✦ LIBER ✦

Three-dimensional Weibel instability in astrophysical scenarios

✍ Scribed by Fonseca, Ricardo A.; Silva, Luı́s O.; Tonge, John W.; Mori, Warren B.; Dawson, John M.

Book ID: 120460749
Publisher: American Institute of Physics
Year: 2003
Tongue: English
Weight: 437 KB
Volume: 10
Category: Article
ISSN: 1070-664X
DOI: 10.1063/1.1556605

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

On the role of the purely transverse Wei

On the role of the purely transverse Weibel instability in fast ignitor scenarios

✍ Silva, Luı́s O.; Fonseca, Ricardo A.; Tonge, John W.; Mori, Warren B.; Dawson, J 📂 Article 📅 2002 🏛 American Institute of Physics 🌐 English ⚖ 297 KB

Effects of Beam Energy Spread on the Wei

Effects of Beam Energy Spread on the Weibel Instability in Fast Ignitor Scenarios

✍ Hong-Bo, Cai; Shao-Ping, Zhu; Chun-Yang, Zheng; Xian-Tu, He; Ji-Wei, Li 📂 Article 📅 2006 🏛 Institute of Physics 🌐 English ⚖ 275 KB

Three dimensional reconnection in astrop

Three dimensional reconnection in astrophysical plasmas

✍ D.S. Spicer 📂 Article 📅 1990 🏛 Elsevier Science 🌐 English ⚖ 881 KB

Three-Dimensional Magnetic Structures Ge

Three-Dimensional Magnetic Structures Generated by the Development of the Filamentation (Weibel) Instability in the Relativistic Regime

✍ Califano, F.; Del Sarto, D.; Pegoraro, F. 📂 Article 📅 2006 🏛 The American Physical Society 🌐 English ⚖ 370 KB

Three-Dimensional Magnetic Reconnection

Three-Dimensional Magnetic Reconnection in Astrophysical Plasmas - MHD Approach

✍ A. Otto 📂 Article 📅 1998 🏛 Springer Netherlands 🌐 English ⚖ 366 KB

Instability in three-dimensional, unstea

Instability in three-dimensional, unsteady, stenotic flows

✍ Francois Mallinger; Dimitris Drikakis 📂 Article 📅 2002 🏛 Elsevier Science 🌐 English ⚖ 536 KB

The paper presents a computational investigation of instabilities in pulsatile flow through a three-dimensional stenosis. The computations have been conducted using a third-order high-resolution scheme and a non-linear multigrid algorithm. The simulations reveal the existence of unstable flow throug