Solar Physics paper

Solar Physics paper | Research Square window.SnipcartSettings = { analytics: { enabled: false } }; (function() { var accessVector = localStorage.getItem('access_vector') || ''; window.dataLayer = window.dataLayer || []; if (accessVector) { window.dataLayer.push({ user: { profile: { profileInfo: { snid: accessVector } } } }); } })(); (function(w,d,s,l,i){w[l]=w[l]||[];w[l].push({'gtm.start':new Date().getTime(),event:'gtm.js'});var f=d.getElementsByTagName(s)[0],j=d.createElement(s),dl=l!='dataLayer'?'&l='+l:'';j.async=true;j.src='https://www.googletagmanager.com/gtm.js?id='+i+dl;f.parentNode.insertBefore(j,f);})(window,document,'script','dataLayer','GTM-K279D39R'); Browse Preprints In Review Journals COVID-19 Preprints AJE Video Bytes Research Tools Research Promotion AJE Professional Editing AJE Rubriq About Preprint Platform In Review Editorial Policies Our Team Advisory Board Help Center Sign In Submit a Preprint Cite Share Download PDF Research Article Solar Physics paper NOUR ABDULAMEER, habeeb allawi, Balazs ujvari This is a preprint; it has not been peer reviewed by a journal. https://doi.org/ 10.21203/rs.3.rs-3920803/v1 This work is licensed under a CC BY 4.0 License Status: Posted Version 1 posted You are reading this latest preprint version Abstract This study examines the complex relationships among high-energy solar particle events (SEPs), solar flares, and coronal mass ejections (CMEs) at the onset of Solar Cycle 25. We investigate the sources and characteristics of high-energy solar particles and explore the dynamics of solar flares and CMEs within this evolving solar cycle. While CMEs are often associated with SEPs, their occurrence isn't guaranteed due to the intricate interplay of magnetic fields and propagation conditions. Understanding this variability is crucial for improving predictive capabilities related to space weather events. We leverage advanced observational techniques to analyze CMEs and assess their correlations with solar cycle activity. Our research also considers the potential impacts of these solar events on Earth's space weather and technology infrastructure. Comparisons with previous solar cycles provide valuable insights into the evolving nature of solar activity. We conclude by discussing the current state of predictive modeling and forecasting, emphasizing the need for continued advancements in space weather prediction models. Overall, this study contributes to our understanding of solar physics and space weather, particularly regarding the dynamics of high-energy solar particle events and their relationships with flares and CMEs during Solar Cycle 25's early stages. Solar Cycle 25 High-energy solar particle events (SEPs) Solar flares Coronal Mass Ejections (CMEs) Space weather Solar activity Sunspots Particle acceleration Space weather impacts Solar physics Forecasting and prediction models Electromagnetic radiation Solar dynamics Solar wind. Full Text Additional Declarations No competing interests reported. Cite Share Download PDF Status: Posted Version 1 posted You are reading this latest preprint version Research Square lets you share your work early, gain feedback from the community, and start making changes to your manuscript prior to peer review in a journal. As a division of Research Square Company, we’re committed to making research communication faster, fairer, and more useful. We do this by developing innovative software and high quality services for the global research community. Our growing team is made up of researchers and industry professionals working together to solve the most critical problems facing scientific publishing. Also discoverable on Platform About Our Team In Review Editorial Policies Advisory Board Help Center Resources Author Services Accessibility API Access RSS feed Manage Cookie Preferences © Research Square 2026 | ISSN 2693-5015 (online) Privacy Policy Terms of Service Do Not Sell My Personal Information {"props":{"pageProps":{"initialData":{"identity":"rs-3920803","acceptedTermsAndConditions":true,"allowDirectSubmit":true,"archivedVersions":[],"articleType":"Research Article","associatedPublications":[],"authors":[{"id":270758786,"identity":"ed9e3d54-c0cf-4398-b3e9-00a03fec8e5f","order_by":0,"name":"NOUR ABDULAMEER","email":"data:image/png;base64,iVBORw0KGgoAAAANSUhEUgAAAZAAAAAyAQMAAABI0h/eAAAABlBMVEX///8AAABVwtN+AAAACXBIWXMAAA7EAAAOxAGVKw4bAAAA7klEQVRIiWNgGAWjYNCCCgkexvbmgw8+ANls7ERpOWMjw9xzLNlwBkgLMzE6GNvSbNhn5JhJ84B4hLSYi509uoGB7TAPb88BM2mbX9vk+ZgZGD98zMGtxXJ2XtoNBp7DPJLtDcnWuX23DduYGZglZ27DrcXgdo7ZDQaJwzyGPQcO3s7tuc0I1MLGzEtQi8FhHvsbiQ3Slj237YnUkpDGwzgjmUma4cftROK0JByw4WHsOcZs2NtwO7mNmbGZsF8+/pOwZ2zv//jgx5/btvOBcfrhIx4tYJAAYzC2gckGAupRwB9SFI+CUTAKRsFIAQCAU1PfI8DZhAAAAABJRU5ErkJggg==","orcid":"","institution":"University of Debrecen","correspondingAuthor":true,"prefix":"","firstName":"NOUR","middleName":"","lastName":"ABDULAMEER","suffix":""},{"id":270758787,"identity":"2b447742-23de-416e-9a8c-5c447fe54da3","order_by":1,"name":"habeeb allawi","email":"","orcid":"","institution":"University of Dhi Qar","correspondingAuthor":false,"prefix":"","firstName":"habeeb","middleName":"","lastName":"allawi","suffix":""},{"id":270758788,"identity":"11a8c584-ec32-4d01-9925-59895eb5b3ce","order_by":2,"name":"Balazs ujvari","email":"","orcid":"","institution":"University of Debrecen","correspondingAuthor":false,"prefix":"","firstName":"Balazs","middleName":"","lastName":"ujvari","suffix":""}],"badges":[],"createdAt":"2024-02-02 12:14:47","currentVersionCode":1,"declarations":"","doi":"10.21203/rs.3.rs-3920803/v1","doiUrl":"https://doi.org/10.21203/rs.3.rs-3920803/v1","draftVersion":[],"editorialEvents":[],"editorialNote":"","failedWorkflow":false,"files":[{"id":54386604,"identity":"1296ff18-51e8-4c70-ba93-5d0626e2f070","added_by":"auto","created_at":"2024-04-09 17:53:41","extension":"pdf","order_by":1,"title":"","display":"","copyAsset":false,"role":"manuscript-pdf","size":627031,"visible":true,"origin":"","legend":"","description":"","filename":"SolarPhysicspaper1.pdf","url":"https://assets-eu.researchsquare.com/files/rs-3920803/v1_covered_e3288bfc-a294-4303-be88-af3ac21dfde4.pdf"}],"financialInterests":"No competing interests reported.","formattedTitle":"Solar Physics paper","fulltext":[],"fulltextSource":"","fullText":"","funders":[],"hasAdminPriorityOnWorkflow":false,"hasManuscriptDocX":false,"hasOptedInToPreprint":true,"hasPassedJournalQc":"","hasAnyPriority":false,"hideJournal":true,"highlight":"","institution":"","isAcceptedByJournal":false,"isAuthorSuppliedPdf":true,"isDeskRejected":"","isHiddenFromSearch":false,"isInQc":false,"isInWorkflow":false,"isPdf":true,"isPdfUpToDate":true,"isWithdrawnOrRetracted":false,"journal":{"display":true,"email":"[email protected]","identity":"researchsquare","isNatureJournal":false,"hasQc":true,"allowDirectSubmit":true,"externalIdentity":"","sideBox":"","snPcode":"","submissionUrl":"/submission","title":"Research Square","twitterHandle":"researchsquare","acdcEnabled":true,"dfaEnabled":false,"editorialSystem":"","reportingPortfolio":"","inReviewEnabled":false,"inReviewRevisionsEnabled":true},"keywords":"Solar Cycle 25, High-energy solar particle events (SEPs), Solar flares, Coronal Mass Ejections (CMEs), Space weather, Solar activity, Sunspots, Particle acceleration, Space weather impacts, Solar physics, Forecasting and prediction models, Electromagnetic radiation, Solar dynamics, Solar wind.","lastPublishedDoi":"10.21203/rs.3.rs-3920803/v1","lastPublishedDoiUrl":"https://doi.org/10.21203/rs.3.rs-3920803/v1","license":{"name":"CC BY 4.0","url":"https://creativecommons.org/licenses/by/4.0/"},"manuscriptAbstract":"\u003cp\u003eThis study examines the complex relationships among high-energy solar particle events (SEPs), solar flares, and coronal mass ejections (CMEs) at the onset of Solar Cycle 25. We investigate the sources and characteristics of high-energy solar particles and explore the dynamics of solar flares and CMEs within this evolving solar cycle.\u0026nbsp;\u003c/p\u003e\n\u003cp\u003eWhile CMEs are often associated with SEPs, their occurrence isn't guaranteed due to the intricate interplay of magnetic fields and propagation conditions. Understanding this variability is crucial for improving predictive capabilities related to space weather events.\u0026nbsp;\u003c/p\u003e\n\u003cp\u003eWe leverage advanced observational techniques to analyze CMEs and assess their correlations with solar cycle activity. Our research also considers the potential impacts of these solar events on Earth's space weather and technology infrastructure.\u0026nbsp;\u003c/p\u003e\n\u003cp\u003eComparisons with previous solar cycles provide valuable insights into the evolving nature of solar activity. 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