Erratum to "Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory" [Astroparticle Physics 32(2) (2009), 89-99]
Erratum to "Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory" [Astroparticle Physics 32(2) (2009), 89-99]
复制标题
“用皮埃尔·俄歇天文台表面探测器观测到的大气对大范围空气簇射的影响”勘误表 [AstropolitanarticlePhysics 32(2) (2009), 89-99]
DOI：
10.1016/j.astropartphys.2009.10.005
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发表时间：
2010
影响因子：
3.5
通讯作者：
Abraham J
中科院分区：
文献类型：
--
作者：
Abraham J
高能宇宙射线（CR）是通过记录它们在大气中产生的二次粒子的大量空气簇射（EAS）来测量的。由于大气是流星雨演化的介质，其状态影响着流星雨的横向和纵向发展。压力 (P) 和空气密度 (ρ) 是主要影响 EAS 的大气属性。地面 P 的增加（或减少）对应于增加（或
High-energy cosmic rays (CRs) are measured by recording the extensive air showers (EAS) of secondary particles they produce in the atmosphere. As the atmosphere is the medium in which the shower evolves, its state affects the lateral and longitudinal development of the shower. Pressure (P) and air density (ρ) are the properties of the atmosphere that mostly affect the EAS. An increase (or decrease) of the ground P corresponds to an increased (or