T 73: Cosmic Ray 4
Wednesday, March 23, 2022, 16:15–18:15, T-H32
| |
16:15 |
T 73.1 |
The contribution has been withdrawn.
|
|
|
 |
16:30 |
T 73.2 |
Incorporating the Galactic magnetic field into the propagation effects of cosmic rays in the transition region* — •Alex Kääpä
|
|
|
|
16:45 |
T 73.3 |
Influence of diffusive cosmic-ray transport on multimessenger observables — •Patrick Reichherzer, Julia Becker Tjus, Lukas Merten, Leander Schlegel, Julien Dörner, M.J. Pueschel, and Ellen Zweibel
|
|
|
|
17:00 |
T 73.4 |
Perception of arrival direction maps of cosmic rays — •Edyvania Emily Pereira Martins, Markus Roth, and Darko Veberič
|
|
|
|
17:15 |
T 73.5 |
Self-confinement of low-energy cosmic rays around supernova remnants — •Hanno Jacobs, Philipp Mertsch, and Vo-Hong Minh Phan
|
|
|
|
17:30 |
T 73.6 |
No longer ballistic, not yet diffusive--the formation of cosmic ray small-scale anisotropies — •Marco Kuhlen, Vo Hong Minh Phan, and Philipp Mertsch
|
|
|
|
17:45 |
T 73.7 |
Non-thermal ion acceleration at highly oblique non-relativistic shocks — •Naveen Kumar and Brian Reville
|
|
|
|
18:00 |
T 73.8 |
Can superbubbles accelerate PeV protons? — •Thibault Vieu and Brian Reville
|
|
|
