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Signatures of the propagation of primary and secondary cosmic ray electrons and positrons in the galaxy /Porter, Troy Anthony. January 1999 (has links) (PDF)
Thesis (Ph. D.)--University of Adelaide, Dept. of Physics and Mathematical Physics, 1999. / Includes bibliographical references (8 p. ).
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Signatures of the propagation of primary and secondary cosmic ray electrons and positrons in the galaxyPorter, Troy Anthony. January 1999 (has links) (PDF)
Includes bibliographical references (8 p.) Examines some of the consequences of the acceleration and production, and propagation, of high energy electrons and positrons in the Galaxy. In particular, predictions are made of the diffuse photon signals arising from the interactions of electrons and positrons with gas, low energy photons, and the galactic magnetic field during their transport in the Galaxy.
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Signatures of the propagation of primary and secondary cosmic ray electrons and positrons in the galaxy / Troy Anthony Porter.Porter, Troy Anthony January 1999 (has links)
Includes bibliographical references (8 p.) / ix, 173, [8] p. : ill. ; 30 cm. / Title page, contents and abstract only. The complete thesis in print form is available from the University Library. / Examines some of the consequences of the acceleration and production, and propagation, of high energy electrons and positrons in the Galaxy. In particular, predictions are made of the diffuse photon signals arising from the interactions of electrons and positrons with gas, low energy photons, and the galactic magnetic field during their transport in the Galaxy. / Thesis (Ph.D.)--University of Adelaide, Dept. of Physics and Mathematical Physics, 1999
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Signatures of the propagation of primary and secondary cosmic ray electrons and positrons in the galaxy / Troy Anthony Porter.Porter, Troy Anthony January 1999 (has links)
Includes bibliographical references (8 p.) / ix, 173, [8] p. : ill. ; 30 cm. / Title page, contents and abstract only. The complete thesis in print form is available from the University Library. / Examines some of the consequences of the acceleration and production, and propagation, of high energy electrons and positrons in the Galaxy. In particular, predictions are made of the diffuse photon signals arising from the interactions of electrons and positrons with gas, low energy photons, and the galactic magnetic field during their transport in the Galaxy. / Thesis (Ph.D.)--University of Adelaide, Dept. of Physics and Mathematical Physics, 1999
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