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Numerical Simulations of Flare-productive Active Regions: δ-sunspots, Sheared Polarity Inversion Lines, Energy Storage, and Predictions

The Astrophysical journal, 2017-11, Vol.850 (1), p.39

2017

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A Self-consistent Model of the Solar Tachocline

The Astrophysical journal, 2018-02, Vol.853 (2), p.97

2018

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GLOBAL HELIOSEISMIC EVIDENCE FOR A DEEPLY PENETRATING SOLAR MERIDIONAL FLOW CONSISTING OF MULTIPLE FLOW CELLS

Astrophysical journal. Letters, 2013-12, Vol.778 (2), p.1-7

2013

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TURBULENT PUMPING OF MAGNETIC FLUX REDUCES SOLAR CYCLE MEMORY AND THUS IMPACTS PREDICTABILITY OF THE SUN'S ACTIVITY

Astrophysical journal. Letters, 2012-12, Vol.761 (1), p.1-5

2012

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Solar inertial modes: Observations, identification, and diagnostic promise

Astronomy and astrophysics (Berlin), 2021-08, Vol.652, p.L6

2021

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Time-distance helioseismology of solar Rossby waves

Astronomy and astrophysics (Berlin), 2019-06, Vol.626, p.A3

2019

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MAGNETIC WREATHS AND CYCLES IN CONVECTIVE DYNAMOS

The Astrophysical journal, 2013-01, Vol.762 (2), p.1-20

2013

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Viscous inertial modes on a differentially rotating sphere: Comparison with solar observations

Astronomy and astrophysics (Berlin), 2022-08, Vol.664, p.A6

2022

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Two-step Emergence of the Magnetic Flux Sheet from the Solar Convection Zone

The Astrophysical journal, 2010-05, Vol.714 (1), p.505-516

2010

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Theory of solar oscillations in the inertial frequency range: Amplitudes of equatorial modes from a nonlinear rotating convection simulation

Astronomy and astrophysics (Berlin), 2022-10, Vol.666, p.A135

2022

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Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone

Astronomy and astrophysics (Berlin), 2022-06, Vol.662, p.A16

2022

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Asymptotic g modes: Evidence for a rapid rotation of the solar core

Astronomy and astrophysics (Berlin), 2017-08, Vol.604, p.A40

2017

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Solar meridional circulation from twenty-one years of SOHO/MDI and SDO/HMI observations: Helioseismic travel times and forward modeling in the ray approximation

Astronomy and astrophysics (Berlin), 2018-11, Vol.619, p.A99

2018

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A New Generation of Standard Solar Models

The Astrophysical journal, 2017-02, Vol.835 (2), p.202

2017

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On rising magnetic flux tube and formation of sunspots in a deep domain

Monthly notices of the Royal Astronomical Society, 2020-05, Vol.494 (2), p.2523-2537

2020

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MERIDIONAL CIRCULATION IN SOLAR AND STELLAR CONVECTION ZONES

The Astrophysical journal, 2015-05, Vol.804 (1), p.1-21

2015

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Searching for dark energy with the Sun

Astronomy and astrophysics (Berlin), 2022-11, Vol.667, p.A115

2022

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Searching for g modes

Astronomy and astrophysics (Berlin), 2019, Vol.624

2019

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Evidence of persistence of weak magnetic cycles driven by meridional plasma flows during solar grand minima phases

Monthly notices of the Royal Astronomical Society. Letters, 2022-11, Vol.517 (1), p.L36-L40

2022

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Modelling stellar convective transport with plumes – I. Non-equilibrium turbulence effect in double-averaging formulation

Monthly notices of the Royal Astronomical Society, 2022-09, Vol.516 (2), p.2718-2735

2022

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A Babcock-Leighton dynamo model of the Sun incorporating toroidal flux loss and the helioseismically inferred meridional flow

Astronomy and astrophysics (Berlin), 2023-12, Vol.680, p.A42

2023

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On the hydrostatic stratification of the solar tachocline

Monthly notices of the Royal Astronomical Society, 2018-07, Vol.477 (3), p.3845-3852

2018

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The rotation rate of solar active and ephemeral regions – II. Temporal variations of the rotation rates

Monthly notices of the Royal Astronomical Society, 2023-03, Vol.519 (4), p.5315-5323

2023

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Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun

Astronomy and astrophysics (Berlin), 2023-02, Vol.670, p.A101

2023

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Exploring the reliability of polar field rise rate as a precursor for an early prediction of solar cycle

Monthly notices of the Royal Astronomical Society, 2023-10, Vol.526 (3), p.3994-4003

2023

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Numerical Simulations of Flare-productive Active Regions: δ-sunspots, Sheared Polarity Inversion Lines, Energy Storage, and Predictions

A Self-consistent Model of the Solar Tachocline

GLOBAL HELIOSEISMIC EVIDENCE FOR A DEEPLY PENETRATING SOLAR MERIDIONAL FLOW CONSISTING OF MULTIPLE FLOW CELLS

TURBULENT PUMPING OF MAGNETIC FLUX REDUCES SOLAR CYCLE MEMORY AND THUS IMPACTS PREDICTABILITY OF THE SUN'S ACTIVITY

Solar inertial modes: Observations, identification, and diagnostic promise

Time-distance helioseismology of solar Rossby waves

MAGNETIC WREATHS AND CYCLES IN CONVECTIVE DYNAMOS

Viscous inertial modes on a differentially rotating sphere: Comparison with solar observations

Two-step Emergence of the Magnetic Flux Sheet from the Solar Convection Zone

Theory of solar oscillations in the inertial frequency range: Amplitudes of equatorial modes from a nonlinear rotating convection simulation

Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone

Asymptotic g modes: Evidence for a rapid rotation of the solar core

Solar meridional circulation from twenty-one years of SOHO/MDI and SDO/HMI observations: Helioseismic travel times and forward modeling in the ray approximation

A New Generation of Standard Solar Models

On rising magnetic flux tube and formation of sunspots in a deep domain

MERIDIONAL CIRCULATION IN SOLAR AND STELLAR CONVECTION ZONES

Searching for dark energy with the Sun

Searching for g modes

Evidence of persistence of weak magnetic cycles driven by meridional plasma flows during solar grand minima phases

Modelling stellar convective transport with plumes – I. Non-equilibrium turbulence effect in double-averaging formulation

A Babcock-Leighton dynamo model of the Sun incorporating toroidal flux loss and the helioseismically inferred meridional flow

On the hydrostatic stratification of the solar tachocline

The rotation rate of solar active and ephemeral regions – II. Temporal variations of the rotation rates

Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun

Exploring the reliability of polar field rise rate as a precursor for an early prediction of solar cycle

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