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Simultaneous evaluation of solar activity proxies during geomagnetic storms using principal component analysis: Case study of the African low and mid-latitude regions

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F25%3A00618933" target="_blank" >RIV/68378289:_____/25:00618933 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.sciencedirect.com/science/article/pii/S1364682625000616" target="_blank" >https://www.sciencedirect.com/science/article/pii/S1364682625000616</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.jastp.2025.106477" target="_blank" >10.1016/j.jastp.2025.106477</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Simultaneous evaluation of solar activity proxies during geomagnetic storms using principal component analysis: Case study of the African low and mid-latitude regions

  • Original language description

    We simultaneously evaluate the contributions of the mostly used solar activity indices to the modelling of geomagnetic storms using principal component analysis (PCA). The selected indices are the sunspot number (SSN), solar radio flux at a wavelength of 10.7 cm (F10.7), 12-month running average of SSN (R12), 81-day running average of F10.7 (F10.781), and the modified F10.7 index herein referred to as F10.7p. The assessment of these indices was accomplished by first developing five storm-time empirical models of the ionosphere with ionospheric total electron content (TEC) as dependent variable, and each of the five solar proxies as the independent variable. As the energy from the Sun differs from one latitudinal region to another on Earth, two locations at different latitudes were considered for the analysis. Based on their long data coverage periods, Hartebeesthoek (HRAO, geographic coordinates: 25.89 degrees S, 27.69 degrees E, geomagnetic coordinates: 36.32 degrees S, 94.69 degrees E), South Africa, and Mbarara (MBAR, geographic coordinates: 0.60 degrees S and 30.74 degrees E, geomagnetic coordinates: 10.22 degrees S and 102.36 degrees E), Uganda, were chosen to represent the middle and low latitude ionospheric regions, respectively. Their data coverage periods are 27 September 1996 to 30 March 2024 (HRAO) and 17 July 2001 to 30 March 2024 (MBAR) and only storm-time TEC data within these periods selected based on the criterion Dst <=50 nT or Kp >= 4 were considered for the statistical analysis. Through PCA decomposition, TEC data were broken up into a matrix of principal directions of the maximum variances in the dataset (or matrix of eigenvectors of the covariance matrix) and a matrix of principal components (PCs) which represent the projection of data onto the principal directions. For each model, PCs were thereafter modelled in terms of the corresponding solar activity index and the modelled quantities were further combined with the original PC vectors to get the reconstructed TEC for the entire period of the study. With reference to the ionospheric storm-time model implemented using SSN as solar activity representation, a statistical analysis revealed that, overall, the storm-time empirical models developed using either F10.7, F10.781, R12, or F10.7p, perform about 8%, 15%, 18%, 22%, respectively, better in reconstructing actual TEC than the SSN based model for HRAO, and 11%, 23%, 19%, 24% for MBAR. Validating the models over selected four storms, results showed that running average based indices led to more accurate TEC predictions compared to the usual daily Wolf's SSN and F10.7.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10509 - Meteorology and atmospheric sciences

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Journal of Atmospheric and Solar-Terrestrial Physics

  • ISSN

    1364-6826

  • e-ISSN

    1879-1824

  • Volume of the periodical

    270

  • Issue of the periodical within the volume

    May

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    11

  • Pages from-to

    106477

  • UT code for WoS article

    001457638800001

  • EID of the result in the Scopus database

    2-s2.0-105001007096