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Formation of the largest galactic cores through binary scouring and gravitational wave recoil

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Does magnetic field impact tidal dynamics inside the convective zone of low-mass stars along their evolution?

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Application and interpretation of deep learning for identifying pre-emergence magnetic field patterns

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Validation of a wave heated 3D MHD coronal-wind model using Polarized Brightness and EUV observations

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Determining the source and eruption dynamics of a stealth CME using NLFFF modelling and MHD simulations

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Dynamical coupling of a mean-field dynamo and its wind: Feedback loop over a stellar activity cycle

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Ambipolar diffusion: Self-similar solutions and MHD code testing

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

The angular-momentum flux in the solar wind observed during Solar Orbiter’s first orbit

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Impact of spatially correlated fluctuations in sunspots on metrics related to magnetic twist

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Toroidal Flux Loss due to Flux Emergence Explains why Solar Cycles Rise Differently but Decay in a Similar Way

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Identifying solar-like magnetic cycles with Zeeman-Doppler-Imaging

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

A New Space Weather Tool for Identifying Eruptive Active Regions

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Rossby and Magnetic Prandtl Number Scaling of Stellar Dynamos

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Signature of solar g modes in first-order p-mode frequency shifts

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Large-amplitude Prominence Oscillations following Impact by a Coronal Jet

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Alfvén-wave-driven Magnetic Rotator Winds from Low-mass Stars. I. Rotation Dependences of Magnetic Braking and Mass-los...

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Predicting frequency changes of global-scale solar Rossby modes due to solar cycle changes in internal rotation

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

From stellar coronae to gyrochronology: A theoretical and observational exploration

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Efficient and Accurate Algorithm for the Full Modal Green's Kernel of the Scalar Wave Equation in Helioseismology

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Solar east-west flow correlations that persist for months at low latitudes are dominated by active region inflows

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Radiative transfer with opacity distribution functions: Application to narrowband filters

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Simulating the Coronal Evolution of Bipolar Active Regions to Investigate the Formation of Flux Ropes

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Can Multi-threaded Flux Tubes in Coronal Arcades Support a Magnetohydrodynamic Avalanche?

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Understanding convection-driven coronal heating in the quiet Sun

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

Temporal evolution of oscillating coronal loops

Project: WHOLE SUN

Updated at: 27-04-2024

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Project acronym WHOLE SUN

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Formation of the largest galactic cores through binary scouring and gravitational wave recoil

Does magnetic field impact tidal dynamics inside the convective zone of low-mass stars along their evolution?

Application and interpretation of deep learning for identifying pre-emergence magnetic field patterns

Validation of a wave heated 3D MHD coronal-wind model using Polarized Brightness and EUV observations

Determining the source and eruption dynamics of a stealth CME using NLFFF modelling and MHD simulations

Dynamical coupling of a mean-field dynamo and its wind: Feedback loop over a stellar activity cycle

Ambipolar diffusion: Self-similar solutions and MHD code testing

The angular-momentum flux in the solar wind observed during Solar Orbiter’s first orbit

Impact of spatially correlated fluctuations in sunspots on metrics related to magnetic twist

Toroidal Flux Loss due to Flux Emergence Explains why Solar Cycles Rise Differently but Decay in a Similar Way

Identifying solar-like magnetic cycles with Zeeman-Doppler-Imaging

A New Space Weather Tool for Identifying Eruptive Active Regions

Rossby and Magnetic Prandtl Number Scaling of Stellar Dynamos

Signature of solar g modes in first-order p-mode frequency shifts

Large-amplitude Prominence Oscillations following Impact by a Coronal Jet

Alfvén-wave-driven Magnetic Rotator Winds from Low-mass Stars. I. Rotation Dependences of Magnetic Braking and Mass-los...

Predicting frequency changes of global-scale solar Rossby modes due to solar cycle changes in internal rotation

From stellar coronae to gyrochronology: A theoretical and observational exploration

Efficient and Accurate Algorithm for the Full Modal Green's Kernel of the Scalar Wave Equation in Helioseismology

Solar east-west flow correlations that persist for months at low latitudes are dominated by active region inflows

Radiative transfer with opacity distribution functions: Application to narrowband filters

Simulating the Coronal Evolution of Bipolar Active Regions to Investigate the Formation of Flux Ropes

Can Multi-threaded Flux Tubes in Coronal Arcades Support a Magnetohydrodynamic Avalanche?

Understanding convection-driven coronal heating in the quiet Sun

Temporal evolution of oscillating coronal loops