Magnitude of the Dynamo-generated Magnetic-field in Solar-type Convective Zones

N Kleeorin; I Rogachevskii; A Ruzmaikin

Magnitude of the Dynamo-generated Magnetic-field in Solar-type Convective Zones

Department of Mechanical Engineering

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	159-167
Number of pages	9
Journal	Astronomy and Astrophysics
Volume	297
Issue number	1
State	Published - May 1995

Keywords

Mhd
Stars, magnetic fields
Sun, magnetic fields
Sun, x-rays
Turbulence

Cite this

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title = "Magnitude of the Dynamo-generated Magnetic-field in Solar-type Convective Zones",

keywords = "Mhd, Stars, magnetic fields, Sun, magnetic fields, Sun, x-rays, Turbulence",

author = "N Kleeorin and I Rogachevskii and A Ruzmaikin",

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month = may,

language = "English",

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journal = "Astronomy and Astrophysics",

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T1 - Magnitude of the Dynamo-generated Magnetic-field in Solar-type Convective Zones

AU - Kleeorin, N

AU - Rogachevskii, I

AU - Ruzmaikin, A

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KW - Sun, magnetic fields

KW - Sun, x-rays

KW - Turbulence

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M3 - Article

SN - 0004-6361

VL - 297

SP - 159

EP - 167

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 1

ER -

Magnitude of the Dynamo-generated Magnetic-field in Solar-type Convective Zones

Keywords

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Cite this