supported by the National Key Research and Development Program of China(2023YFD1200105);the National Natural Science Foundation of China(31972446);the 5·5 Engineering Research&Innovation Team Project of Beijing Forestry University,China(BLRC2023A06)。
Tree peony is an emerging woody oilseed crop that has the potential to help meet the growing demand for edible oil and biofuel,and breeding high-yield varieties is the key to increasing production.The DA1 gene regulat...
supported in China by NSFC grant No.12393853;the Department of Science and Technology of Sichuan Province China with grant No.24NSFSC0449;NSFC grant No.U2031205。
With its high duty cycle, wide field of view and high detection sensitivity, Water Chereknov Detector Array as one of sub-arrays of Large High Altitude Air Shower Observatory is a promising facility to monitor transie...
gratefully acknowledge the financial support from the Scientific and Technological Innovation 2030-“New Generation Artificial Intelligence”Major Project(2021ZD0112301);National Natural Science Foundation of China(62273011,62076013,62303027).
Steam-assisted combustion elevated flares are currently the most widely used type of petrochemical flares.Due to the complex and variable composition of the waste gas they handle,the combustion environment is severely...
The time series of daily data on solar activity proxies, namely the sunspot number(SSN), sunspot area(SSA), solar radio flux(F10.7), modified coronal index(MCI), solar flare index(FI), and cosmic ray intensity(CRI), w...
supported by the National Natural Science Foundation of China (NSFC 42174200);Shenzhen Science and Technology Program (grant No. RCJC20210609 104422048);Shenzhen Key Laboratory Launching Project (No. ZDSYS20210702140800001);Guangdong Basic and Applied Basic Research Foundation (2023B1515040021);the Fundamental Research Funds for the Central Universities (grant No. HIT.OCEF.2023047)。
The solar coronal magnetic field is a pivotal element in the study of eruptive phenomena, and understanding its dynamic evolution has long been a focal point in solar physics. Numerical models, driven directly by obse...
partially supported by the National Natural Science Foundation of China (NSFC, grant Nos. 12433004, U2031201, and 11733001);Guangdong Major Project of Basic and Applied Basic Research (grant No. 2019B030302001);the science research grants from the China Manned Space Project with No. CMS-CSST-2021-A06;the support for Astrophysics Key Subjects of Guangdong Province and Guangzhou City;The Key Laboratory for Astronomical Observation and Technology of Guangzhou also supports the work。
A Very High-energy(VHE) flare was observed by Major Atmospheric Gamma Imaging Cherenkov Telescopes on MJD 57788. This VHE flare was characterized by increased VHE flux and short timescales. In this study, we used one-...
funded by the National Natural Science Foundation of China (NSFC) under Nos. 41074132, 41274193, 41474166, and 41774085;the Special Fund of the Institute of Geophysics, China Earthquake Administration (Grant No. DQJB22X12)。
We studied the latitudinal and solar cycle distribution of extreme(≥X5) solar flares spanning 1976–2018. We found that all such flares were confined within the latitudinal range of [S30, N35]. Nonetheless, the major...
supported by the National Natural Science Foundation of China(NSFC)U2031108;Yunnan Key Laboratory of Solar Physics and Space Science under the number YNSPCC202213。
Solar active regions(ARs)are formed by the emergence of current-carrying magnetic flux tubes from below the photosphere.Although for an isolated flux tube the direct and return currents flowing along the tube should b...
supported by the National Key R&D Program of the Ministry of Science and Technology (2022YFC2304303)。
Flare and multiple recurrences pose significant challenges in gouty arthritis.Traditional treatments provide temporary relief from inflammation but fail to promptly alleviate patient pain or effectively prevent subseq...
supported by the National Key R&D Program of China 2021YFA1600502(Grant No.2021YFA1600500);the National Natural Science Foundation of China(Grant Nos.11973092,12073081,12003064;12333009);supported by the Surface Project of Jiangsu Province(Grant No.BK20211402);Yunnan Key Laboratory of Solar Physics and Space Science(202205AG070009)(Grant No.YNSPCC202207);a collaborative project conducted by the National Astronomical Observatories of CAS,Peking University,Tongji University,Xi’an Institute of Optics and Precision Mechanics of CAS and the Innovation Academy for Microsatellites of CAS;supported by the China National Space Administration(CNSA)。
Kink oscillations,which are frequently observed in coronal loops and prominences,are often accompanied by extreme-ultraviolet(EUV)waves.However,much more needs to be explored regarding the causal relationships between...