

Simulations of structured upflows from plumes and their connection to the solar wind
by: Bora, Kamlesh, et al.
Published: (2025)

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

Phosphorus in cool stars of various metallicities: The non-local thermodynamic equilibrium consideration
by: Andrievsky, S. M., et al.
Published: (2026)

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

Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main sequence stars
by: Bhattacharya, Shatanik, et al.
Published: (2024)

Main sequence dynamo magnetic fields emerging in the white dwarf phase
by: Camisassa, Maria, et al.
Published: (2024)

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

Magnetic reconnection sustains the mass budget of the solar wind
by: Chen, Yajie, et al.
Published: (2025)

eROSITA's cool star population explained
by: Schmitt, J. H. M. M., et al.
Published: (2026)

Signatures of convection in the atmospheres of cool evolved stars
by: Chiavassa, Andrea, et al.
Published: (2024)

Magnetic field generation in mergers of massive main sequence stars
by: Ohlmann, Sebastian T., et al.
Published: (2025)

Convection, rotation, and magnetic activity of solar-like stars from asteroseismology
by: Mathur, Savita
Published: (2024)

Ca ii 854.2 nm in an enhanced network region simulated with MURaM-ChE
by: Ondratschek, P. A., et al.
Published: (2026)

Mg ii h&k spectra of an enhanced network region simulated with the MURaM-ChE code. Results using 1.5D synthesis
by: Ondratschek, P., et al.
Published: (2024)

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

The magnetic fields in Be stars are stronger than previously suggested
by: Hubrig, S., et al.
Published: (2026)