Relationship between Solar Flux and Sunspot Activity Using Several Regression Models

Ruben Cornelius Siagian, L. Alfaris, G. Ahmad, Nazish Laeiq, Aldi Cahya Muhammad, Ukta Indra Nyuswantoro, Budiman Nasution
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Abstract

This study examines the correlation and prediction between sunspots and solar flux, two closely related factors associated with solar activity, covering the period from 2005 to 2022. The study utilizes a combination of linear regression analysis and the ARIMA prediction method to analyze the relationship between these factors and forecast their values. The analysis results reveal a significant positive correlation between sunspots and solar flux. Additionally, the ARIMA prediction method suggests that the SARIMA model can effectively forecast the values of both sunspots and solar flux for a 12-period timeframe. However, it is essential to note that this study solely focuses on correlation analysis and does not establish a causal relationship. Nonetheless, the findings contribute valuable insights into future variations in solar flux and sunspot numbers, thereby aiding scientists in comprehending and predicting solar activity's potential impact on Earth. The study recommends further research to explore additional factors that may influence the relationship between sunspots and solar flux, extend the research period to enhance the accuracy of solar activity predictions and investigate alternative prediction methods to improve the precision of forecasts.
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太阳通量与黑子活动的几种回归模型关系
本文研究了2005年至2022年期间太阳黑子与太阳通量这两个与太阳活动密切相关的因素之间的相关性和预测。本研究采用线性回归分析与ARIMA预测方法相结合的方法,分析这些因素之间的关系并预测其值。分析结果表明,太阳黑子与太阳通量之间存在显著的正相关关系。此外,ARIMA预测方法表明,SARIMA模式可以有效地预测太阳黑子和太阳通量在12周期内的数值。然而,需要注意的是,本研究仅侧重于相关性分析,并未建立因果关系。尽管如此,这些发现对太阳通量和太阳黑子数量的未来变化提供了有价值的见解,从而帮助科学家理解和预测太阳活动对地球的潜在影响。该研究建议进一步研究可能影响太阳黑子与太阳通量之间关系的其他因素,延长研究周期以提高太阳活动预测的准确性,并研究替代预测方法以提高预测精度。
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审稿时长
6 weeks
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