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Magnetic Flux of Active Regions Determining the Eruptive Character of Large Solar Flares

The Astrophysical journal, 2020-09, Vol.900 (2), p.128

2020

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Tuning the Exospace Weather Radio for Stellar Coronal Mass Ejections

The Astrophysical journal, 2020-05, Vol.895 (1), p.47

2020

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Evidence for a Coronal Shock Wave Origin for Relativistic Protons Producing Solar Gamma-Rays and Observed by Neutron Monitors at Earth

The Astrophysical journal, 2020-04, Vol.893 (1), p.76

2020

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How Many CMEs Have Flux Ropes? Deciphering the Signatures of Shocks, Flux Ropes, and Prominences in Coronagraph Observations of CMEs

Solar physics, 2013-05, Vol.284 (1), p.179-201

2013

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Simple Model for Temporal Variations of Hα Spectrum by an Eruptive Filament from a Superflare on a Solar-type Star

The Astrophysical journal, 2024-03, Vol.963 (1), p.50

2024

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Solar Coronal Mass Ejections Plasma Diagnostics Expressed as Potential Stellar CME Signatures

The Astronomical journal, 2022-09, Vol.164 (3), p.108

2022

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Sun-as-a-star Analyses of Various Solar Active Events Using Hα Spectral Images Taken by SMART/SDDI

The Astrophysical journal, 2022-11, Vol.939 (2), p.98

2022

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Solar–Stellar Connection: X-Ray Flares to Energetic (E > 10 MeV) Particle Events

The Astrophysical journal, 2023-10, Vol.956 (1), p.24

2023

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The Common Origin of High-energy Protons in Solar Energetic Particle Events and Sustained Gamma-Ray Emission from the Sun

The Astrophysical journal, 2021-07, Vol.915 (2), p.82

2021

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Solar Longitude Distribution of High-energy Proton Flares: Fluences and Spectra

Astrophysical journal. Letters, 2020-09, Vol.900 (1), p.L11

2020

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Coronal Mass Ejections and Non-recurrent Forbush Decreases

Solar physics, 2014-10, Vol.289 (10), p.3949-3960

2014

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Peak Temperatures of Large Solar X-Ray Flares and Associated CME Speeds and Widths

The Astrophysical journal, 2020-03, Vol.891 (1), p.54

2020

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Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review)

Solar physics, 2014-09, Vol.289 (9), p.3233-3277

2014

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PROPAGATION OF THE 2014 JANUARY 7 CME AND RESULTING GEOMAGNETIC NON-EVENT

The Astrophysical journal, 2015-10, Vol.812 (2), p.145

2015

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Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum

Solar physics, 2014-10, Vol.289 (10), p.3773-3797

2014

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Catalog of Geomagnetic Storms with Dst Index ≤ −50 nT and Their Solar and Interplanetary Origin (1996–2019)

Atmosphere, 2023-12, Vol.14 (12), p.1744

2023

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The Solar Connection of Enhanced Heavy Ion Charge States in the Interplanetary Medium: Implications for the Flux-Rope Structure of CMEs

Solar physics, 2013-05, Vol.284 (1), p.17-46

2013

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Simultaneous Observation of a Flux Rope Eruption and Magnetic Reconnection during an X-class Solar Flare

Astrophysical journal. Letters, 2018-01, Vol.853 (1), p.L18

2018

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Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. I. Reconciliation of “EIT Waves”, Type II Radio Bursts, and Leading Edges of CMEs

Solar physics, 2011-11, Vol.273 (2), p.433-460

2011

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The Physical Processes of CME/ICME Evolution

Space science reviews, 2017-11, Vol.212 (3-4), p.1159-1219

2017

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Successive X-class Flares and Coronal Mass Ejections Driven by Shearing Motion and Sunspot Rotation in Active Region NOAA 12673

The Astrophysical journal, 2018-03, Vol.856 (1), p.79

2018

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WHY IS THE GREAT SOLAR ACTIVE REGION 12192 FLARE-RICH BUT CME-POOR?

Astrophysical journal. Letters, 2015-05, Vol.804 (2), p.1-6

2015

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Statistical Study of GOES X-Ray Quasi-periodic Pulsations in Solar Flares

The Astrophysical journal, 2020-05, Vol.895 (1), p.50

2020

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DIRECT EVIDENCE FOR A FAST CORONAL MASS EJECTION DRIVEN BY THE PRIOR FORMATION AND SUBSEQUENT DESTABILIZATION OF A MAGNETIC FLUX ROPE

The Astrophysical journal, 2013-02, Vol.764 (2), p.1-13

2013

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How Does Magnetic Reconnection Drive the Early-stage Evolution of Coronal Mass Ejections?

The Astrophysical journal, 2020-04, Vol.893 (2), p.141

2020

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Magnetic Flux of Active Regions Determining the Eruptive Character of Large Solar Flares

Tuning the Exospace Weather Radio for Stellar Coronal Mass Ejections

Evidence for a Coronal Shock Wave Origin for Relativistic Protons Producing Solar Gamma-Rays and Observed by Neutron Monitors at Earth

How Many CMEs Have Flux Ropes? Deciphering the Signatures of Shocks, Flux Ropes, and Prominences in Coronagraph Observations of CMEs

Simple Model for Temporal Variations of Hα Spectrum by an Eruptive Filament from a Superflare on a Solar-type Star

Solar Coronal Mass Ejections Plasma Diagnostics Expressed as Potential Stellar CME Signatures

Sun-as-a-star Analyses of Various Solar Active Events Using Hα Spectral Images Taken by SMART/SDDI

Solar–Stellar Connection: X-Ray Flares to Energetic (E > 10 MeV) Particle Events

The Common Origin of High-energy Protons in Solar Energetic Particle Events and Sustained Gamma-Ray Emission from the Sun

Solar Longitude Distribution of High-energy Proton Flares: Fluences and Spectra

Coronal Mass Ejections and Non-recurrent Forbush Decreases

Peak Temperatures of Large Solar X-Ray Flares and Associated CME Speeds and Widths

Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review)

PROPAGATION OF THE 2014 JANUARY 7 CME AND RESULTING GEOMAGNETIC NON-EVENT

Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum

Catalog of Geomagnetic Storms with Dst Index ≤ −50 nT and Their Solar and Interplanetary Origin (1996–2019)

The Solar Connection of Enhanced Heavy Ion Charge States in the Interplanetary Medium: Implications for the Flux-Rope Structure of CMEs

Simultaneous Observation of a Flux Rope Eruption and Magnetic Reconnection during an X-class Solar Flare

Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. I. Reconciliation of “EIT Waves”, Type II Radio Bursts, and Leading Edges of CMEs

The Physical Processes of CME/ICME Evolution

Successive X-class Flares and Coronal Mass Ejections Driven by Shearing Motion and Sunspot Rotation in Active Region NOAA 12673

WHY IS THE GREAT SOLAR ACTIVE REGION 12192 FLARE-RICH BUT CME-POOR?

Statistical Study of GOES X-Ray Quasi-periodic Pulsations in Solar Flares

DIRECT EVIDENCE FOR A FAST CORONAL MASS EJECTION DRIVEN BY THE PRIOR FORMATION AND SUBSEQUENT DESTABILIZATION OF A MAGNETIC FLUX ROPE

How Does Magnetic Reconnection Drive the Early-stage Evolution of Coronal Mass Ejections?

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