Effect of random nature of cosmic ray sources - Supernova remnants - on cosmic ray intensity fluctuations, anisotropy, and electron energy spectrum

被引：60

作者：

Ptuskin, V. S. ^{[1
]}

Jones, F. C.

Seo, E. S.

Sina, R.

机构：

[1] IZMIRAN, Inst Terr Magnetism Ionosphere & Radiowave Propag, Lab Astrophys Res, Moscow 142190, Russia

[2] Univ Maryland, Inst Phys Sci & Technol, College Pk, MD 20742 USA

[3] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA

来源：

ASTROPHYSICS | 2006年 / 37卷 / 10期

基金：

俄罗斯基础研究基金会; 美国国家航空航天局;

关键词：

cosmic rays; supernova remnants;

D O I：

10.1016/j.asr.2005.08.036

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The random nature of sources (the supernova remnants) leads to the fluctuations of cosmic ray intensity in space and time. We calculate the expected fluctuations in a flat-halo diffusion model for particles with energies from 0.1 to 10(3) TeV. The data on energy spectra and anisotropy of very high energy protons, nuclei and electrons, and the astronomical data on supernova remnants, the potential sources of cosmic rays, are used to constrain the value of the cosmic-ray diffusion coefficient and its dependence on energy. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：1909 / 1912

页数：4

共 16 条

[1] Search for the sidereal and solar diurnal modulations in the total MACRO muon data set -: art. no. 042002 [J].

Ambrosio, M ;

Antolini, R ;

Baldini, A ;

Barbarino, GC ;

Barish, BC ;

Battistoni, G ;

Becherini, Y ;

Bellotti, R ;

Bemporad, C ;

Bernardini, P ;

Bilokon, H ;

Bower, C ;

Brigida, M ;

Bussino, S ;

Cafagna, F ;

Calicchio, M ;

Campana, D ;

Carboni, M ;

Caruso, R ;

Cecchini, S ;

Cei, F ;

Chiarella, V ;

Chiarusi, T ;

Choudhary, BC ;

Coutu, S ;

Cozzi, M ;

De Cataldo, G ;

Dekhissi, H ;

De Marzo, C ;

De Mitri, I ;

Derkaoui, J ;

De Vincenzi, M ;

Di Credico, A ;

Erriquez, O ;

Favuzzi, C ;

Forti, C ;

Fusco, P ;

Giacomelli, G ;

Giannini, G ;

Giglietto, N ;

Giorgini, M ;

Grassi, M ;

Grillo, A ;

Gustavino, C ;

Habig, A ;

Hanson, K ;

Heinz, R ;

Katsavounidis, E ;

Katsavounidis, I ;

Kearns, E .

PHYSICAL REVIEW D, 2003, 67 (04)

[2] Discovery of a young nearby supernova remnant [J].

Aschenbach, B .

NATURE, 1998, 396 (6707) :141-142

[3]

Berezinskii V. S., 1990, Astrophysics of cosmic rays

[4]

CASE G, 1996, A AS, V120, P437

[5] DIFFUSION OF THE GALACTIC COSMIC-RAYS IN THE VICINITY OF THE SOLAR-SYSTEM [J].

DORMAN, LI ;

GHOSH, A ;

PTUSKIN, VS .

ASTROPHYSICS AND SPACE SCIENCE, 1985, 109 (01) :87-97

[6] Emission from 44Ti associated with a previously unknown Galactic supernova [J].

Iyudin, AF ;

Schönfelder, V ;

Bennett, K ;

Bloemen, H ;

Diehl, R ;

Hermsen, W ;

Lichti, GG ;

van der Meulen, RD ;

Ryan, J ;

Winkler, C .

NATURE, 1998, 396 (6707) :142-144

[7] The modified weighted slab technique: Models and results [J].

Jones, FC ;

Lukasiak, A ;

Ptuskin, V ;

Webber, W .

ASTROPHYSICAL JOURNAL, 2001, 547 (01) :264-271

[8]

JONES FC, 1969, ACTA PHYS ACAD SC S1, V29, P23

[9] The most likely sources of high-energy cosmic-ray electrons in supernova remnants [J].

Kobayashi, T ;

Komori, Y ;

Yoshida, K ;

Nishimura, J .

ASTROPHYSICAL JOURNAL, 2004, 601 (01) :340-351

[10]

Lagutin A. A., 1995, Journal of Experimental and Theoretical Physics, V81, P825

← 1 2 →