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The middle atmosphere is an important region of the Earth's atmosphere and plays very important role in deciphering atmospheric dynamics.
Also, the effect of the outer belt electron sink on the chemistry of the middle atmosphere is introduced.
The thermal regime of the middle atmosphere is determined to a great extent by the balance between the incoming solar and outgoing infrared radiation.
During the solar eclipse, the absorption of ultraviolet radiation by ozone that heats the middle atmosphere is cut off in the shadow region.
A new analytical approach for CR ionization by protons and nuclei with charge Z in the lower ionosphere and middle atmosphere is developed in this paper.
For example, the wintertime Arctic middle atmosphere is characterised by the presence of large amplitude planetary Rossby waves that often interact with the stratospheric polar vortex and trigger sudden stratospheric warming (SSW) events (Chandran et al. 2013).
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Computations for cosmic ray ionization in the middle atmosphere are made.
The equatorial middle atmosphere was poorly studied compared with the number of observations made at mid- and high latitudes.
The basic characteristics of these long period oscillations and their effect on the middle atmosphere are known to some extent.
The effects of galactic and solar cosmic rays (CR) in the middle atmosphere are considered in this work.
Some conclusions concerning seasonal, solar activity and long-term variations in the vertical structure of the middle atmosphere are elaborated.
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