formation
发表于 2025-3-21 19:19:17
书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0380607<br><br> <br><br>书目名称Gamma Rays in the 100 TeV Region from Potential Galactic PeVatron Candidates读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0380607<br><br> <br><br>
平常
发表于 2025-3-21 23:03:56
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
认识
发表于 2025-3-22 02:25:46
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
人类
发表于 2025-3-22 07:37:19
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GREG
发表于 2025-3-22 10:29:57
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Demulcent
发表于 2025-3-22 16:36:55
978-981-97-1645-6The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
Demulcent
发表于 2025-3-22 20:57:40
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来这真柔软
发表于 2025-3-22 21:15:58
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表脸
发表于 2025-3-23 03:50:42
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
发表于 2025-3-23 07:27:33
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.