An early prediction of 25th solar cycle using Hurst exponent

被引:0
|
作者
A. K. Singh
Asheesh Bhargawa
机构
[1] University of Lucknow,Department of Physics
来源
关键词
The Sun; Solar activity; Hurst exponent; Sunspot numbers; F10.7 cm radio flux;
D O I
暂无
中图分类号
学科分类号
摘要
The analysis of long memory processes in solar activity, space weather and other geophysical phenomena has been a major issue even after the availability of enough data. We have examined the data of various solar parameters like sunspot numbers, 10.7 cm radio flux, solar magnetic field, proton flux and Alfven Mach number observed for the year 1976–2016. We have done the statistical test for persistence of solar activity based on the value of Hurst exponent (H\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$H$\end{document}) which is one of the most classical applied methods known as rescaled range analysis. We have discussed the efficiency of this methodology as well as prediction content for next solar cycle based on long term memory. In the present study, Hurst exponent analysis has been used to investigate the persistence of above mentioned (five) solar activity parameters and a simplex projection analysis has been used to predict the ascension time and the maximum number of counts for 25th solar cycle. For available dataset of the year 1976–2016, we have calculated H=0.86\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$H = 0.86$\end{document} and 0.82 for sunspot number and 10.7 cm radio flux respectively. Further we have calculated maximum number of counts for sunspot numbers and F10.7 cm index as 102.8±24.6\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$102.8\pm 24.6$\end{document} and 137.25±8.9\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$137.25\pm 8.9$\end{document} respectively. Using the simplex projection analysis, we have forecasted that the solar cycle 25th would start in the year 2021 (January) and would last up to the year 2031 (September) with its maxima in June 2024.
引用
收藏
相关论文
共 50 条
  • [11] An early prediction of the maximum amplitude of the solar cycle 25
    Helal, Hamid R.
    Galal, A. A.
    [J]. JOURNAL OF ADVANCED RESEARCH, 2013, 4 (03) : 275 - 278
  • [12] Predicting the 25th solar cycle using deep learning methods based on sunspot area data
    Li, Qiang
    Wan, Miao
    Zeng, Shu-Guang
    Zheng, Sheng
    Deng, Lin-Hua
    [J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2021, 21 (07)
  • [13] Predicting indices of the ionosphere response to solar activity for the ascending phase of the 25th solar cycle
    Gulyaeva, T. L.
    [J]. ADVANCES IN SPACE RESEARCH, 2019, 63 (05) : 1588 - 1595
  • [14] Predicting the 25th solar cycle using deep learning methods based on sunspot area data
    Qiang Li
    Miao Wan
    Shu-Guang Zeng
    Sheng Zheng
    Lin-Hua Deng
    [J]. Research in Astronomy and Astrophysics, 2021, 21 (07) : 292 - 300
  • [15] A Catalog of Geoefficient Flare Events of the Current 25th Solar Cycle in a Modern Presentation
    Zabarinskaya, L. P.
    Ishkov, V. N.
    Sergeeva, N. A.
    [J]. COSMIC RESEARCH, 2023, 61 (06) : 487 - 490
  • [16] A Catalog of Geoefficient Flare Events of the Current 25th Solar Cycle in a Modern Presentation
    L. P. Zabarinskaya
    V. N. Ishkov
    N. A. Sergeeva
    [J]. Cosmic Research, 2023, 61 : 487 - 490
  • [17] Solar Cycle 25 prediction
    不详
    [J]. WEATHER, 2020, 75 (03) : 71 - 71
  • [18] Forecast of Modulation of Cosmic Rays with Rigidity of 10 GV in the 25th Solar Activity Cycle
    Yanke, V. G.
    Belov, A. V.
    Gushchina, R. T.
    Kobelev, P. G.
    Trefilova, L. A.
    [J]. GEOMAGNETISM AND AERONOMY, 2024, 64 (02) : 201 - 210
  • [19] The Forbush decrease observed by the SEVAN particle detector network in the 25th solar activity cycle
    Karapetyan, T.
    Chilingarian, A.
    Hovsepyan, G.
    Martoyan, H.
    Sargsyan, B.
    Langer, R.
    Chum, J.
    Nikolova, N.
    Angelov, Hristo
    Haas, Diana
    Knapp, Johannes
    Walter, Michael
    Ploc, Ondrej
    Slegl, Jakub
    Kakona, Martin
    Ambrozova, Iva
    [J]. JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2024, 262
  • [20] Solar Cycle Pairing and Prediction of Cycle 25
    Nagovitsyn, Y. A.
    Ivanov, V. G.
    [J]. SOLAR PHYSICS, 2023, 298 (03)