相关期刊:《Meteorological and Environmental Research》《Journal of High Energy Physics, Gravitation and Cosmology》《Journal of Modern Physics》《Natural Science》更多>>
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...
Solar flares, sudden bursts of intense electromagnetic radiation from the Sun, can significantly disrupt technological infrastructure, including communication and navigation satellites. To mitigate these risks, accura...
The automatic detection and analysis of sunspots play a crucial role in understanding solar dynamics and predicting space weather events.This paper proposes a novel method for sunspot group detection and classificatio...
1) The observation by Allais of the precession of pendulums from 1954 to 1960 highlighted regularities of astral origin an in-depth analysis of which showed that, apparently, no classical phenomenon can explain them. ...
supported by the National Natural Science Foundation of China(NSFC,grant No.11973056);the National Key R&D Program of China(grant No.2021YFA1600500)。
Accurate measurement of magnetic fields is very important for understanding the formation and evolution of solar magnetic fields.Currently,there are two types of solar magnetic field measurement instruments:filter-bas...
the support of the National Key Research and Development Program of China(No.2022YFA1604600);the National Natural Science Foundation of China(NSFC,Grant No.11975086)。
Eruption of solar flares is a complex nonlinear process,and the rays and high-energy particles generated by such an eruption are detrimental to the reliability of space-based or ground-based systems.So far,there are n...
the support of the National Key Research and Development Program of China(No.2022YFF0503601);the National Natural Science Foundation of China(No.11975086)。
The research of flare forecast based on the machine learning algorithm is an important content of space science.In order to improve the reliability of the data-driven model and weaken the impact of imbalanced data set...
supported by the International Space Science Institute (ISSI),Bern,Switzerland and ISSI-Beijing,China。
A combined uniform and long-time series of Ca-K images from the Kodaikanal Observatory,Mount Wilson Observatory and Mauna Loa Solar Observatory was used to identify and study the Ca-K small-scale features and their so...
Solar magnetic activity is expressed via variations of sunspots and active regions varying on different timescales. The most accepted is an 11-year period supposedly induced by the electromagnetic solar dynamo mechani...
supported by the National Natural Science Foundation of China(11973084,11873087,12003066 and 11527804);Yunnan Key Laboratory of Solar Physics and Space Science under number 202205AG070009;Yunnan Science Foundation of China under number:202201AT070194;Youth Innovation Promotion Association,CAS(No.2019061);CAS“Light of West China”Program;Yunnan Science Foundation for Distinguished Young Scholars(No.202001AV070004);Key Research and Development Project of Yunnan Province under number 202003AD150019;Young Elite Scientists Sponsorship Program by YNAST.9。
The decay of sunspot plays a key role in magnetic flux transportation in solar active regions(ARs).To better understand the physical mechanism of the entire decay process of a sunspot,an α-configuration sunspot in AR...