✦ LIBER ✦

Numerical MHD simulation of interplanetary shock pairs

✍ Scribed by Steinolfson, Richard S.; Dryer, Murray; Nakagawa, Yoshinari

Book ID: 119711927
Publisher: American Geophysical Union
Year: 1975
Tongue: English
Weight: 782 KB
Volume: 80
Category: Article
ISSN: 0148-0227
DOI: 10.1029/ja080i010p01223

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Numerical MHD modeling of propagation of

Numerical MHD modeling of propagation of interplanetary shock through the magnetosheath

✍ Samsonov, A. A.; Němeček, Z.; Šafránková, J. 📂 Article 📅 2006 🏛 American Geophysical Union 🌐 English ⚖ 437 KB

Numerical simulation of MHD shock waves

Numerical simulation of MHD shock waves in the solar wind

✍ Steinolfson, Richard S.; Dryer, Murray 📂 Article 📅 1978 🏛 American Geophysical Union 🌐 English ⚖ 651 KB

MHD simulations of solar and interplanet

MHD simulations of solar and interplanetary phenomena

✍ M. Dryer 📂 Article 📅 1996 🏛 Springer Netherlands 🌐 English ⚖ 522 KB

MHD simulation for the interaction of an

MHD simulation for the interaction of an interplanetary shock with the Earth's magnetosphere

✍ Samsonov, A. A.; Sibeck, D. G.; Imber, J. 📂 Article 📅 2007 🏛 American Geophysical Union 🌐 English ⚖ 394 KB

Numerical simulations of MHD dynamos

✍ Daniel O. Gómez; Pablo Mininni 📂 Article 📅 2005 🏛 Elsevier Science 🌐 English ⚖ 272 KB

Numerical simulations of MHD turbulence

✍ A. Pouquet 📂 Article 📅 1988 🏛 Elsevier Science 🌐 English ⚖ 489 KB

Several results using numerical experimentation on homogeneous three-dimensional turbulent MHD flows are reviewed. The role (or absence thereof) of chaos and that of kinetic helicity for the kinematic dynamo problem is described. A second topic concerns the formation of large scale coherent structur