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This work contributes immensely to current understanding of solar eclipses most especially total solar eclipses, it origin, and reveal a quite difference ionospheric behavior at different period of solar X-ray flare classes production during total eclipse in middle latitude ionosonde station situated along the path of totality of eclipse. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially obscuring Earth's view of the Sun. This configuration can only occur during a new moon, when the Sun and Moon are aligned as seen from the Earth. This phenomena and on ionosphere F2 are reveals.…mehr

Produktbeschreibung
This work contributes immensely to current understanding of solar eclipses most especially total solar eclipses, it origin, and reveal a quite difference ionospheric behavior at different period of solar X-ray flare classes production during total eclipse in middle latitude ionosonde station situated along the path of totality of eclipse. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially obscuring Earth's view of the Sun. This configuration can only occur during a new moon, when the Sun and Moon are aligned as seen from the Earth. This phenomena and on ionosphere F2 are reveals.
Autorenporträt
Adekoya Bolarinwa John received is B.Sc. and M.Sc degree in Physics (physic with Electronics option) and (Atmospheric Physics option) from Olabisi Onabanjo University, Ago-Iwoye, Ogun-state, Nigeria, in 2008 and 2011 respectively. He is currently doing is PhD in Physics (Atmospheric Physics option. He is an Assistant Lecturer at the same University