ERD

Topological changes in the magnetic field of LQ Hya during an activity minimum

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Scalable communication for high-order stencil computations using CUDA-aware MPI

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Solar-Cycle Variation of quiet-Sun Magnetism and Surface Gravity Oscillation Mode

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Constraining Global Solar Models through Helioseismic Analysis

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

From convective stellar dynamo simulations to Zeeman-Doppler images

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Numerical evidence for a small-scale dynamo approaching solar magnetic Prandtl numbers

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Socio-economic pandemic modelling: Case of Spain

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

The small-scale dynamo in a multiphase supernova-driven medium

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Computational approaches to modeling dynamos in galaxies

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Compressible test-field method and its application to shear dynamos

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

The role of dynamo instabilities in the dynamics of solar-like cool stars

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Transition from small-scale to large-scale dynamo in a supernova-driven, multiphase medium

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Small-scale dynamos: from idealized models to solar and stellar applications

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Almostfifty years of Metsähovi solar observations on 37 GHz with recovered digitised historical maps

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Exploration of the effects of epidemics on the regional socio-economics: a modelling approach

Project: UniSDyn

Updated at: 15-06-2024

Show more information

Project acronym UniSDyn

Physically motivated heat-conduction treatment in simulations of solar-like stars: effects on dynamo transitions

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

A Knee Point in the Rotation–Activity Scaling of Late-type Stars with a Connection to Dynamo Transitions

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Common dynamo scaling in slowly rotating young and evolved stars

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Shapes of stellar activity cycles

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Stellar coronal X-ray emission and surface magnetic flux

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Generation of mean flows in rotating anisotropic turbulence: The case of solar near-surface shear layer

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Investigating Global Convective Dynamos with Mean-field Models: Full Spectrum of Turbulent Effects Required

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Small-scale Dynamo in Supernova-driven Interstellar Turbulence

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Compressible test-field method and its application to shear dynamos

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

The Pencil Code, a modular MPI code for partial differential equations and particles: multipurpose and multiuser-maintai...

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Spot evolution on LQ Hya from 2006–2017: temperature maps based on SOFIN and FIES data

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

On the Existence of Shear-current Effects in Magnetized Burgulence

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Differences in the solar cycle variability of simple and complex active regions during 1996–2018

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Topological changes in the magnetic field of LQ Hya during an activity minimum

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Stellar X-rays and magnetic activity in 3D MHD coronal models

Project: UniSDyn

Updated at: 27-04-2024

Show more information

Project acronym UniSDyn

Resources

Selected filters:

Topological changes in the magnetic field of LQ Hya during an activity minimum

Scalable communication for high-order stencil computations using CUDA-aware MPI

Solar-Cycle Variation of quiet-Sun Magnetism and Surface Gravity Oscillation Mode

Constraining Global Solar Models through Helioseismic Analysis

From convective stellar dynamo simulations to Zeeman-Doppler images

Numerical evidence for a small-scale dynamo approaching solar magnetic Prandtl numbers

Socio-economic pandemic modelling: Case of Spain

The small-scale dynamo in a multiphase supernova-driven medium

Computational approaches to modeling dynamos in galaxies

Compressible test-field method and its application to shear dynamos

The role of dynamo instabilities in the dynamics of solar-like cool stars

Transition from small-scale to large-scale dynamo in a supernova-driven, multiphase medium

Small-scale dynamos: from idealized models to solar and stellar applications

Almostfifty years of Metsähovi solar observations on 37 GHz with recovered digitised historical maps

Exploration of the effects of epidemics on the regional socio-economics: a modelling approach

Physically motivated heat-conduction treatment in simulations of solar-like stars: effects on dynamo transitions

A Knee Point in the Rotation–Activity Scaling of Late-type Stars with a Connection to Dynamo Transitions

Common dynamo scaling in slowly rotating young and evolved stars

Shapes of stellar activity cycles

Stellar coronal X-ray emission and surface magnetic flux

Generation of mean flows in rotating anisotropic turbulence: The case of solar near-surface shear layer

Investigating Global Convective Dynamos with Mean-field Models: Full Spectrum of Turbulent Effects Required

Small-scale Dynamo in Supernova-driven Interstellar Turbulence

Compressible test-field method and its application to shear dynamos

The Pencil Code, a modular MPI code for partial differential equations and particles: multipurpose and multiuser-maintai...

Spot evolution on LQ Hya from 2006–2017: temperature maps based on SOFIN and FIES data

On the Existence of Shear-current Effects in Magnetized Burgulence

Differences in the solar cycle variability of simple and complex active regions during 1996–2018

Topological changes in the magnetic field of LQ Hya during an activity minimum

Stellar X-rays and magnetic activity in 3D MHD coronal models