Possible solar cycle variations in the convection zone

Preprint

26 January 2000

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0001444

Abstract

Using data from the Global Oscillations Network Group (GONG) that covers the period from 1995 to 1998 we study the change in frequencies of solar oscillations with solar activity. From these frequencies we attempt to determine any possible variation in solar structure with solar activity. We do not find any evidence of a change in the convection zone depth or extent of overshoot below the convection zone during the solar cycle.

Keywords

SOLAR OSCILLATIONS
CYCLE VARIATIONS
SOLAR STRUCTURE
CONVECTION ZONE
SOLAR ACTIVITY
FREQUENCIES
SOLAR CYCLE
ZONE USING

All Related Versions

Version 1, 2000-01-26, ArXiv
Published version: Solar Physics, 192 (1/2), 449.

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