Bonn 2020 –
wissenschaftliches Programm
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T 103: Cosmic rays IV
Freitag, 3. April 2020, 11:00–13:00, L-3.002
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11:00 |
T 103.1 |
Connection between turbulence and diffusive Cosmic Ray transport in the ISM — •Julien Dörner, Patrick Reichherzer, and Julia Tjus
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11:15 |
T 103.2 |
Propagation in the Galactic magnetic field: Effects on the spectrum, composition and anisotropy of Galactic and extragalactic cosmic rays * — •Alex Kääpä for the Pierre Auger collaboration
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11:30 |
T 103.3 |
Deepening the understanding of cosmic-ray diffusion — •Patrick Reichherzer, Julia Tjus, Ellen Zweibel, Lukas Merten, and M.J. Pueschel
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11:45 |
T 103.4 |
Investigation of a Combined Fit Method to Identify a Nearby Cosmic Ray Source — Teresa Bister, Martin Erdmann, •Josina Schulte, and Marcus Wirtz
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12:00 |
T 103.5 |
Predicting the UHE photon flux from GZK-interactions of hadronic cosmic rays using CRPropa 3 — •Anna Bobrikova, Marcus Niechciol, Markus Risse, and Philip Ruehl for the Pierre Auger collaboration
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12:15 |
T 103.6 |
Search for Cosmic Ray Sources Using Graph Convolutional Neural Networks — Teresa Bister, Martin Erdmann, Jonas Glombitza, •Niklas Langner, Josina Schulte, and Marcus Wirtz
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12:30 |
T 103.7 |
Testing The Pierre Auger Observatory Starburst Galaxy and Active Galactic Nuclei Correlation Anisotropy Result with CRPropa Simulations — •Wilson Namasaka
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12:45 |
T 103.8 |
Fitting cosmic ray charges to cluster in accordance with an extragalactic source model — •Teresa Bister, Martin Erdmann, and Marcus Wirtz
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