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Cosmic Ray Anisotropy Workshop 2023

May 16 – 19, 2023
Loyola University - Chicago
US/Central timezone

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Contribution List

45 out of 45 displayed
  1. 7. Registration
    5/16/23, 8:00 AM
  2. 8. Welcome
    Rasha Abbasi (Loyola University Chicago)
    5/16/23, 8:30 AM
  3. 52. Recent Results in Cosmic-Ray Astrophysics
    Carmelo Evoli (Gran Sasso Science Institute)
    5/16/23, 8:45 AM
  4. 48. Turbulence and CR propagation (remote)
    Gwenael Giacinti
    5/16/23, 9:30 AM
  5. 13. Recent Progress in Direct Measurements of Cosmic Rays (remote)
    Eun-Suk Seo (University of Maryland)
    5/16/23, 10:05 AM
  6. 51. Observation of cosmic-ray anisotropy with LHAASO (remote)
    Wei Gao
    5/16/23, 11:10 AM
  7. 12. Indirect Measurements of galactic Cosmic Rays
    Giuseppe Di Sciascio
    5/16/23, 11:45 AM
  8. 28. Living in the Bubble: structure, formation, and how it affects us
    Efrem Maconi
    5/16/23, 2:00 PM
  9. 14. CR anisotropy with IceCube
    Frank McNally (Mercer University), Rasha Abbasi (Loyola University Chicago)
    5/16/23, 2:35 PM
  10. 10. Transport of Galactic Cosmic-Ray Nuclei
    Benedikt Schroer
    5/16/23, 3:10 PM
  11. 11. Cosmic rays in a turbulent interstellar medium: Recent progress and open questions
    Philipp Mertsch
    5/16/23, 4:15 PM
  12. 16. Registration
    5/17/23, 8:00 AM
  13. 17. Selected Aspects of Magnetized Turbulence (with implications for CRs)
    Alex Lazarian
    5/17/23, 8:45 AM
  14. 18. Second order Fermi Acceleration in Galaxy Clusters
    Gianfranco Brunetti
    5/17/23, 9:30 AM
  15. 19. CR Acceleration in Turbulent Magnetic Reconnection (remote)
    Elisabete de Gouveia Dal Pino (IAG - Universidade de São Paulo)
    5/17/23, 10:00 AM
  16. 20. Cosmic ray diffusion in anisotropic MHD turbulence
    Siyao Xu
    5/17/23, 11:00 AM
  17. 22. Results from the High Altitude Water Cherenkov Observatory
    Miguel Mostafa
    5/17/23, 11:30 AM
  18. 21. Constraining the sources of ultra-high-energy cosmic rays with the Pierre Auger Observatory
    Teresa Bister
    5/17/23, 12:00 PM
  19. 43. Results from TA
    Tareq Abu-Zayyad
    5/17/23, 2:00 PM
  20. 38. Cosmic Ray Anisotropy with the Telescope Array
    Jihyun Kim
    5/17/23, 2:30 PM
  21. 23. New Models of the Magnetic Field of the Galaxy
    Michael Unger
    5/17/23, 3:00 PM
  22. 24. UHECR anisotropies
    Glennys Farrar
    5/17/23, 4:00 PM
  23. 25. Registration
    5/18/23, 8:00 AM
  24. 26. Heliosphere in the Local Interstellar Medium
    Nick Pogorelov
    5/18/23, 8:45 AM
  25. 27. The IBEX Ribbon and its Relation to the Solar-Interstellar Interaction (remote)
    Eric Zirnstein
    5/18/23, 9:30 AM
  26. 30. Cosmic ray pitch angle anisotropies in the Very Local Interstellar Medium
    Jaime Rankin
    5/18/23, 10:00 AM
  27. 29. Review of the Local ISM
    Jeff Linsky
    5/18/23, 11:00 AM
  28. 31. Turbulence in the local ISM
    Federico Fraternale
    5/18/23, 11:45 AM
  29. 47. The curious maximum-rigidity distribution of ultra-high-energy-cosmic-ray accelerators
    Foteini Oikonomou (Norwegian University of Science and Technology)
    5/18/23, 12:15 PM

    A standard assumption among models of candidate source populations of ultra-high energy cosmic rays (UHECRs) is that all sources in a candidate source population accelerate particles to the same maximum energy. Motivated by the fact that candidate astrophysical accelerators exhibit a vast diversity in terms of their relevant properties, such as luminosity, Lorentz factor, and magnetic field...

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  30. 34. Configuration of Interstellar Magnetic Field Surrounding the Heliosphere (remote)
    Priscilla Frisch
    5/18/23, 2:15 PM
  31. 33. Heliosphere and TeV CR anisotropy
    Ming Zhang (Florida Institute of Technology)
    5/18/23, 2:45 PM
  32. 32. Modeling of cosmic-ray anisotropy at TeV energies in an MHD model heliosphere
    Takashi Sako
    5/18/23, 3:15 PM
  33. 40. The Relationship between the Local ISM Distribution and Milky Way Spiral Structure
    Robert Benjamin
    5/18/23, 4:15 PM
  34. 44. IceCube: The first Decade of Neutrino Astronomy
    Francis Halzen (University of Wisconsin–Madison)
    5/19/23, 8:45 AM
  35. 35. Cross-correlation studies with UHECRs (remote)
    Federico Urban
    5/19/23, 9:30 AM
  36. 36. Local Sources of Cosmic Rays
    Igor Moskalenko
    5/19/23, 10:30 AM
  37. 37. Wrapping up and Collecting thoughts on Cosmic Ray Astrophysics
    Pasquale Blasi
    5/19/23, 11:00 AM
  38. 49. Cosmic Ray Anisotropy with the Telescope Array
    Jihyun Kim (University of Utah)

    Ultra-high energy cosmic rays (UHECRs) are charged particles that are extremely energetic, with $E > 10^{18}$ eV. They impinge on the Earth's atmosphere from outer space. The Telescope Array experiment, the largest UHECR observatory in the northern hemisphere, is situated in the western desert of Utah, USA, and has been collecting data continuously since May 2008. It is designed to detect...

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  39. 45. Cosmic rays in a turbulent interstellar medium: Recent progress and open questions
    Philipp Mertsch

    TBD

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  40. 15. CR anisotropy with IceTop - Rasha Abbasi
  41. 41. Modeling of cosmic-ray anisotropy at TeV energies in an MHD model heliosphere
    Takashi Sako

    Past and on-going cosmic-ray experiments have reported small (∼0.1%) anisotropies in the arrival directions of TeV cosmic rays observed at the Earth.
    We are attempting to estimate anisotropic features at the heliospheric boundary by applying the idea of Liouville mapping to the data of the Tibet AS$\gamma$ experiment.
    Our preliminary results have indicated small, possibly spurious,...

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  42. 50. Observation of cosmic-ray anisotropy with LHAASO
    Wei Gao (Institute of High Energy Physics)

    Observation of cosmic-ray anisotropy with LHAASO

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  43. 42. Review of the Local ISM
    Prof. Jeffrey Linsky (University of Colorado)

    The local interstellar medium (LISM), consisting of neutral and ionized gas, dust, and magnetic fields, is the environment for the heliosphere and stellar astrospheres. LISM gas and magnetic fields penetrate deeply into these environments. The LISM consists of the partially ionized gas clouds extending to about 10 pc from the Sun, the surrounding Local Bubble with its fully ionized hydrogen...

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  44. 46. The IBEX Ribbon and its Relation to the Solar-Interstellar Interaction
    Eric Zirnstein (Princeton University)

    NASA’s Interstellar Boundary Explorer (IBEX), an Earth-orbiting Small Explorer spacecraft, measures energetic neutral atom (ENAs) produced primarily by charge exchange in the outer heliosphere. There are two main sources of ENAs. The first, called the “globally distributed flux”, is formed from neutralization of interstellar pickup ions that were preferentially accelerated at the heliospheric...

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  45. 39. Welcome