activity
20172026
most citedExtending Counter-Streaming Motion from an Active Region Filament to Sunspot Light Bridge

24 citations · 117 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Statistical Analysis of Minifilament Eruptions Using Full-disk H Blue-wing Observations at Big Bear Solar Observatory

Artin Khaleghi, Qin Li, Nengyi Huang +2

This paper presents a comprehensive statistical analysis of minifilament eruptions (MFEs) using high-cadence full-disk H blue-wing observations from Big Bear Solar Observatory.…

astro-ph.SR2025★ 4 cited

Solar Alfvenic Pulses and Mesoscale Solar Wind

Jeongwoo Lee, Manolis K. Georgoulis, Rahul Sharma +3

Large-scale solar ejections are well understood, but the extent to which small-scale solar features directly influence the solar wind remains an open question, primarily due to the…

astro-ph.SR2024

Super-Resolution of SOHO/MDI Magnetograms of Solar Active Regions Using SDO/HMI Data and an Attention-Aided Convolutional Neural Network

Chunhui Xu, Jason T. L. Wang, Haimin Wang +4

Image super-resolution has been an important subject in image processing and recognition. Here, we present an attention-aided convolutional neural network (CNN) for solar image sup…

astro-ph.SR2022★ 9 cited

A Deep Learning Approach to Generating Photospheric Vector Magnetograms of Solar Active Regions for SOHO/MDI Using SDO/HMI and BBSO Data

Haodi Jiang, Qin Li, Zhihang Hu +8

Solar activity is usually caused by the evolution of solar magnetic fields. Magnetic field parameters derived from photospheric vector magnetograms of solar active regions have bee…

astro-ph.SR2022★ 8 cited

Inferring Line-of-Sight Velocities and Doppler Widths from Stokes Profiles of GST/NIRIS Using Stacked Deep Neural Networks

Haodi Jiang, Qin Li, Yan Xu +5

Obtaining high-quality magnetic and velocity fields through Stokes inversion is crucial in solar physics. In this paper, we present a new deep learning method, named Stacked Deep N…

astro-ph.SR2022★ 23 cited

Solar Flare Index Prediction Using SDO/HMI Vector Magnetic Data Products with Statistical and Machine Learning Methods

Hewei Zhang, Qin Li, Yanxing Yang +4

Solar flares, especially the M- and X-class flares, are often associated with coronal mass ejections (CMEs). They are the most important sources of space weather effects, that can…

astro-ph.SR2022★ 16 cited

Predicting Solar Energetic Particles Using SDO/HMI Vector Magnetic Data Products and a Bidirectional LSTM Network

Yasser Abduallah, Vania K. Jordanova, Hao Liu +3

Solar energetic particles (SEPs) are an essential source of space radiation, which are hazards for humans in space, spacecraft, and technology in general. In this paper we propose…

astro-ph.SR2021★ 16 cited

Tracing Halpha Fibrils through Bayesian Deep Learning

Haodi Jiang, Ju Jing, Jiasheng Wang +5

We present a new deep learning method, dubbed FibrilNet, for tracing chromospheric fibrils in Halpha images of solar observations. Our method consists of a data pre-processing comp…

astro-ph.SR2020★ 9 cited

Machine Learning in Heliophysics and Space Weather Forecasting: A White Paper of Findings and Recommendations

Gelu Nita, Manolis Georgoulis, Irina Kitiashvili +38

The authors of this white paper met on 16-17 January 2020 at the New Jersey Institute of Technology, Newark, NJ, for a 2-day workshop that brought together a group of heliophysicis…

astro-ph.SR2017★ 24 cited

Extending Counter-Streaming Motion from an Active Region Filament to Sunspot Light Bridge

Haimin Wang, Rui Liu, Qin Li +6

We analyze the high-resolution observations from the 1.6m telescope at Big Bear Solar Observatory that cover an active region filament. Counter-streaming motions are clearly observ…

astro-ph.SR2017★ 8 cited

High-resolution Observation of Downflows at One End of a Pre-eruption Filament

Qin Li, Na Deng, Ju Jing +1

Studying the dynamics of filaments at pre-eruption phase can shed light on the precursor of eruptive events. Such studies in high-resolution (in the order of 0.1") are highly desir…