不同经纬度机场宇宙射线粒子的渐近方向和磁刚性截止

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2022-12-08 DOI:10.3103/S088459132206006X
Witold Wozniak, Krzysztof Iskra, Marek Siluszyk
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引用次数: 0

摘要

计算宇宙射线粒子的渐近方向是确定给定地理位置的刚性截止点的重要工具。本文利用地球磁场中宇宙辐射的荷电粒子运动方程的数值积分,给出了位于不同纬度和经度的8个机场(Apatity、Oulu、Warsaw、Lae、Buenos Aires、Wellington和Mc Murdo)的渐近纬度和渐近经度以及磁刚性截止值的计算结果。从地球中心到地面的初始距离为20公里。在大约这个高度,大多数宇宙射线会发生核碰撞。2015年对国际地磁场(IGRF)模型进行了计算。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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The Asymptotic Directions of Approach and the Magnetic Rigidity Cutoff of Cosmic Ray Particles for Airports at Different Latitudes and Longitudes

The calculation of asymptotic directions of approach of cosmic ray particles is an important tool in the determination of the rigidity cutoff for a given geographical site. We present the results of computations of the asymptotic latitude and asymptotic longitude and the magnetic rigidity cutoff for the eight airports (Apatity, Oulu, Warsaw, Lae, Buenos Aires Wellington and Mc Murdo) located at different latitudes and longitudes based on the numerical integration of equations of motion of charged particles of cosmic radiation in the Earth’s magnetic field. The initial distance from the center of the Earth was taken as 20 km above the surface. At about this altitude, most cosmic rays undergo nuclear collisions. Calculations were made for the model of the International Geomagnetic Reference Field (IGRF) in 2015.

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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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