Steady State Acceleration Model of Cosmic Ray in the Atmosphere

Akande P. I

Review of Industrial Engineering Letters, 2014, vol. 1, issue 1, 16-24

Abstract: Hydrodynamic equations were simplified to a layman understanding together with the diffusion-convection transport equation for the cosmic-ray distribution function f(t,r,p), which depends on time t , radial distance from the point of supernova explosion r and the particle momentum p. From the results, gas density p is inversely proportional to the gas velocity u ; flux tubes have a tendency to rise at an appreciable speed; pressure of the atmospheric gas Pg depends on the cosmic-ray pressure Pc and the internal energy of the electron U is directly proportional to the gas density p . Based on what Vladimir, et al. [1] said: “More work is needed to understand how robust our results are”, this has helped in making their bulky equations clearer and showing how robust their work are. In the cause of breaking down or simplifying the high energy equations, it was found that cosmic rays move with Alfven speed.

Keywords: Hydrodynamic; Cosmic ray; Atmosphere; Acceleration; High energy; Particles; Density; Steady state (search for similar items in EconPapers)
Date: 2014
References: Add references at CitEc
Citations: View citations in EconPapers (1)

Downloads: (external link)
https://archive.conscientiabeam.com/index.php/71/article/view/2637/4070 (application/pdf)

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:pkp:roiele:v:1:y:2014:i:1:p:16-24:id:2637

Access Statistics for this article

More articles in Review of Industrial Engineering Letters from Conscientia Beam
Bibliographic data for series maintained by Dim Michael ().