{"title":"Solar activity and ionospheric variation: A comprehensive study using hurst exponent and probability density functions analysis","authors":"Mahdi Momeni , Yenca Migoya-Orué","doi":"10.1016/j.asr.2025.02.060","DOIUrl":null,"url":null,"abstract":"<div><div>This study analyzes the ionospheric dynamics during the solar maximum of 2014 and the solar minimum of 2019, focusing on Vertical Total Electron Content (vTEC) and key solar and geomagnetic indices, including SYM-H, X-ray flux, and Extreme Ultraviolet (EUV) irradiance. By employing the Hurst exponent and Probability Density Function (PDF) analysis, we quantify the persistence and correlation properties of ionospheric fluctuations under varying solar conditions. The Hurst exponent reveals significant long-range correlations in vTEC, indicating a high level of persistence, particularly during solar minimum. In contrast, solar maximum conditions exhibit more unstable behavior across all indices, with lower Hurst values suggesting enhanced short-term irregularities. PDF analysis shows leptokurtic distributions, highlighting the prevalence of extreme events, especially during heightened solar activity. Our findings underscore the complex interplay between solar activity and ionospheric behavior, providing valuable insights for improving predictive models related to space weather impacts on communication and navigation systems.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"75 10","pages":"Pages 7668-7683"},"PeriodicalIF":2.8000,"publicationDate":"2025-03-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advances in Space Research","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0273117725001954","RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
This study analyzes the ionospheric dynamics during the solar maximum of 2014 and the solar minimum of 2019, focusing on Vertical Total Electron Content (vTEC) and key solar and geomagnetic indices, including SYM-H, X-ray flux, and Extreme Ultraviolet (EUV) irradiance. By employing the Hurst exponent and Probability Density Function (PDF) analysis, we quantify the persistence and correlation properties of ionospheric fluctuations under varying solar conditions. The Hurst exponent reveals significant long-range correlations in vTEC, indicating a high level of persistence, particularly during solar minimum. In contrast, solar maximum conditions exhibit more unstable behavior across all indices, with lower Hurst values suggesting enhanced short-term irregularities. PDF analysis shows leptokurtic distributions, highlighting the prevalence of extreme events, especially during heightened solar activity. Our findings underscore the complex interplay between solar activity and ionospheric behavior, providing valuable insights for improving predictive models related to space weather impacts on communication and navigation systems.
期刊介绍:
The COSPAR publication Advances in Space Research (ASR) is an open journal covering all areas of space research including: space studies of the Earth''s surface, meteorology, climate, the Earth-Moon system, planets and small bodies of the solar system, upper atmospheres, ionospheres and magnetospheres of the Earth and planets including reference atmospheres, space plasmas in the solar system, astrophysics from space, materials sciences in space, fundamental physics in space, space debris, space weather, Earth observations of space phenomena, etc.
NB: Please note that manuscripts related to life sciences as related to space are no more accepted for submission to Advances in Space Research. Such manuscripts should now be submitted to the new COSPAR Journal Life Sciences in Space Research (LSSR).
All submissions are reviewed by two scientists in the field. COSPAR is an interdisciplinary scientific organization concerned with the progress of space research on an international scale. Operating under the rules of ICSU, COSPAR ignores political considerations and considers all questions solely from the scientific viewpoint.