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Cosmic Ray Anisotropy Workshop 2011

28–29 Oct 2011
University of Wisconsin Pyle Center
US/Central timezone

Session

Anisotropy measurements and astrophysical models

session4_day1
28 Oct 2011, 16:40
309 (University of Wisconsin Pyle Center)

309

University of Wisconsin Pyle Center

702 Langdon Street Madison, WI 53706-1487

Presentation materials

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  1. 15. Large scale distribution of arrival directions of cosmic rays above ~100 PeV
    Dr Olivier Deligny (Institut de Physique Nucléaire Orsay)
    28/10/2011, 16:40
    Scrutiny of the large scale distribution of arrival directions of cosmic rays with energies above ~100 PeV is one important observable to provide key elements for understanding the end of Galactic cosmic rays, and for establishing at which energy the flux of extragalactic cosmic rays starts to dominate the cosmic ray energy spectrum. Using the large amount of data collected by the Pierre...
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  2. 25. An explanation for the cosmic ray anisotropies at multiple scales
    Dr Gwenael Giacinti (NTNU Trondheim and APC Paris)
    28/10/2011, 17:10
    We propose an explanation for the origin of the observed cosmic ray anisotropies at multiple scales. We discuss its implications, and future perspectives.
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  3. 27. The origin of the cosmic ray positron/electron excess and beyond
    Dr Hasan Yuksel (LANL)
    28/10/2011, 17:40
    The spectra of cosmic electrons and positrons should have contributions from known sources such as particles accelerated in supernova remnants and from interactions of cosmic and interstellar protons. Any evidence for an additional component, as reported by PAMELA, Fermi and HESS experiments, may carry hints of a new phenomenon. I will examine the implications of the recent detection of...
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