Constraining the Thickness of the Galactic Halo through Cosmic-Ray Anisotropy Using the Spatial-Dependent-Propagation Model

Constraining the Thickness of the Galactic Halo through Cosmic-Ray Anisotropy Using the Spatial-Dependent-Propagation Model

The spatial-dependent-propagation (SDP) model with a nearby source works well to reproduce the coevolving features of both cosmic-ray (CR)-nuclei spectra and anisotropy. However, it is well known that the Sun is actually deviating from the galactic disk. This will lead to a dominating anisotropy in...

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Bibliographic Details
Main Authors: Bing-Qiang Qiao, Yu-Hua Yao, Wei Liu, Qiang Yuan, Xiao-Jun Bi, Hong-Bo Hu, Yi-Qing Guo
Format: Article
Language:English
Published: MDPI AG 2023-08-01
Series:Universe
Subjects:
spatial-dependent propagation
cosmic-ray anisotropy
nearby source
solar offset
thick halo
Online Access:https://www.mdpi.com/2218-1997/9/8/363

Internet

https://www.mdpi.com/2218-1997/9/8/363

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