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Journals / Turkish Journal of Astronomy and Astrophysics / 2023 / Cilt: 4 Sayı: 3 Özel Sayı

Relationship between Cycle 24 Solar Flares and Coronal Mass Ejections

24. Çevrim Güneş Parlamaları ile Koronal Kütle Atımları İlişkisi

Hasret Atasoy(İSTANBUL ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ)0000-0003-4089-3491
Zahide Funda Bostancı Güver(İSTANBUL ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ)0000-0002-5665-3452
Pages
447–452
Publication Date
2023-12-31
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AI Summary & Key Takeaways

AI Insight
⚡ TL;DR(Too Long; Didn't Read)

In this study, the statistical relationship and results between the solar flares observed with the GOES satellite and the coronal mass ejections observed with the SOHO/LASCO satellite during the Solar Cycle 24 will be discussed.

📌 3 Key Takeaways

🎯
Objective & Hypothesis:Solar flare is the sudden release of enormous energy stored in magnetic fields associated with active regions due to the heating of plasma in the Sun's atmosphere, while Coronal Mass Ejection is the ejection of atmospheric plasma into interplanetary space.
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Key Findings & Data:Therefore, CSHKP (Carmichael (1964), Sturrock (1966), Hirayama (1974), Kopp & Pneuman (1976)) flare model is based on magnetic reconnection and it is thought that CME formation may occur close to the flare formation process.
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Conclusion & Impact:In this study, the statistical relationship and results between the solar flares observed with the GOES satellite and the coronal mass ejections observed with the SOHO/LASCO satellite during the Solar Cycle 24 will be discussed.
🔬Design:Modeling & Simulation
📍Scope:Comprehensive Sample
⚙️Variables:Sun · solar flares · CME

Abstract

Solar flare is the sudden release of enormous energy stored in magnetic fields associated with active regions due to the heating of plasma in the Sun's atmosphere, while Coronal Mass Ejection is the ejection of atmospheric plasma into interplanetary space. Both events are thought to be different manifestations of the same process that releases magnetic energy stored in the Sun's atmosphere. Therefore, CSHKP (Carmichael (1964), Sturrock (1966), Hirayama (1974), Kopp & Pneuman (1976)) flare model is based on magnetic reconnection and it is thought that CME formation may occur close to the flare formation process. In this study, the statistical relationship and results between the solar flares observed with the GOES satellite and the coronal mass ejections observed with the SOHO/LASCO satellite during the Solar Cycle 24 will be discussed.

Özet

Güneş parlaması, Güneş atmosferinde plazma ısınmasına bağlı olarak aktif bölgeler ile ilişkili manyetik alanlarda depolanan muazzam bir enerjinin aniden serbest kalması, Koronal Kütle Atımı ise atmosferik plazmanın gezegenler arası boşluğa püskürülmesidir. Her iki olayında Güneş atmosferinde depolanan manyetik enerjiyi serbest bırakan aynı sürecin farklı tezahürleri olduğu düşünülmektedir. Bu nedenle CSHKP (Carmichael (1964), Sturrock (1966), Hirayama (1974), Kopp & Pneuman (1976)) parlama modeli manyetik yeniden birleşmeyi temel alarak CME oluşumu parlamanın oluşum sürecine yakın zamanlarda meydana gelebileceği düşünülmektedir.Bu çalışmada 24. Güneş Leke Çevrimi boyunca, GOES uydusuyla gözlenen Güneş parlamaları ile SOHO/LASCO uydusuyla gözlenen koronal kütle atımları arasındaki istatistiksel ilişkisi ve sonuçları tartışılacaktır.

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Cite This Article

Atasoy, H., Güver, Z. F. B. (2023). Relationship between Cycle 24 Solar Flares and Coronal Mass Ejections. Turkish Journal of Astronomy and Astrophysics, Cilt: 4 Sayı: 3 Özel Sayı, 447–452. https://doi.org/10.55064/tjaa.1203786

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