P 15: Astrophysical Plasmas
Wednesday, April 2, 2025, 16:15–17:45, ZHG102
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16:15 |
P 15.1 |
Can a Compressible Jet Sustain Significant Turbulence in a (Magnetized) Turbulent Environment? — •David Kube, Gabriele Camerlengo, Wolf-Christian Müller, and Jörn Sesterhenn
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16:30 |
P 15.2 |
Nonmetal-to-metal transition in liquid hydrogen using density functional theory and the HSE XC functional — Armin Bergermann, Lucas Kleindienst, and •Ronald Redmer
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16:45 |
P 15.3 |
Marginal Role of the Electrostatic Instability in the GeV Scale Cascade Flux from 1ES 0229+200 — •Martin Pohl and Mahmoud Alawashra
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17:00 |
P 15.4 |
Particle acceleration at oblique high-Mach-Number shocks propagating in a turbulent medium — •Eloise Moore, Karol Fulat, Michelle Tsirou, and Martin Pohl
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17:15 |
P 15.5 |
Measuring the Free-Free Opacity of Hydrogen at Stellar Interior Conditions Using the National Ignition Facility — •Samuel Schumacher, Julian Lütgert, Ronald Redmer, Mandy Bethkenhagen, Laurent Masse, Dirk Gericke, Siegfried Glenzer, Tilo Döppner, Tina Ebert, Gareth Hall, Otto Landen, Markus Schölmerich, Charles Starrett, Nathaniel Shaffer, Laurent Divol, Benjamin Bachmann, Steve MacLaren, Clement Trosseille, Shahab Khan, and Dominik Kraus
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17:30 |
P 15.6 |
Stereoscopic observations reveal coherent morphology and evolution of solar coronal loops — •B. Ram, L. P. Chitta, S. Mandal, H. Peter, and F. Plaschke
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