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Cophasal regions on the Sun

Journal Article:

Abstract

The subsequent development of the phenomenological model of the solar convective zone is carried out. The cophasal region, in which unilateral movement of the matter is supposed, is considered. Quantitative relations for kinematic parameters of solar sport groups, agreeing well with the observations, are given. The cophasal regions distribution due to their linear dimensions is obtained. It is shown that the effective depth of the convective zone is found to change with the phase of the activity cycle: less in the minimum and more in the maximum of activity.
Authors:
Kozhevnikov, N I [1] 
  1. Moskovskij Gosudarstvennyj Univ. (USSR). Gosudarstvennyj Astronomicheskij Inst. ''GAISh''
Publication Date:
Jan 01, 1977
Product Type:
Journal Article
Reference Number:
AIX-09-409786; EDB-79-015140
Resource Relation:
Journal Name: Astron. Zh.; (USSR); Journal Volume: 54:6
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; SUN; CONVECTION; COMPARATIVE EVALUATIONS; DEPTH; SOLAR ACTIVITY; SPATIAL DISTRIBUTION; STAR MODELS; SUNSPOTS; TIME DEPENDENCE; VELOCITY; DIMENSIONS; DISTRIBUTION; MAIN SEQUENCE STARS; MATHEMATICAL MODELS; STARS; 640104* - Astrophysics & Cosmology- Solar Phenomena
OSTI ID:
6567971
Country of Origin:
USSR
Language:
Russian
Other Identifying Numbers:
Journal ID: CODEN: ASZHA
Submitting Site:
INIS
Size:
Pages: 1325-1334
Announcement Date:

Journal Article:

Citation Formats

Kozhevnikov, N I. Cophasal regions on the Sun. USSR: N. p., 1977. Web.
Kozhevnikov, N I. Cophasal regions on the Sun. USSR.
Kozhevnikov, N I. 1977. "Cophasal regions on the Sun." USSR.
@misc{etde_6567971,
title = {Cophasal regions on the Sun}
author = {Kozhevnikov, N I}
abstractNote = {The subsequent development of the phenomenological model of the solar convective zone is carried out. The cophasal region, in which unilateral movement of the matter is supposed, is considered. Quantitative relations for kinematic parameters of solar sport groups, agreeing well with the observations, are given. The cophasal regions distribution due to their linear dimensions is obtained. It is shown that the effective depth of the convective zone is found to change with the phase of the activity cycle: less in the minimum and more in the maximum of activity.}
journal = {Astron. Zh.; (USSR)}
volume = {54:6}
journal type = {AC}
place = {USSR}
year = {1977}
month = {Jan}
}