collaborators

5 papers

astro-ph.SR2026

New Statistical Topology Theory Predicts Turbulent Magnetic Emergence from the Sun's Interior

Anda Xiong, Hongyan Li, Shangbin Yang +6

We propose and verify a new statistical topology framework to study the complex magnetic field evolution of Sun-like stars. The Sun, as the star we are most familiar with, exhibits…

astro-ph.SR2026

Distribution of magnetic helicity and energy with height in solar atmosphere

Hongyan Li, Shangbin Yang, Haiqing Xu +3

Magnetic helicity and magnetic energy are key to understanding the solar dynamo and eruptions, and their three-dimensional distributions are of great significance. However, how the…

astro-ph.SR2025

Estimation of gravitational wave from solar emerging magnetic flux tube

Siqi Guan, Shangbin Yang, Xiao Guo

This study investigates the gravitational waves (GWs) generated by the emergence of magnetic flux tubes in the solar convection zone. We focus on the upward buoyancy of magnetic fl…

astro-ph.SR2025

Helicity Fluxes and Hemispheric Helicity Rule of Active Regions Emerging from the Convection Zone Dynamo

V. V. Pipin, Shangbin Yang, A. G. Kosovichev

Using a 3D non-linear mean-field solar dynamo model, we investigate the magnetic helicity flux and magnetic twist, and tilt parameters of bipolar magnetic regions (BMRs) emerging f…

astro-ph.SR2025

Solar Cycle Prediction Using TCN Deep Learning Model with One-Step Pattern

Cui Zhao, Kun Liu, Shangbin Yang +5

Human living environment is influenced by intense solar activity. The solar activity exhibits periodicity and regularity. Although many deep-learning models are currently used for…