A5073086731- Solar and Space Plasma Dynamics
- Solar Radiation and Photovoltaics
- Stellar, planetary, and galactic studies
- Astronomy and Astrophysical Research
- Linguistic, Cultural, and Literary Studies
- Families in Therapy and Culture
- Gamma-ray bursts and supernovae
- Cultural and Sociopolitical Studies
- Turkish Literature and Culture
- Historical Astronomy and Related Studies
- Islamic Thought and Society Studies
- Educational Methods and Analysis
- Education Practices and Challenges
- Historical Turkish Studies
- Monetary Policy and Economic Impact
- Market Dynamics and Volatility
- Astrophysics and Star Formation Studies
- Ionosphere and magnetosphere dynamics
- Geophysics and Gravity Measurements
- Music Education and Analysis
- Data Mining and Machine Learning Applications
Çanakkale Onsekiz Mart Üniversitesi
2019-2023
The presence of pulsating stars in eclipsing binary systems (EBs) makes these objects significant since they allow us to investigate the stellar interior structure and evolution. Different types could be found EBs such as Delta Scuti variables. have been known for decades increasing number is important understanding pulsational structure. Hence, this study, a research was carried out on southern TESS field discover new EBs. We produced an algorithm search detached semi-detached considering...
ABSTRACT Eclipsing binaries with (a) pulsating component(s) are remarkable objects to investigate the evolution and structure of stellar systems. Detailed studies such systems also important reveal their pulsation properties. The largest sample eclipsing is one containing δ Scuti variables. In this study, we present a comprehensive spectroscopic photometric study three systems, GQ Dra, RR Lep, TYC 683-640-1. Their orbital parameters were derived from large-amplitude radial velocity...
This study aims to develop artificial neural networks predict the physical parameters of shock waves in interplanetary (IP) environment which are closely correlated sunspot number as demonstrated previous studies [1] and [2]. is done by training ANNs with current available data then use model for years where there no present. For this purpose, NASA's Advanced Composition Explorer (ACE) WIND spacecrafts used obtain calculated using Cavus2013 hydrodynamical model. These describe properties IP...
ABSTRACT Although the source active regions of some coronal mass ejections (CMEs) were identified in CME catalogues, vast majority CMEs do not have an region. We propose a method that uses filtration process and machine learning to identify sunspot groups associated with large fraction compare physical parameters these properties their corresponding find mechanisms behind initiation CMEs. These taken from Coordinated Data Analysis Workshops (CDAW) data base hosted at NASA’s website. The...
The presence of pulsating stars in eclipsing binary systems (EBs) makes these objects significant since they allow us to investigate the stellar interior structure and evolution. Different types could be found EBs such as Delta Scuti variables. have been known for decades increasing number is important understanding pulsational structure. Hence, this study, a research was carried out on southern TESS field discover new EBs. We produced an algorithm search detached semi-detached considering...
We present the time series analysis of GS UMa.GS UMa is a suspected δ Scuti variable with primary frequency 6.0987 d -1 .