GALPROP WebRun: An internet-based service for calculating galactic cosmic ray propagation and associated photon emissions

被引:189
|
作者
Vladimirov, A. E. [1 ,2 ]
Digel, S. W. [1 ,2 ]
Johannesson, G. [1 ,2 ]
Michelson, P. P. [1 ,2 ]
Moskalenko, I. V. [1 ,2 ]
Nolan, P. L. [1 ,2 ]
Orlando, E. [1 ,2 ]
Porter, T. A. [1 ,2 ]
Strong, A. W. [3 ]
机构
[1] Stanford Univ, Dept Phys, WW Hansen Expt Phys Lab, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
[2] Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA
[3] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
关键词
Astroparticle physics; Diffusion; Elementary particles; Cosmic rays; ISM: general; Dark matter; Diffuse radiation; Gamma rays: ISM; Infrared: ISM; Radio continuum: ISM; X-rays: ISM; CONTINUUM GAMMA-RAYS; SECONDARY ANTIPROTONS; SUPERNOVA-REMNANTS; MILKY-WAY; GALAXY; MODEL;
D O I
10.1016/j.cpc.2011.01.017
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
GALPROP is a numerical code for calculating the galactic propagation of relativistic charged particles and the diffuse emissions produced during their propagation. The code incorporates as much realistic astrophysical input as possible together with latest theoretical developments and has become a de facto standard in astrophysics of cosmic rays. We present GALPROP WebRun, a service to the scientific community enabling easy use of the freely available GALPROP code via web browsers. In addition, we introduce the latest GALPROP version 54, available through this service. (C) 2011 Elsevier B.V. All rights reserved.
引用
收藏
页码:1156 / 1161
页数:6
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