A Case Study on Statistical Analysis of Geomagnetic Storm 3-5 August 2010

Zehra Can; Hasan Şafak Erdağ

Makale detayları

A Case Study on Statistical Analysis of Geomagnetic Storm 3-5 August 2010

Yazarlar:

Zehra Can | Hasan Şafak Erdağ

Yayıncı:

Istanbul University

Ana Başlıklar:

Klasik Fizik (Diğer)

Dergi:

Physics and Astronomy Reports Vol.2 Issue 2, pp.83-87

Belge Tipi:

Makale

Yayın Tarihi:

12/2024

Belge Dili:

İngilizce

Document ID (Org No.):

2001340630

pISSN:

2980-3012

Anahtar kelimeler:

Özet:

 The solar flare that occurred on August 1, 2010, was a powerful event that led to the interaction of two coronal mass ejections CMEs, resulting in a significant CME-CME eruption. This eruption struck Earth on August 3, causing a major geomagnetic storm that had widespread impacts on Earths magnetic environment. Detecting geomagnetic storms is essential for safeguarding space missions, satellite operations, and communications systems. Failure to accurately predict these storms can disrupt critical infrastructure. The CME-CME interaction in August 2010 differs from ordinary CMEs in terms of particle velocity and density, which were observed to reach unprecedented levels during this event.In this study, a statistical model using the multiple linear regression method was developed to examine the effects of CME-CME interaction on Earths magnetic field by utilizing charac teristics such as particle velocity  and density . The study evaluated the effects of solar parameters during G3 and G2-level geomagnetic storms. It was found that particle density significantly increases the intensity and duration of geomagnetic storms, whereas particle velocity notably reduces these effects, exhibiting an opposing influence.

 The solar flare that occurred on August 1, 2010, was a powerful event that led to the interaction of two coronal mass ejections CMEs, resulting in a significant CME-CME eruption. This eruption struck Earth on August 3, causing a major geomagnetic storm that had widespread impacts on Earths magnetic environment. Detecting geomagnetic storms is essential for safeguarding space missions, satellite operations, and communications systems. Failure to accurately predict these storms can disrupt critical infrastructure. The CME-CME interaction in August 2010 differs from ordinary CMEs in terms of particle velocity and density, which were observed to reach unprecedented levels during this event.In this study, a statistical model using the multiple linear regression method was developed to examine the effects of CME-CME interaction on Earths magnetic field by utilizing charac teristics such as particle velocity  and density . The study evaluated the effects of solar parameters during G3 and G2-level geomagnetic storms. It was found that particle density significantly increases the intensity and duration of geomagnetic storms, whereas particle velocity notably reduces these effects, exhibiting an opposing influence.

 The solar flare that occurred on August 1, 2010, was a powerful event that led to the interaction of two coronal mass ejections CMEs, resulting in a significant CME-CME eruption. This eruption struck Earth on August 3, causing a major geomagnetic storm that had widespread impacts on Earths magnetic environment. Detecting geomagnetic storms is essential for safeguarding space missions, satellite operations, and communications systems. Failure to accurately predict these storms can disrupt critical infrastructure. The CME-CME interaction in August 2010 differs from ordinary CMEs in terms of particle velocity and density, which were observed to reach unprecedented levels during this event.In this study, a statistical model using the multiple linear regression method was developed to examine the effects of CME-CME interaction on Earths magnetic field by utilizing charac teristics such as particle velocity  and density . The study evaluated the effects of solar parameters during G3 and G2-level geomagnetic storms. It was found that particle density significantly increases the intensity and duration of geomagnetic storms, whereas particle velocity notably reduces these effects, exhibiting an opposing influence.

 The solar flare that occurred on August 1, 2010, was a powerful event that led to the interaction of two coronal mass ejections CMEs, resulting in a significant CME-CME eruption. This eruption struck Earth on August 3, causing a major geomagnetic storm that had widespread impacts on Earths magnetic environment. Detecting geomagnetic storms is essential for safeguarding space missions, satellite operations, and communications systems. Failure to accurately predict these storms can disrupt critical infrastructure. The CME-CME interaction in August 2010 differs from ordinary CMEs in terms of particle velocity and density, which were observed to reach unprecedented levels during this event.In this study, a statistical model using the multiple linear regression method was developed to examine the effects of CME-CME interaction on Earths magnetic field by utilizing charac teristics such as particle velocity  and density . The study evaluated the effects of solar parameters during G3 and G2-level geomagnetic storms. It was found that particle density significantly increases the intensity and duration of geomagnetic storms, whereas particle velocity notably reduces these effects, exhibiting an opposing influence.

Makale detayları

A Case Study on Statistical Analysis of Geomagnetic Storm 3-5 August 2010

Yazarlar:

Zehra Can | Hasan Şafak Erdağ

Yayıncı:

Istanbul University

Ana Başlıklar:

Klasik Fizik (Diğer)

Dergi:

Physics and Astronomy Reports Vol.2 Issue 2, pp.83-87

Belge Tipi:

Makale

Yayın Tarihi:

12/2024

Belge Dili:

İngilizce

Document ID (Org No.):

2001340630

pISSN:

2980-3012

Geomagnetic storm

coronal mass ejection

CME-CME interaction

regression

statistical analysis

space weather

Sayı

Makale detayları

A Case Study on Statistical Analysis of Geomagnetic Storm 3-5 August 2010

Yazarlar: Zehra Can | Hasan Şafak Erdağ

Yayıncı: Istanbul University

Ana Başlıklar: Klasik Fizik (Diğer)

Dergi: Physics and Astronomy Reports Vol.2 Issue 2, pp.83-87

Belge Tipi: Makale

Yayın Tarihi: 12/2024

Belge Dili: İngilizce

Document ID (Org No.): 2001340630

pISSN: 2980-3012

Geomagnetic storm

coronal mass ejection

CME-CME interaction

regression

statistical analysis

space weather

Sayı

Yazarlar:

Zehra Can | Hasan Şafak Erdağ

Yayıncı:

Istanbul University

Ana Başlıklar:

Klasik Fizik (Diğer)

Dergi:

Physics and Astronomy Reports Vol.2 Issue 2, pp.83-87

Belge Tipi:

Makale

Yayın Tarihi:

12/2024

Belge Dili:

İngilizce

Document ID (Org No.):

2001340630

pISSN:

2980-3012