汪景琇：
1. Wang,J., Shi,Z., Flare-associated magnetic changes in an active region Ⅱ. Flux emergence and cancellation, Solar Phys., 143(1993), 119-139.
2. Wang,J., Wang,H., Tang,F., Lee,J.W., and Zirin,H. Flux distribution of solar intranetwork magnetic fields, Solar Phys., 160(1995), 277-288.
3. Wang,J., Shi,Z., Wang,H., and Lu,Y., Flares and the magnetic nonpotentiality, Ap.J., 456(1996)，861-878.
4. Wang,J, Li,W., Lee,C.Y., Wang,H., Goode,P.R., McAllister,A., Martin,S.F., Minifilament eruption on the quiet Sun, I. Observations at the H-alpha central line, Ap.J., 530(2000), 1071-1084.
5. Wang, JingXiu; Zhang, YuZong; He, Han; Chen, AnQin; Jin, ChunLan; Zhou, GuiPing 2015, Cluster of solar active regions and onset of coronal mass ejections，SCPMA, 58, 5682-5689（已读）
周桂萍：
1、An observational overview of solar flares
2、Solar prominences: observations
3、Extreme solar events
4、Solar coronal magnetic field measurements using spectral lines available in Hinode/EIS observations: Strong and weak field techniques and temperature diagnostics
5、Slow wind belt in the quiet solar corona
杨书红：
1. Quiet Sun magnetic fields: an observational view
https://ui.adsabs.harvard.edu/abs/2019LRSP...16....1B/abstract
2. Photospheric flux cancellation and associated flux rope formation and eruption
https://ui.adsabs.harvard.edu/abs/2011A%26A...526A...2G/abstract
3. Electric Currents in Flare Ribbons: Observations and Three-dimensional Standard Model（已读）
https://ui.adsabs.harvard.edu/abs/2014ApJ...788...60J/abstract
4. Generation of solar spicules and subsequent atmospheric heating
https://ui.adsabs.harvard.edu/abs/2019Sci...366..890S/abstract
5. Flare-productive active regions
https://ui.adsabs.harvard.edu/abs/2019LRSP...16....3T/abstract
李婷：
1、MAGNETIC PROPERTIES OF SOLAR ACTIVE REGIONS THAT GOVERN LARGE SOLAR FLARES AND ERUPTIONS（已读）
https://ui.adsabs.harvard.edu/abs/2017ApJ...834...56T/abstract
2、PLASMOID EJECTIONS AND LOOP CONTRACTIONS IN AN ERUPTIVE M7.7 SOLAR FLARE: EVIDENCE OF PARTICLE ACCELERATION AND HEATING IN MAGNETIC RECONNECTION OUTFLOWS
https://ui.adsabs.harvard.edu/abs/2013ApJ...767..168L/abstract
3、Small-scale filament eruptions as the driver of X-ray jets in solar coronal holes
https://ui.adsabs.harvard.edu/abs/2015Natur.523..437S/abstract
4、Observation of an evolving magnetic flux rope before and during a solar eruption
https://ui.adsabs.harvard.edu/abs/2012NatCo...3..747Z/abstract
5、WHY IS THE GREAT SOLAR ACTIVE REGION 12192 FLARE-RICH BUT CME-POOR?
https://ui.adsabs.harvard.edu/abs/2015ApJ...804L..28S/abstract
李乐平：
1、Multi-Scale Variability of Coronal Loops Set by Thermal Non-Equilibrium and Instability as a Probe for Coronal Heating
https://ui.adsabs.harvard.edu/abs/2022FrASS...920116A/abstract
2、 Origin and Structures of Solar Eruptions I: Magnetic Flux Rope
https://ui.adsabs.harvard.edu/abs/2017ScChD..60.1383C/abstract
3、Physics of Solar Prominences: II—Magnetic Structure and Dynamics
https://ui.adsabs.harvard.edu/abs/2010SSRv..151..333M/abstract
4、Coronal Mass Ejections: Models and Their Observational Basis
https://ui.adsabs.harvard.edu/abs/2011LRSP....8....1C/abstract
5、Chirality and Magnetic Configurations of Solar Filaments
https://ui.adsabs.harvard.edu/abs/2017ApJ...835...94O/abstract
金春兰：
1、Microflares and nanoflares in the solar corona
https://ui.adsabs.harvard.edu/abs/2020PhyU...63..783B/abstract
2、On the Magnetic Nature of an Exploding Granule as Revealed by Sunrise/IMaX
https://ui.adsabs.harvard.edu/abs/2020ApJ...896...62G/abstract
3、A journey of exploration to the polar regions of a star: probing the solar poles and the heliosphere from high helio-latitude
https://ui.adsabs.harvard.edu/abs/2021ExA...tmp...93H/abstract
4、High-resolution observations of flare precursors in the low solar atmosphere（已读）
https://ui.adsabs.harvard.edu/abs/2017NatAs...1E..85W/abstract
5、Stellar activity and coronal heating: an overview of recent results（已读）
https://ui.adsabs.harvard.edu/abs/2015RSPTA.37340259T/abstract
张宇宗：
1、Space Weather: The Solar Perspective
https://ui.adsabs.harvard.edu/abs/2006LRSP....3....2S
2、Space Weather: Terrestrial Perspective
https://ui.adsabs.harvard.edu/abs/2007LRSP....4....1P
3、The 1859 space weather event revisited: limits of extreme activity
https://ui.adsabs.harvard.edu/abs/2013JSWSC...3A..31C
4、Fair space weather for solar cycle 24（已读）
https://ui.adsabs.harvard.edu/abs/2005GeoRL..3221106S
5、Extreme Space Weather Events: From Cradle to Grave
https://ui.adsabs.harvard.edu/abs/2018SSRv..214...21R
侯义军：
1、Are IRIS Bombs Connected to Ellerman Bombs?
https://ui.adsabs.harvard.edu/abs/2016ApJ...824...96T/abstract
2、Light Bridge in a Developing Active Region. I. Observation of Light Bridge and its Dynamic Activity Phenomena
https://ui.adsabs.harvard.edu/abs/2015ApJ...811..137T/abstract
3、A Model for Magnetically Coupled Sympathetic Eruptions
https://ui.adsabs.harvard.edu/abs/2011ApJ...739L..63T/abstract
4、Some interesting topics provoked by the solar filament research in the past decade
https://ui.adsabs.harvard.edu/abs/2020RAA....20..166C/abstract
5、Persistent Horizontal Flows and Magnetic Support of Vertical Threads in a Quiescent Prominence
https://ui.adsabs.harvard.edu/abs/2008ApJ...689L..73C/abstract
6、Velocity vectors of a quiescent prominence observed by Hinode/SOT and the MSDP (Meudon)
https://ui.adsabs.harvard.edu/abs/2010A%26A...514A..68S/abstract
7、A White-light Flare Powered by Magnetic Reconnection in the Lower Solar Atmosphere（已读）
https://ui.adsabs.harvard.edu/abs/2020ApJ...893L..13S/abstract
8、Superflares on solar-type stars（已读）
https://ui.adsabs.harvard.edu/abs/2012Natur.485..478M/abstract
9、Statistical Studies of Solar White-light Flares and Comparisons with Superflares on Solar-type Stars
https://ui.adsabs.harvard.edu/abs/2017ApJ...851...91N/abstract
10、New Evidence that Magnetoconvection Drives Solar–Stellar Coronal Heating
https://ui.adsabs.harvard.edu/abs/2017ApJ...843L..20T/abstract
雷亚娟：
1、Stellar evolution of low and intermediate-mass stars. I. Mass loss on the AGB and its consequences for stellar evolution.
2、Stellar evolution of low- and intermediate-mass stars. II. Post-AGB evolution.
3、Stellar evolution of low and intermediate-mass stars III. An application of evolutionary post-AGB models: the variable central star FG Sagitta
4、Stellar evolution of low and intermediate-mass stars. IV. Hydrodynamically-based overshoot and nucleosynthesis in AGB stars.
5、Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 Msun, and from Z=0.0004 to 0.03
