supported by the National Natural Science Foundation of China(Nos.42071044,42230720);the Strategic Priority Research Program of the Chinese Academy of Sciences(CAS)(No.XDA23060304);the Youth Innovation Promotion Association CAS(No.2020420).
The cosmic-ray neutron technology is a novel method for upscaling soil moisture,holding significant importance in drought monitoring,soil water storage estimation,calibration of remote sensing products,and data assimi...
The extended-range multi-sphere neutron spectrometer(EBSS)was used to measure the ^(252)Cf neutron spectrum and the cosmic-ray neutron spectrum.It consists of seven polyethylene-only spheres and seven extended-range s...
funded by the Strategic Priority Science and Technology Projects in Space Science of Chinese Academy of Sciences(CAS);supported by the National Natural Science Foundation of China(11921003,11903084,12003076,12022503,12103094,and 12220101003);the Strategic Priority Science and Technology Projects of CAS(XDA15051100);the CAS Project for Young Scientists in Basic Research(YSBR-061);the Youth Innovation Promotion Association of CAS;the Natural Science Foundation of Jiangsu Province(BK20201107);the Program for Innovative Talents and Entrepreneur in Jiangsu;supported by the Swiss National Science Foundation(SNSF),Switzerland;the National Institute for Nuclear Physics(INFN),Italy;the European Research Council(ERC)under the European Unions Horizon 2020 research and innovation programme(851103)。
Boron nuclei in cosmic rays(CRs)are believed to be mainly produced by the fragmentation of heavier nuclei,such as carbon and oxygen,via collisions with the interstellar matter.Therefore,the boron-tocarbon flux ratio(B...
supported in part by the National Natural Science Foundation of China under Grants No. 11875327 and No. 11805288;the Fundamental Research Funds for the Central Universities;the Sun YatSen University Science Foundation;supported by the Program for Innovative Talents and Entrepreneur in Jiangsu。
We attempt to interpret the cosmic-ray positron excess by injection from the nearby pulsar Geminga,assuming a two-zone diffusion scenario and an injection spectrum with a low energy cutoff.Since the high energy positr...
funding was provided by China Sponsorship Council(Grant Number:202004910534).
Purpose The distributions of energy responses of helium measured by the electromagnetic calorimeter(ECAL)of Alpha Magnetic Spectrometer(AMS-02)in Monte-Carlo do not agree with those in real data,thus using energy resp...
Supported in part by the National Natural Science Foundation of China (11620101004,11475093,12127808);the Key Laboratory of Particle&Radiation Imaging(Tsinghua University);the CAS Center for Excellence in Particle Physics (CCEPP);Guangdong Basic and Applied Basic Research Foundation(2019A1515012216);Portion of this work performed at Brookhaven National Laboratory is supported in part by the United States Department of Energy (DESC0012704)。
Solar,terrestrial,and supernova neutrino experiments are subject to muon-induced radioactive background.The China Jinping Underground Laboratory(CJPL),with its unique advantage of a 2400 m rock coverage and long dista...
Supported in part by Guangdong Basic and Applied Basic Research Foundation (2019A1515012216);National Undergraduate Innovation and Entrepreneurship Training Program (20201023);the CAS Center for Excellence in Particle Physics (CCEPP)。
Dark matter(DM)direct detection experiments have been setting strong limits on the DM-nucleon scattering cross section at the DM mass above a few GeV,but leave large parameter spaces unexplored in the low mass region....
Supported by the National Key R&D Program of China(2018YFA0404203);the International Scholarship Program of the MOST of China(G2021166002L);National Natural Science Foundation of China(NSFC)(12147208,U2031103,U1931204);the Science and Technology Department of Sichuan Province(2021YFSY0031)。
In the first part of this Chapter the present state of knowledge from the observations of cosmic rays between 10^(13) and 10^(20) eV is summarized.This is not intended to be a complete review,but rather a broad overvi...
supported by the Outstanding Youth Science Foundation of NSFC(Grant No.12022503);the Joint Funds of the National Natural Science Foundation of China(Grant Nos.U1738208,U1738139,U1738135 and U1738207);the National Natural Science Foundation of China(Grant Nos.11673021,11705197,11773085 and 11851302);the National Key Research and Development Program of China(Grant No.2016YFA0400200);Youth Innovation Promotion Association CAS(Grant No.2021450)。
A method of identifying positron/electron species from the cosmic rays was studied in the DArk Matter Particle Explorer(DAMPE)experiment.As there is no onboard magnet on the satellite,the different features imposed by...
supported by the Ministry of Science and Technology of China Foundation(No.2020YFE0202001);the National Natural Science Foundation of China(No.11875163);the Natural Science Foundation of Hunan Province(No.2021JJ20006).
The muon radiography imaging technique for high-atomic-number objects(Z)and large-volume objects via muon transmission imaging and muon multiple scattering imaging remains a popular topic in the field of radiation det...