activity
20032026
most citedThe origin, early evolution and predictability of solar eruptions

257 citations · 564 across the 13 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

10 papers · 1 filter

astro-ph.SR2026

A multi-source dataset for solar energetic particle forecasting

Yian Yu, Yang Chen, Lulu Zhao +3

Solar energetic particle (SEP) event forecasting often involves integrating heterogeneous observations that differ in cadence, temporal coverage, format, and historical availabilit…

astro-ph.SR2026

Realtime forecasting of solar energetic particle event and proton flux using multi-source solar observations and multi-task deep learning

Yian Yu, Yang Chen, Lulu Zhao +3

Solar energetic particle (SEP) events, defined by proton flux exceeding 10 pfu in the > 10 MeV channel, pose major risks to spacecraft operations, astronaut safety, and high-latitu…

astro-ph.SR2026★ 1 cited

Review of Machine Learning Models for Solar Energetic Particle Prediction

Spiridon Kasapis, Pouya Hosseinzadeh, Kathryn Whitman +73

Solar energetic particle (SEP) events have attracted increasing attention due to their significant radiation hazards for aviation, spacecraft electronics, and human missions beyond…

astro-ph.SR2024

Exploring the Dynamics of CME-Driven Shocks by Comparing Numerical Modeling and Observations

Meng Jin, Gang Li, Nariaki Nitta +9

Shocks driven by coronal mass ejections (CMEs) are primary drivers of gradual solar energetic particle (SEP) events, posing significant risks to space technology and astronauts. Co…

astro-ph.SR2024

Uncovering Heterogeneity of Solar Flare Mechanism With Mixture Models

Bach Viet Do, Yang Chen, XuanLong Nguyen +1

The physics of solar flares occurring on the Sun is highly complex and far from fully understood. However, observations show that solar eruptions are associated with the intense ki…

astro-ph.SR2020★ 20 cited

Thermodynamic Structure of the Solar Corona: Tomographic Reconstructions and MHD Modeling

D. G. Lloveras, A. M. Vásquez, F. A. Nuevo +5

We carry out a study of the global three-dimensional (3D) structure of the electron density and temperature of the quiescent inner solar corona () by means of tomog…

astro-ph.SR2018★ 49 cited

Probing the Puzzle of Behind-the-Limb -ray Flares: Data-driven Simulations of Magnetic Connectivity and CME-driven Shock Evolution

Meng Jin, Vahe Petrosian, Wei Liu +8

Recent detections of high-energy -rays from behind-the-limb (BTL) solar flares by the \emph{Fermi -ray Space Telescope} pose a puzzle and challenge on the particle accelerati…

astro-ph.SR2018★ 257 cited

The origin, early evolution and predictability of solar eruptions

Lucie Green, Tibor Torok, Bojan Vrsnak +2

Coronal mass ejections (CMEs) were discovered in the early 1970s when space-borne coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known that t…

astro-ph.SR2012★ 42 cited

Buildup of Magnetic Shear and Free Energy During Flux Emergence and Cancellation

Fang Fang, Ward Manchester, William P. Abbett +1

We examine a simulation of flux emergence and cancellation, which shows a complex sequence of processes that accumulate free magnetic energy in the solar corona essential for the e…

astro-ph.SR2011★ 33 cited

Dynamic Coupling of Convective Flows and Magnetic Field during Flux Emergence

Fang Fang, Ward Manchester, William P. Abbett +1

We simulate the buoyant rise of a magnetic flux rope from the solar convection zone into the corona to better understand the energetic coupling of the solar interior to the corona.…