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Heiko Burau

dblp:136/7898 · DBLP profile ↗
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1ranked-venue papers
0as first author
0since 2021 · last 2013
—ORCID · unresolved

Domains — the database's venue-derived domains; a paper can count in several

Systems, architecture and hardware · 1

Expertise — from the expertise taxonomy: the topics of the expert's papers under the CCF categories. A weight counts papers with recency: 1 for a paper about the topic, 0.3 when the topic is its context, halved every five years.

Interdisciplinary, comprehensive, and emerging computing
1 paper
Computational science and engineering · 100%
Computer architecture, parallel and distributed computing, and storage systems
1 paper
High-performance computing · 100%

Topics — the 4 heaviest of 4, each with the papers that count most for it

TopicWeightPapersLastEvidence papers
Computational science and engineering › astronomy
astrophysics		 0.212013
Radiative signatures of the relativistic Kelvin-Helmholtz instability · SC 2013
Computational science and engineering › numerical simulation › particle simulation
particle-in-cell simulation		 0.212013
Radiative signatures of the relativistic Kelvin-Helmholtz instability · SC 2013
Computational science and engineering
plasma physics		 0.212013
Radiative signatures of the relativistic Kelvin-Helmholtz instability · SC 2013
High-performance computing
scientific computing systems		 0.012013
Radiative signatures of the relativistic Kelvin-Helmholtz instability · SC 2013

Methods — techniques the papers use, named apart from their topics

radiation spectra computation · 0.3particle-in-cell simulation · 0.3
YearPublicationVenuePosition
2013 Radiative signatures of the relativistic Kelvin-Helmholtz instability
abstract
We present a particle-in-cell simulation of the relativistic Kelvin-Helmholtz Instability (KHI) that for the first time delivers angularly resolved radiation spectra of the particle dynamics during the formation of the KHI. This enables studying the formation of the KHI with unprecedented spatial, angular and spectral resolution. Our results are of great importance for understanding astrophysical jet formation and comparable plasma phenomena by relating the particle motion observed in the KHI to its radiation signature.
Michael Bussmann, Heiko Burau, Thomas E. Cowan, Alexander Debus, Axel Huebl, Guido Juckeland, Thomas Kluge, Wolfgang E. Nagel, Richard Pausch, Felix Schmitt 0004, Ulrich Schramm, Joseph Schuchart, René Widera
 SC2