Titlebook: Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates; Observation with the Sei Kato Book 2024 The Editor(s) (if app

formation

書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates影響因子(影響力)




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates影響因子(影響力)學(xué)科排名




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates網(wǎng)絡(luò)公開度




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates被引頻次




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates被引頻次學(xué)科排名




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates年度引用




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates年度引用學(xué)科排名




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates讀者反饋




書目名稱Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates讀者反饋學(xué)科排名

平常

Tibet Air Shower Array and the Muon Detector Array,ray covers a geometrical area of . and captures extensive air showers initiated by primary particles to estimate their incoming directions and energies. The MD array with a geometrical area of . installed underground counts the number of muons contained in air showers and discriminates CR- and gamma

認(rèn)識(shí)

Data Analysis,?to . from the conventional range up?to . in previous studies. The extension improves the photon statistics by . for the sources studied in this work. From a Monte Carlo analysis, the angular and energy resolutions of the experiment for sub-PeV gamma rays are estimated to be . and ., respectively. T

人類

GREG

Demulcent

978-981-97-1645-6The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor

Demulcent

來這真柔軟

表臉

Vertragskosten und Technologie,Search for PeVatrons: Galactic astrophysical accelerators of PeV cosmic rays through the observation of sub-PeV gamma rays (.) is important to understand the origin of the knee of the cosmic-ray energy spectrum observed on the Earth.

易于

Conclusions and Future Prospects,Search for PeVatrons: Galactic astrophysical accelerators of PeV cosmic rays through the observation of sub-PeV gamma rays (.) is important to understand the origin of the knee of the cosmic-ray energy spectrum observed on the Earth.