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•Does a CME Flux Rope "change" its Footpoints to New Location during Eruption? (2019-12-19)
•Researchers Found Indirect Evidence of Broad-line Region of Active Galactic N... (2019-12-17)
•Does the Solar Corona Rotate Faster and Faster during the Past Eight Decades? (2019-12-11)
•NVST and SDO Observations Reveal the Difference Between Sunspot Umbra and Pen... (2019-12-10)
•Researchers Detect a New Type of Orbital Period Variations in Close Binary (2019-11-18)
•Astronomers Obtain the Largest Binary Stars Catalog with Plentiful Parameters (2019-11-18)
•New Sources of Disturbance to the Solar Atmosphere Discovered during Solar St... (2019-11-08)
•Round-Trip Slipping Magnetic Reconnection in a Fan-Spine Jet Observed for the... (2019-11-01)
•Does Kelvin-Helmholtz Instability Heat Plasma in the Solar Atmosphere? (2019-10-21)
•Researchers Modify the Energy-Limited Equation to Estimate the Exoplanetary M... (2019-10-11)
•The Yunnan Observatories' 40-meter Radio Telescope Achieved EVLBI Observation (2019-09-29)
•Researchers Discover Solar Jets Come from the Eruption of Mini-filaments (2019-09-29)
•Supra-arcade Fans May be Region Containing Termination Shocks in Solar Flares? (2019-09-17)
•Researchers Get Distance of the Convective Overshooting Region in Low-mass Stars (2019-09-17)
•Scientists Find Solution to Long-standing "Solar Abundance Problem" (2019-09-05)
•How does One Non-Radial Solar Eruption Produce Two Coronal Mass Ejections on ... (2019-08-22)
•Inner Structure and Evolutionary Status of SPB Star HD 50230 Precisely Determ... (2019-08-20)
•Does the Sun Exhibit Similar Oscillation Behavior on Both Hemispheres? (2019-08-13)
•Researchers Observed How the Solar Filaments "fed" (2019-08-13)
•Witnessing Small-scale Current Sheet Formation in the Solar Atmosphere (2019-07-11)
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