Lista de obras - Yang Guo - Dominio Público Uruguay

3D Magnetic Field Configuration of the 2006 December 13 Flare Extrapolated with the Optimization Method ⬇️

scientific article published in the Astrophysical Journal

A circular white-light flare with impulsive and gradual white-light kernels

artículo científico publicado en 2017

A comparative study of confined and eruptive flares in NOAA AR 10720 ⬇️

scientific article published in the Astrophysical Journal

An Observationally Constrained Model of a Flux Rope that Formed in the Solar Corona ⬇️

article by Alexander W. James et al published 7 March 2018 in Letters of the Astrophysical Journal

Chain reconnections observed in sympathetic eruptions ⬇️

artículo científico publicado en 2016

Coexisting flux rope and dipped arcade sections along one solar filament ⬇️

artículo científico publicado en 2010

Data-driven Modeling of a Coronal Magnetic Flux Rope: From Birth to Death

artículo científico publicado en 2024

Driving mechanism and onset condition of a confined eruption ⬇️

scholarly article

Dynamic evolution of an X-shaped structure above a trans-equatorial quadrupole solar active region group ⬇️

scholarly article

Evolution of hard X-ray sources and ultraviolet solar flare ribbons for a confined eruption of a magnetic flux rope ⬇️

artículo científico publicado en 2012

Explosive chromospheric evaporation in a circular-ribbon flare ⬇️

artículo científico publicado en 2016

Flare energy build-up in a decaying active region near a coronal hole ⬇️

artículo científico publicado en 2009

Formation heights of extreme ultraviolet lines in an active region derived by correlation of Doppler velocity and magnetic field ⬇️

scientific article published in the Astrophysical Journal

Formation of a double-decker magnetic flux rope in the sigmoidal solar active region 11520 ⬇️

artículo científico publicado en 2014

Homologous Circular-ribbon Flares Driven by Twisted Flux Emergence

artículo científico publicado en 2017

Investigating two successive flux rope eruptions in a solar active region ⬇️

artículo científico publicado en 2013

Investigation of the moving structures in a coronal bright point ⬇️

scientific article published in the Astrophysical Journal

Magnetic Field Structures in a Facular Region Observed by THEMIS and Hinode

Magnetic Helicity Estimations in Models and Observations of the Solar Magnetic Field. III. Twist Number Method

scientific article published in the Astrophysical Journal

Magneto-frictional modeling of coronal nonlinear force-free fields. I. Testing with analytic solutions ⬇️

artículo científico publicado en 2016

Magneto-frictional modeling of coronal nonlinear force-free fields. II. Application to observations ⬇️

artículo científico publicado en 2016

Magnetohydrodynamic seismology of a coronal loop system by the first two modes of standing kink waves ⬇️

artículo científico publicado en 2015

Modeling magnetic field structure of a solar active region Corona using nonlinear force-free fields in spherical geometry ⬇️

scientific article published in the Astrophysical Journal

Nonlinear damping of Alfven waves in the solar Corona below 1.5 solar radii ⬇️

artículo científico publicado en 2015

Observationally quantified reconnection providing a viable mechanism for active region coronal heating.

artículo científico publicado en 2018

On the 2012 October 23 circular ribbon flare: emission features and magnetic topology ⬇️

artículo científico publicado en 2015

On the nature of the extreme-ultraviolet late phase of solar flares ⬇️

artículo científico publicado en 2014

On the relationship between a hot-channel-like solar magnetic flux rope and its embedded prominence ⬇️

scholarly article

Production of the extreme-ultraviolet late phase of an X class flare in a three-stage magnetic reconnection process ⬇️

scholarly article

Quantifying the topology and evolution of a magnetic flux rope associated with multi-flare activities ⬇️

artículo científico publicado en 2016

Rapid Buildup of a Magnetic Flux Rope during a Confined X2.2 Class Flare in NOAA AR 12673 ⬇️

Re-flaring of a post-flare loop system driven by flux rope emergence and twisting ⬇️

scholarly article

Recurrent coronal jets induced by repetitively accumulated electric currents

scientific article published in Astronomy and Astrophysics

Rotation and Confined Eruption of a Double Flux-rope System

artículo científico publicado en 2024

Slow patchy extreme-ultraviolet propagating fronts associated with fast coronal magneto-acoustic waves in solar eruptions

scholarly article

Solar Magnetic Flux Rope Eruption Simulated by a Data-driven Magnetohydrodynamic Model ⬇️

Temporal evolution of the magnetic topology of the NOAA active region 11158 ⬇️

artículo científico publicado en 2014

Three-dimensional Velocity Fields of the Solar Filament Eruptions Detected by CHASE

scholarly article

Three-dimensional prominence-hosting magnetic configurations: creating a helical magnetic flux rope ⬇️

artículo científico publicado en 2013

Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events

Tracking the evolution of a coherent magnetic flux rope continuously from the inner to the outer Corona ⬇️

artículo científico publicado en 2013

Twist accumulation and topology structure of a solar magnetic flux rope ⬇️

artículo científico publicado en 2013

Twisting solar coronal jet launched at the boundary of an active region

artículo científico publicado en 2013

Two types of magnetic reconnection in coronal bright points and the corresponding magnetic configuration ⬇️

scientific article published in the Astrophysical Journal

Understanding the white-light flare on 2012 March 9: evidence of a two-step magnetic reconnection

artículo científico publicado en 2012

Where do flare ribbons stop?

article by PengFei Chen et al published 9 November 2011 in Science Bulletin

Lista de obras de Yang Guo

3D Magnetic Field Configuration of the 2006 December 13 Flare Extrapolated with the Optimization Method ⬇️

A circular white-light flare with impulsive and gradual white-light kernels

A comparative study of confined and eruptive flares in NOAA AR 10720 ⬇️

An Observationally Constrained Model of a Flux Rope that Formed in the Solar Corona ⬇️

Chain reconnections observed in sympathetic eruptions ⬇️

Coexisting flux rope and dipped arcade sections along one solar filament ⬇️

Data-driven Modeling of a Coronal Magnetic Flux Rope: From Birth to Death

Driving mechanism and onset condition of a confined eruption ⬇️

Dynamic evolution of an X-shaped structure above a trans-equatorial quadrupole solar active region group ⬇️

Evolution of hard X-ray sources and ultraviolet solar flare ribbons for a confined eruption of a magnetic flux rope ⬇️

Explosive chromospheric evaporation in a circular-ribbon flare ⬇️

Flare energy build-up in a decaying active region near a coronal hole ⬇️

Formation heights of extreme ultraviolet lines in an active region derived by correlation of Doppler velocity and magnetic field ⬇️

Formation of a double-decker magnetic flux rope in the sigmoidal solar active region 11520 ⬇️

Homologous Circular-ribbon Flares Driven by Twisted Flux Emergence

Investigating two successive flux rope eruptions in a solar active region ⬇️

Investigation of the moving structures in a coronal bright point ⬇️

Magnetic Field Structures in a Facular Region Observed by THEMIS and Hinode

Magnetic Helicity Estimations in Models and Observations of the Solar Magnetic Field. III. Twist Number Method

Magneto-frictional modeling of coronal nonlinear force-free fields. I. Testing with analytic solutions ⬇️

Magneto-frictional modeling of coronal nonlinear force-free fields. II. Application to observations ⬇️

Magnetohydrodynamic seismology of a coronal loop system by the first two modes of standing kink waves ⬇️

Modeling magnetic field structure of a solar active region Corona using nonlinear force-free fields in spherical geometry ⬇️

Nonlinear damping of Alfven waves in the solar Corona below 1.5 solar radii ⬇️

Observationally quantified reconnection providing a viable mechanism for active region coronal heating.

On the 2012 October 23 circular ribbon flare: emission features and magnetic topology ⬇️

On the nature of the extreme-ultraviolet late phase of solar flares ⬇️

On the relationship between a hot-channel-like solar magnetic flux rope and its embedded prominence ⬇️

Production of the extreme-ultraviolet late phase of an X class flare in a three-stage magnetic reconnection process ⬇️

Quantifying the topology and evolution of a magnetic flux rope associated with multi-flare activities ⬇️

Rapid Buildup of a Magnetic Flux Rope during a Confined X2.2 Class Flare in NOAA AR 12673 ⬇️

Re-flaring of a post-flare loop system driven by flux rope emergence and twisting ⬇️

Recurrent coronal jets induced by repetitively accumulated electric currents

Rotation and Confined Eruption of a Double Flux-rope System

Slow patchy extreme-ultraviolet propagating fronts associated with fast coronal magneto-acoustic waves in solar eruptions

Solar Magnetic Flux Rope Eruption Simulated by a Data-driven Magnetohydrodynamic Model ⬇️

Temporal evolution of the magnetic topology of the NOAA active region 11158 ⬇️

Three-dimensional Velocity Fields of the Solar Filament Eruptions Detected by CHASE

Three-dimensional prominence-hosting magnetic configurations: creating a helical magnetic flux rope ⬇️

Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events

Tracking the evolution of a coherent magnetic flux rope continuously from the inner to the outer Corona ⬇️

Twist accumulation and topology structure of a solar magnetic flux rope ⬇️

Twisting solar coronal jet launched at the boundary of an active region

Two types of magnetic reconnection in coronal bright points and the corresponding magnetic configuration ⬇️

Understanding the white-light flare on 2012 March 9: evidence of a two-step magnetic reconnection

Where do flare ribbons stop?

Why are halo coronal mass ejections faster?