✦ LIBER ✦

On the magnetization of solar convective zones

✍ Scribed by Yu. V. Vandakurov

Book ID: 119979760
Publisher: SP MAIK Nauka/Interperiodica
Year: 1999
Tongue: English
Weight: 63 KB
Volume: 25
Category: Article
ISSN: 1063-7850
DOI: 10.1134/1.1262501

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Limits on the magnetic field strength at

Limits on the magnetic field strength at the base of the solar convection zone

✍ Sydney D'Silva; Robert F. Howard 📂 Article 📅 1993 🏛 Springer 🌐 English ⚖ 439 KB

The magnetic field transfer in the solar

The magnetic field transfer in the solar convective zone

✍ A. A. Ruzmaikin; S. I. Vainshtein 📂 Article 📅 1978 🏛 Springer Netherlands 🌐 English ⚖ 352 KB

Magnetization and nature of the rotation

Magnetization and nature of the rotation of the solar convective zone

✍ Yu. V. Vandakurov 📂 Article 📅 1999 🏛 SP MAIK Nauka/Interperiodica 🌐 English ⚖ 47 KB

Commentary on a putative magnetic field

Commentary on a putative magnetic field variation in the solar convection zone

✍ Gough, D. O. 📂 Article 📅 2013 🏛 John Wiley and Sons 🌐 English ⚖ 401 KB

Dynamical behavior of strong magnetic fi

Dynamical behavior of strong magnetic fields in the solar convection zone

✍ S. Vainshtein; E. H. Levy 📂 Article 📅 1991 🏛 Springer 🌐 English ⚖ 644 KB

Magnetic buoyancy is thought to play an important role in the dynamical behavior of the Sun's magnetic field in the convection zone. Magnetic buoyancy is commonly thought to cause inescapable rapid loss of toroidal flux from much of the convection zone, thereby suppressing effective operation of a s

A model of the solar convection zone

✍ H. C. Spruit 📂 Article 📅 1974 🏛 Springer 🌐 English ⚖ 745 KB

A model of the convection zone is presented which matches an empirical model atmosphere (HSRA) and an interior model. A mixing length formalism containing four adjustable parameters is used. Thermodynamical considerations provide limits on two of these parameters. The average temperature-pressure re