Predicting Solar Energetic Particles Using SDO/HMI Vector Magnetic Data Products and a Bidirectional LSTM Network.
Abduallah, Y., Jordanova, V. K., Liu, H.,
Li, Q., Wang, J. T. L., Wang, H.,
ApJS.,
260:16, 2022.
Tracing Hα Fibrils through Bayesian Deep Learning.
Jiang, H., Jing, J., Wang, J., Liu, C., Li, Q., Xu, Y.,
Wang, J. T. L., Wang, H.,
ApJS.,
256:20, 2021.
An Investigation of the Causal Relationship between Sunspot Groups and
Coronal Mass Ejections by Determining Source Active Regions.
Raheem, A., Cavus, H., Coban, G. C., Kinaci, A. C., Wang, H., Wang, J. T. L.,
Monthly Notices of the Royal Astronomical Society, 506(2):1916-1926,
2021.
DeepSun: Machine-Learning-as-a-Service for Solar Flare Prediction.
Abduallah, Y., Wang, J. T. L., Nie, Y., Liu, C., Wang, H.,
Research in Astronomy and Astrophysics,
21:160, 2021.
Machine-learning
Approach to Identification of Coronal Holes in Solar Disk Images and Synoptic
Maps.
Illarionov, E., Kosovichev, A., Tlatov, A., ApJ., 903:115, 2020.
High-resolution
Observations of Small-scale Flux Emergence by GST.
Wang, J., Liu, C., Cao, W., Wang, H., ApJ., 900:84, 2020.
Magnetic
Reconnection during the Post-impulsive Phase of a Long-duration Solar Flare:
Bidirectional Outflows as a Cause of Microwave and X-Ray Bursts.
Yu, S., Chen, B., Reeves, K. K., Gary, D. E., Musset, S., Fleishman, G. D.,
Nita, G. M., Glesener, L., ApJ., 900:17, 2020.
Identifying
and Tracking Solar Magnetic Flux Elements with Deep Learning.
Jiang, H., Wang, J., Liu, C., Jing, J., Liu, H., Wang, J. T. L., Wang, H.,
ApJS., 250:5, 2020.
A New Comprehensive Data Set of
Solar Filaments of 100 yr Interval. I.
Lin, G., Zhu, G., Yang, X., Song, Y., Zhang, M., Liu, S., Wang, X., Su, J.,
Zheng, S., Zhang, J., Tao, D., Zeng, S., Wang, H., Liu, C., Xu, Y., ApJS.,
249:11, 2020.
An Eruptive Circular-ribbon Flare
with Extended Remote Brightenings.
Liu, C., Prasad, A., Lee, J., Wang, H., ApJ., 899:34, 2020.
Comparison
of Enhanced Absorption in He I 10830 A in Observations and Modeling during the
Early Phase of a Solar Flare.
Huang, N., Sadykov, V. M., Xu, Y., Jing, J., Wang, H., ApJL.,
897:L6, 2020.
Measurement of
Magnetic Field and Relativistic Electrons Along a Solar Flare
Current Sheet.
Chen, B., Shen, C., Gary, D. E., Reeves, K. K., Fleishman, G. D., Yu, S., Guo,
F., Krucker, S., Lin, J., Nita, G. M., Kong, X., Nature Astronomy, 2020.
Estimation
of Key Sunquake Parameters through Hydrodynamic Modeling and Cross-correlation
Analysis.
Stefan, J. T., Kosovichev, A. G., ApJ., 895:65, 2020.
Inferring
Vector Magnetic Fields from Stokes Profiles of GST/NIRIS Using a Convolutional
Neural Network.
Liu, H., Xu, Y., Wang, J., Jing, J., Liu, C., Wang, J. T. L., Wang, H., ApJ.,
894:70, 2020.
Evolution
of Flare-accelerated Electrons Quantified by Spatially Resolved
Analysis.
Kuroda, N., Fleishman, G. D., Gary, D. E., Nita, G. M., Chen, B., Yu, S.,
Frontiers in Astronomy and Space Sciences, 7:22, 2020.
Heating
and Eruption of a Solar Circular-ribbon Flare.
Lee, J., Karpen, J. T., Liu, C., Wang, H., ApJ., 893:158, 2020.
Response
of SDO/HMI Observables to Heating of the Solar Atmosphere by
Precipitating High-energy Electrons.
Sadykov, V. M., Kosovichev, A. G., Kitiashvili, I. N., Kerr, G. S., ApJ.,
893:24, 2020.
Predicting
Coronal Mass Ejections Using SDO/HMI Vector Magnetic Data Products and
Recurrent Neural Networks.
Liu, H., Liu, C., Wang, J. T. L., Wang, H., ApJ., 890:12, 2020.
Decay of the
Coronal Magnetic Field Can Release Sufficient Energy to Power a Solar
Flare.
Fleishman, G. D., Gary, D. E., Chen, B., Kuroda, N., Yu, S., Nita, G. M.,
Science, 367(6475):278-280, 2020.
3D
MHD Modeling of the Impact of Subsurface Stratification on the Solar
Dynamo.
Stejko, A. M., Guerrero, G., Kosovichev, A. G., Smolarkiewicz, P. K., ApJ.,
888:16, 2020.
The Eruption of Outer Spine-like Loops Leading to a
Double-stage Circular-ribbon Flare.
Liu, C., Lee, J., Wang, H., ApJ., 883:47, 2019.
High-resolution Observations of Dynamics of
Superpenumbral Hα Fibrils.
Jing, J., Li, Q., Liu, C., Lee, J., Xu, Y., Cao, W., Wang, H., ApJ.,
880:143, 2019.
Spectral
Diagnosis of Mg II and Hα Lines
during the Initial Stage of an M6.5 Solar Flare.
Huang, N., Xu, Y., Sadykov, V. M., Jing, J., Wang, H., ApJ. Letters,
878:L15, 2019.
Predicting
Solar Flares Using a Long Short-term Memory Network.
Liu, H., Liu, C., Wang, J. T. L., Wang, H., ApJ., 877:121, 2019.
