Staff profile

Prof Sir Arnold Wolfendale

Emeritus Professor in the Department of Physics

Telephone: +44 (0) 191 33 43580

Room number: 212

(email at a.w.wolfendale@durham.ac.uk)

Research Groups

High Energy Astrophysics

Publications

Books: authored

Erlykin, AD & Wolfendale, AW (2001). Models for the origin of the knee in the cosmic-ray spectrum. AMSTERDAM: ELSEVIER SCIENCE BV.

Journal papers: academic

Erlykin, A. D. & Wolfendale, A. W. (2006). The anisotropy of galactic cosmic rays as a product of stochastic supernova explosions. Astroparticle Physics 25(3): 183-194.
Erlykin, AD & Wolfendale, AW (2006). The nature of the 'knee' in the cosmic ray energy spectrum. Journal Of Physics G-nuclear And Particle Physics 32(1): 1-7.
Erlykin, AD & Wolfendale, AW (2005). 'Sling effect' in the development of atmospheric cascades induced byprimary cosmic ray nuclei. Journal Of Physics G-nuclear And Particle Physics 31(7): 791-802.
Wibig, T & Wolfendale, AW (2005). At what particle energy do extragalactic cosmic rays start topredominate?. Journal Of Physics G-nuclear And Particle Physics 31(3): 255-264.
Wibig, T & Wolfendale, AW (2005). Cosmic rays and cosmology. International Journal Of Modern Physics A 20(29): 6612-6620.
Wibig, T. & Wolfendale, A. W. (2005). Foreground contributions to the cosmic microwave background. Monthly Notices of the Royal Astronomical Society 360(1): 236-252.
Erlykin, AD & Wolfendale, AW (2005). Further evidence favouring the single source model for cosmic rays. Astroparticle Physics 23(1): 1-9.
Erlykin, A. D. & Wolfendale, A. W. (2005). The origin of cosmic rays. Journal of Physics G-nuclear and Particle Physics 31(12): 1475-1498.
Wibig, T & Wolfendale, AW (2004). Cosmic rays and cosmology. Nuclear Physics B-proceedings Supplements 136: 179-184.
Erlykin, AD & Wolfendale, AW (2004). Cosmic rays and the Monogem supernova remnant. Astroparticle Physics 22(1): 47-63.
Myers, AD, Shanks, T, Outram, PJ, Frith, WJ & Wolfendale, AW (2004). Evidence for an extended Sunyaev-Zel'dovich effect in WMAP data. Monthly Notices Of The Royal Astronomical Society 347(4): L67-L72.
Erlykin, AD & Wolfendale, AW (2004). Sling effect in AA-interactions and its implication for UHECR. Nuclear Physics B-proceedings Supplements 136: 282-289.
Wibig, T & Wolfendale, AW (2004). Ultra-high energy cosmic rays from transient extragalactic sources. Journal Of Physics G-nuclear And Particle Physics 30(4): 525-542.
Wolfendale, A. W. (2003). Cosmic ray origin: the way ahead. Journal of Physics G: Nuclear and Particle Physics 29(5): 787-800.
Erlykin, AD & Wolfendale, AW (2003). High-energy cosmic gamma rays from the 'single source'. Journal Of Physics G-nuclear And Particle Physics 29(4): 709-718.
Erlykin, AD & Wolfendale, AW (2003). How should we modify the high energy interaction models?. Nuclear Physics B-proceedings Supplements 122: 368-371.
Erlykin, AD, Lagutin, AA & Wolfendale, AW (2003). Properties of the interstellar medium and the propagation of cosmicrays in the Galaxy. Astroparticle Physics 19(3): 351-362.
Erlykin, AD & Wolfendale, AW (2003). Spectral features and masses in the PeV region. Nuclear Physics B-proceedings Supplements 122: 209-212.
Erlykin, A. D. & Wolfendale, A. W. (2003). The visibility of shell-type supernova remnants in gamma rays. Journal of Physics G-Nuclear and Particle Physics 29(4): 641-664.
Szabelski, J, Wibig, T & Wolfendale, AW (2002). Cosmic rays of the highest energies: the case for extragalactic heavynuclei. Astroparticle Physics 17(2): 125-131.
Erlykin, AD & Wolfendale, AW (2002). Properties of cosmic ray interactions at PeV energies. Astroparticle Physics 18(2): 151-164.
Erlykin, AD & Wolfendale, AW (2002). Supernova remnants and the origin of cosmic radiation: evidence fromlow-energy gamma rays. Journal Of Physics G-nuclear And Particle Physics 28(9): 2329-2348.
Erlykin, AD & Wolfendale, AW (2002). Supernova remnants and the origin of the cosmic radiation: the electroncomponent. Journal Of Physics G-nuclear And Particle Physics 28(3): 359-378.
Erlykin, AD, Mikhailov, AA & Wolfendale, AW (2002). Ultra high energy cosmic rays and pulsars. Journal Of Physics G-nuclear And Particle Physics 28(8): 2225-2233.
Erlykin, AD, Wibig, T & Wolfendale, AW (2001). A universal origin for cosmic rays above 10(7) GeV?. New Journal Of Physics 3: 181-1814.
Erlykin, AD & Wolfendale, AW (2001). Cosmic ray ions, dust and the interstellar medium. Physica Scripta T95: 92-95.
Erlykin, AD & Wolfendale, AW (2001). Cosmic ray ions, dust and the interstellar medium. Physica Scripta 63(6): 504-507.
Wolfendale, AW & Wibig, T (2001). Prospects for extragalactic particles from exotic processes. Journal Of Physics G-nuclear And Particle Physics 27(7): 1625-1631.
Erlykin, AD & Wolfendale, AW (2001). Structure in the cosmic ray spectrum: an update. Journal Of Physics G-nuclear And Particle Physics 27(5): 1005-1030.
Erlykin, AD & Wolfendale, AW (2001). Supernova remnants and the origin of the cosmic radiation: I. SNRacceleration models and their predictions. Journal Of Physics G-nuclear And Particle Physics 27(5): 941-958.
Erlykin, AD & Wolfendale, AW (2001). Supernova remnants and the origin of the cosmic radiation: II. Spectralvariations in space and time. Journal Of Physics G-nuclear And Particle Physics 27(5): 959-976.
Erlykin, AD & Wolfendale, AW (2001). Supernova remnants and the origin of the cosmic radiation: III.Spectral differences for different nuclei. Journal Of Physics G-nuclear And Particle Physics 27(8): 1709-1721.
Erlykin, AD, Fatemi, SJ & Wolfendale, AW (2000). Fine structure in the energy spectrum of cosmic ray protons at 50 GeV?. Physics Letters B 482(4): 337-342.
Wibig, Y & Wolfendale, AW (2000). Limits to the flux of ultra-high-energy cosmic rays from exoticphenomena in the galactic halo. Journal Of Physics G-nuclear And Particle Physics 26(7): 1033-1047.
Erlykin, AD & Wolfendale, AW (2000). Multiple muons in cosmic rays and the single source model of the knee. Journal Of Physics G-nuclear And Particle Physics 26(2): 203-218.
Erlykin, AD & Wolfendale, AW (2000). The origin of PeV cosmic rays. Astronomy And Astrophysics 356(3): L63-L65.