Sensitivity of Global Oscillation Frequencies to Solar Activity on Short Timescales
Abstract Sun’s oscillations frequencies vary with the changing magnetic activity and hold a strong positive correlation. While most of the analysis for global modes have been carried out using time series longer than a solar rotation, only a few studies are available showing their variation on short...
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Published in | Research notes of the AAS Vol. 8; no. 10; pp. 264 - 263 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
The American Astronomical Society
15.10.2024
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Subjects | |
Online Access | Get full text |
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Summary: | Abstract Sun’s oscillations frequencies vary with the changing magnetic activity and hold a strong positive correlation. While most of the analysis for global modes have been carried out using time series longer than a solar rotation, only a few studies are available showing their variation on shorter timescales. Using Doppler observations from Global Oscillation Network Group during the period 1995–2024, we analyze oscillation frequencies computed on a timescale of nine days and compare them with those obtained from 108 days. We also study their sensitivity in cycles 23 and 24 to the change in solar activity as represented by the 10.7 cm radio flux. |
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Bibliography: | AAS58814 The Sun and the Heliosphere |
ISSN: | 2515-5172 2515-5172 |
DOI: | 10.3847/2515-5172/ad85e8 |