Using high-resolution data from the one-meter New Vacuum Solar Telescope, a research team led by Prof. YAN Xiaoli from the Yunnan Observatories of the Chinese Academy of Sciences has conducted an in-depth study on the physical properties and oscillations of chromospheric fibrils surrounding a quiescent filament.
Researchers from the Xinjiang Astronomical Observatory have revealed the link between nulling fraction and emission height by simulating the examination of the correlations between radio pulse nulling fraction, emission height, and their emission geometry, offerring new insight into the inner workings of pulsar magnetospheres.
Researchers from the Xinjiang Astronomical Observatory of the Chinese Academy of Sciences have developed a hybrid deep learning model that can accurately predict how the Earth's atmosphere delays electromagnetic signals, a key source of error in astronomical observations and geodetic measurements.
A research team from the Yunnan Observatories of the Chinese Academy of Sciences has conducted a study on the binary fraction of Blue Horizontal-branch stars. Their findings provide the intrinsic binary fraction and reveal its relationship with metallicity, kinematics, and effective temperature.
A research team led by Prof. YANG Kai from the Institute of Physics of the Chinese Academy of Sciences, along with Prof. FERNÁNDEZ-ROSSIER Joaquín from International Iberian Nanotechnology Laboratory, demonstrated the all-electrical control of quantum interference in individual atomic spins on a surface.
Researchers from the Xinjiang Astronomical Observatory conducted a systematic study of the galactic molecular cloud G34. They revealed the collisional signatures and dynamical mechanisms of filamentary structures in this region.
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