Researchers at IMP have achieved the first precise mass measurements of several exotic atomic nuclei. Using this mass data, they have determined the proton dripline for aluminum, phosphorus, sulfur, and argon elements, and proposed a new approach to uncover proton halo structures.
A research group from the Changchun Institute of Optics, Fine Mechanics and Physics of the Chinese Academy of Sciences developed a novel type of hand-held surgical forceps equipped with a force-holding function. This innovative design aims to improve clamping accuracy while reducing surgeon fatigue during lengthy procedures.
Scientists have constructed the first complete proton energy spectrum observed during an eruptive solar event in the Martian space, deepening our understanding of the radiation environment around Mars. This study provides a reference for future research on similar space weather phenomena, and also highlights the necessity of continuous and coordinated radiation monitoring on Mars.
Recently, a research team led by Professor JIANG Changlong at Hefei Institutes of Physical Science of the Chinese Academy of Sciences, developed a new donor-acceptor (D-A) type fluorescent dye called AFL. This dye changes its fluorescence color and intensity depending on solvent polarity and temperature, making it useful for quick visual monitoring.
Dr. XIANG Nanbin from Yunnan Observatories of the Chinese Academy of Sciences (CAS), in collaboration with Researcher ZHAO Xinhua from State Key Laboratory of Space Weather at National Space Science Center of the CAS, and Professor DENG Linhua from Yunnan Minzu University, has made progress in the study of radial differential rotation of solar corona.
Researchers at Yunnan Observatories of the Chinese Academy of Sciences simulated the evolution of massive stars with masses ranging from 50 to 150 solar masses during the nitrogen sequence Wolf-Rayet (WNL) star phase. They employed a newly developed k−ω model to handle the convective overshooting processes within the stellar interior, offering a more precise understanding of this complex phenomena in massive stars.
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