P
Patrick Diamond
Researcher at University of California, San Diego
Publications - 621
Citations - 24103
Patrick Diamond is an academic researcher from University of California, San Diego. The author has contributed to research in topics: Turbulence & Wave turbulence. The author has an hindex of 71, co-authored 604 publications receiving 22522 citations. Previous affiliations of Patrick Diamond include General Atomics & University of Wisconsin-Madison.
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Journal ArticleDOI
Editorial introduction to the special issue “Plasma physics in the 20th century as told by players”
TL;DR: The history of plasma physics can be traced back to the period from 1950 to 2000 as discussed by the authors, when the first plasma physics experiments were conducted in the Soviet Union/Russia and beyond, with a key player, Roald Sagdeev, interviewed by one of us.
MonographDOI
Relaxation dynamics in laboratory and astrophysical plasmas
TL;DR: Magnetic Relaxation and Self-Organization in Astrophysical and Laboratory Plasmas: Mean Field Dynamo Theory Origin, Structure and Stability ofAstrophysical MHD Jets Turbulence and Turbulent Transport - The Agents of Relaxation.
Journal Article
Structure and Scale of Cosmic Ray Modified Shocks
TL;DR: In this paper, the authors show that while the CR pressure builds up ahead of the supernova, the acceleration enters into a strongly nonlinear phase in which an acoustic instability, driven by the CR-pressure gradient, dominates other instabilities (at least in the case of low β plasma).
Posted ContentDOI
Mouth Function Determines The Shape Oscillation Pattern In Regenerating Hydra Tissue Spheres
Rui Wang,Tapan Goel,Kate Khazoyan,Ziad Sabry,Heng J. Quan,Patrick Diamond,Eva-Maria S. Collins,Eva-Maria S. Collins +7 more
TL;DR: The experiments demonstrate that the shift in the shape oscillation pattern in regenerating Hydra tissue pieces is caused by the formation of a functional mouth, thereby linking morphological readouts to physiologically relevant events during regeneration.
Proceedings ArticleDOI
Angular distribution of energetic particles scattered by strongly anisotropic MHD turbulence: Understanding Milagro/IceCube results
TL;DR: In this article, the authors proposed a mechanism for producing a cosmic ray (CR) beam which operates en route to the observer using a strongly anisotropic wave spectrum formed by the turbulent cascade across the local field direction.