Loading…

Introduction to Large High Altitude Air Shower Observatory (LHAASO)

Since the century discovery of cosmic ray, the origin of cosmic ray is always a mystery. The study on the origin of high-energy cosmic ray is in an interdiscipline between the very high-energy (VHE) gamma-ray astronomy and the cosmic ray physics. The Large High Altitude Air Shower Observatory (LHAAS...

Full description

Saved in:
Bibliographic Details
Published in:Chinese astronomy and astrophysics 2019-10, Vol.43 (4), p.457-478
Main Authors: Zhen, Cao, Ming-jun, Chen, Song-zhan, Chen, Hong-bo, Hu, Cheng, Liu, Ye, Liu, Ling-ling, Ma, Xin-hua, Ma, Xiang-dong, Sheng, Han-rong, Wu, Gang, Xiao, Zhi-guo, Yao, Li-qiao, Yin, Min, Zha, Shou-shan, Zhang
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Since the century discovery of cosmic ray, the origin of cosmic ray is always a mystery. The study on the origin of high-energy cosmic ray is in an interdiscipline between the very high-energy (VHE) gamma-ray astronomy and the cosmic ray physics. The Large High Altitude Air Shower Observatory (LHAASO) is a unique and new generation cosmic-ray station with the advantages of high altitude, all-weather, and large-scale. It takes the function of hybrid technology to detect cosmic rays and to upgrade greatly the resolving power between gamma rays and cosmic rays. The LHAASO is expected to make the full-sky survey to find new gamma-ray sources, to obtain the highest sensitivity of gamma-ray detection at the high energy band of > 30 TeV, and to make the very high precision measurement on the component energy spectra of cosmic rays in a broad energy range of 5 orders of magnitude, in order to provide the evidence for revealing the mystery of the origin of cosmic ray. This paper describes the detector structure, performance superiority and scientific motivation of the LHAASO.
ISSN:0275-1062
1879-128X
DOI:10.1016/j.chinastron.2019.11.001