Time series analysis of long term full disk observations of the Mn i 539.4 nm solar line

The equivalent width and central depth data of Mn 539.4 nm solar spectral line, observed in the period from 1979 to 1992 at Kitt Peak Observatory, was analyzed in pursuit for periodic changes. As the observations are highly unevenly sampled, test if the periods really exist in the observed data was...

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Bibliographic Details
Main Authors: Danilović Sanja, Vince Ištvan I., Vitas Nikola D., Jovanović Predrag P.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2005-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2005/1450-698X0570079D.pdf
Description
Summary:The equivalent width and central depth data of Mn 539.4 nm solar spectral line, observed in the period from 1979 to 1992 at Kitt Peak Observatory, was analyzed in pursuit for periodic changes. As the observations are highly unevenly sampled, test if the periods really exist in the observed data was needed. Two different methods for spectral analysis were applied to synthesized data sampled in the same way as observations. Comparation of these results with results obtained from the observed data showed that the parameters display at least three periodic changes with the periods of: 11years, quasi-biannual and 27 days. .
ISSN:1450-698X
1820-9289