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Cosmic Ray Anisotropy Workshop 2023

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

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Contribution List

45 out of 45 displayed
  1. 7. Registration
    16/05/2023, 08:00
  2. 8. Welcome
    Rasha Abbasi (Loyola University Chicago)
    16/05/2023, 08:30
  3. 52. Recent Results in Cosmic-Ray Astrophysics
    Carmelo Evoli (Gran Sasso Science Institute)
    16/05/2023, 08:45
  4. 48. Turbulence and CR propagation (remote)
    Gwenael Giacinti
    16/05/2023, 09:30
  5. 13. Recent Progress in Direct Measurements of Cosmic Rays (remote)
    Eun-Suk Seo (University of Maryland)
    16/05/2023, 10:05
  6. 51. Observation of cosmic-ray anisotropy with LHAASO (remote)
    Wei Gao
    16/05/2023, 11:10
  7. 12. Indirect Measurements of galactic Cosmic Rays
    Giuseppe Di Sciascio
    16/05/2023, 11:45
  8. 28. Living in the Bubble: structure, formation, and how it affects us
    Efrem Maconi
    16/05/2023, 14:00
  9. 14. CR anisotropy with IceCube
    Frank McNally (Mercer University), Rasha Abbasi (Loyola University Chicago)
    16/05/2023, 14:35
  10. 10. Transport of Galactic Cosmic-Ray Nuclei
    Benedikt Schroer
    16/05/2023, 15:10
  11. 11. Cosmic rays in a turbulent interstellar medium: Recent progress and open questions
    Philipp Mertsch
    16/05/2023, 16:15
  12. 16. Registration
    17/05/2023, 08:00
  13. 17. Selected Aspects of Magnetized Turbulence (with implications for CRs)
    Alex Lazarian
    17/05/2023, 08:45
  14. 18. Second order Fermi Acceleration in Galaxy Clusters
    Gianfranco Brunetti
    17/05/2023, 09:30
  15. 19. CR Acceleration in Turbulent Magnetic Reconnection (remote)
    Elisabete de Gouveia Dal Pino (IAG - Universidade de São Paulo)
    17/05/2023, 10:00
  16. 20. Cosmic ray diffusion in anisotropic MHD turbulence
    Siyao Xu
    17/05/2023, 11:00
  17. 22. Results from the High Altitude Water Cherenkov Observatory
    Miguel Mostafa
    17/05/2023, 11:30
  18. 21. Constraining the sources of ultra-high-energy cosmic rays with the Pierre Auger Observatory
    Teresa Bister
    17/05/2023, 12:00
  19. 43. Results from TA
    Tareq Abu-Zayyad
    17/05/2023, 14:00
  20. 38. Cosmic Ray Anisotropy with the Telescope Array
    Jihyun Kim
    17/05/2023, 14:30
  21. 23. New Models of the Magnetic Field of the Galaxy
    Michael Unger
    17/05/2023, 15:00
  22. 24. UHECR anisotropies
    Glennys Farrar
    17/05/2023, 16:00
  23. 25. Registration
    18/05/2023, 08:00
  24. 26. Heliosphere in the Local Interstellar Medium
    Nick Pogorelov
    18/05/2023, 08:45
  25. 27. The IBEX Ribbon and its Relation to the Solar-Interstellar Interaction (remote)
    Eric Zirnstein
    18/05/2023, 09:30
  26. 30. Cosmic ray pitch angle anisotropies in the Very Local Interstellar Medium
    Jaime Rankin
    18/05/2023, 10:00
  27. 29. Review of the Local ISM
    Jeff Linsky
    18/05/2023, 11:00
  28. 31. Turbulence in the local ISM
    Federico Fraternale
    18/05/2023, 11:45
  29. 47. The curious maximum-rigidity distribution of ultra-high-energy-cosmic-ray accelerators
    Foteini Oikonomou (Norwegian University of Science and Technology)
    18/05/2023, 12:15

    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
    18/05/2023, 14:15
  31. 33. Heliosphere and TeV CR anisotropy
    Ming Zhang (Florida Institute of Technology)
    18/05/2023, 14:45
  32. 32. Modeling of cosmic-ray anisotropy at TeV energies in an MHD model heliosphere
    Takashi Sako
    18/05/2023, 15:15
  33. 40. The Relationship between the Local ISM Distribution and Milky Way Spiral Structure
    Robert Benjamin
    18/05/2023, 16:15
  34. 44. IceCube: The first Decade of Neutrino Astronomy
    Francis Halzen (University of Wisconsin–Madison)
    19/05/2023, 08:45
  35. 35. Cross-correlation studies with UHECRs (remote)
    Federico Urban
    19/05/2023, 09:30
  36. 36. Local Sources of Cosmic Rays
    Igor Moskalenko
    19/05/2023, 10:30
  37. 37. Wrapping up and Collecting thoughts on Cosmic Ray Astrophysics
    Pasquale Blasi
    19/05/2023, 11:00
  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