Solar irradiance variations and nonlinear mean field dynamo

N. Kleeorin; I. Rogachevskii; A. Ruzmaikin

doi:10.1007/BF00680592

Solar irradiance variations and nonlinear mean field dynamo

N. Kleeorin, I. Rogachevskii, A. Ruzmaikin

Department of Mechanical Engineering

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19 Scopus citations

Abstract

By using a nonlinear model of an axisymmetric α - Ω dynamo, an analytical expression which gives the magnitude of the mean magnetic field as a function of rotation and other parameters for a solar-type convective zone is obtained. The mean magnetic field varies as the {Mathematical expression} power of the rotation rate. The resulting theoretical relationship of the X-ray luminosity as a function of the angular velocity is in agreement with observations by Fleming, Gioia, and Maccacaro (1989).

Original language	English
Pages (from-to)	223-234
Number of pages	12
Journal	Solar Physics
Volume	155
Issue number	2
DOIs	https://doi.org/10.1007/BF00680592
State	Published - 1 Dec 1994

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1007/BF00680592

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title = "Solar irradiance variations and nonlinear mean field dynamo",

abstract = "By using a nonlinear model of an axisymmetric α - Ω dynamo, an analytical expression which gives the magnitude of the mean magnetic field as a function of rotation and other parameters for a solar-type convective zone is obtained. The mean magnetic field varies as the \{Mathematical expression\} power of the rotation rate. The resulting theoretical relationship of the X-ray luminosity as a function of the angular velocity is in agreement with observations by Fleming, Gioia, and Maccacaro (1989).",

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

year = "1994",

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doi = "10.1007/BF00680592",

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pages = "223--234",

journal = "Solar Physics",

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T1 - Solar irradiance variations and nonlinear mean field dynamo

AU - Kleeorin, N.

AU - Rogachevskii, I.

AU - Ruzmaikin, A.

PY - 1994/12/1

Y1 - 1994/12/1

N2 - By using a nonlinear model of an axisymmetric α - Ω dynamo, an analytical expression which gives the magnitude of the mean magnetic field as a function of rotation and other parameters for a solar-type convective zone is obtained. The mean magnetic field varies as the {Mathematical expression} power of the rotation rate. The resulting theoretical relationship of the X-ray luminosity as a function of the angular velocity is in agreement with observations by Fleming, Gioia, and Maccacaro (1989).

AB - By using a nonlinear model of an axisymmetric α - Ω dynamo, an analytical expression which gives the magnitude of the mean magnetic field as a function of rotation and other parameters for a solar-type convective zone is obtained. The mean magnetic field varies as the {Mathematical expression} power of the rotation rate. The resulting theoretical relationship of the X-ray luminosity as a function of the angular velocity is in agreement with observations by Fleming, Gioia, and Maccacaro (1989).

UR - https://www.scopus.com/pages/publications/0006888487

U2 - 10.1007/BF00680592

DO - 10.1007/BF00680592

M3 - Article

AN - SCOPUS:0006888487

SN - 0038-0938

VL - 155

SP - 223

EP - 234

JO - Solar Physics

JF - Solar Physics

IS - 2

ER -

Solar irradiance variations and nonlinear mean field dynamo

Abstract

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