Comparison of the QBO and F10.7 Solar Flux Effects on Total Mass Density
- 作者: Selçuk Sağır 1, Ramazan Atıcı 2
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隶属关系:
- Department of Electronic and Automation, Technical Sciences Vocational School, Mus Alparslan University,
- Faculty of Education, Mus Alparslan University
- 期: 卷 58, 编号 7 (2018)
- 页面: 841-845
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157002
- DOI: https://doi.org/10.1134/S0016793218070186
- ID: 157002
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详细
The comparison of the Quasi Biennial Oscillation (QBO) and F10.7 solar flux effects on Total Mass Density (TMD) obtained from NRLMSIS-00 model for 90 km altitude of ionosphere known as Mesosphere-Lower Thermosphere (MLT) region was made statistically. In the results of calculations, it was observed that QBO and F10.7 solar flux have an effect on TMD. It was determined that about 69% of the variations in TMD could be explained by F10.7 and QBO. Also, it was seen that an increase/a decrease of 1 meter per second occurred in QBO gave rise to an increase/a decrease of 2.36 × 10–9 kg/m3 in TMD while an increase/a decrease of 1 s.f.u. in F10.7 gave rise to a decrease/increase of 1.02 × 10–9 kg/m3 in TMD. Based on these results, it was observed that the effects of stratospheric QBO, which is one of the meteorological processes, and F10.7, which is one of the indicators of the solar processes, were nearly at the same rate on TMD of MLT region. Furthermore, the results show that the stratospheric QBO may be a suitable candidate for increasing the anomalous density reductions observed in TMD.
作者简介
Selçuk Sağır
Department of Electronic and Automation, Technical Sciences Vocational School,Mus Alparslan University,
编辑信件的主要联系方式.
Email: s.sagir@alparslan.edu.tr
土耳其, Mus, 49100
Ramazan Atıcı
Faculty of Education, Mus Alparslan University
Email: s.sagir@alparslan.edu.tr
土耳其, Mus, 49250
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