The atmosphere is a protective gaseous mantle held bound to the Earth by gravitational attraction, extending several thousand kilometers into space. Pure dry air near sea level possesses a remarkably uniform chemical composition:
Based on temperature lapse rates and molecular dynamics, the atmosphere is structured into five concentric thermal layers:
- 1. Troposphere (ক্ষুব্ধমণ্ডল): Lowest layer directly in contact with Earth's surface. Extends up to $18 ext{ km}$ at the equator (due to intense thermal convection) and $8 ext{ km}$ at the poles (mean height $pprox 12 ext{ km}$). Contains over $75\%$ of atmospheric mass and virtually $99\%$ of atmospheric water vapor. Characterized by the Normal Lapse Rate, where temperature decreases steadily with elevation at a rate of $6.5^\circ ext{C}$ per $1,000 ext{ m}$ ($1^\circ ext{C}$ per $165 ext{ m}$). The boundary capping the troposphere is the Tropopause, where temperature drops to $-80^\circ ext{C}$ at the equator and $-45^\circ ext{C}$ at the poles.
- 2. Stratosphere (শান্তমণ্ডল): Extends from the tropopause up to $50 ext{ km}$. Temperature remains isothermal (constant at $-56^\circ ext{C}$) in its lower part, but progressively increases upward to $0^\circ ext{C}$ at the Stratopause. This temperature inversion is caused by the Ozonosphere ($15–35 ext{ km}$), where ozone ($O_3$) molecules absorb lethal solar ultraviolet radiation (UV-B and UV-C) via the Chapman mechanism ($O_2 + h u o O + O$; $O + O_2 o O_3$). The complete absence of turbulent convection, clouds, and water vapor makes the lower stratosphere ideal for long-range supersonic jet aviation.
- 3. Mesosphere (মেসোস্ফিয়ার): Extends from $50 ext{ km}$ to $80 ext{ km}$. Temperature drops sharply with height, reaching approximately $-100^\circ ext{C}$ at the Mesopause, representing the coldest thermal zone in the planetary envelope. Incoming interplanetary meteoroids burn up here due to frictional ablation. Noctilucent (night-shining) ice-crystal clouds occasionally form in polar summer mesopause regions.
- 4. Thermosphere / Ionosphere (আয়নোস্ফিয়ার): Extends from $80 ext{ km}$ to $400 ext{ km}$. Intensely heated by shortwave solar X-rays and extreme UV, temperature rises rapidly exceeding $1,500^\circ ext{C}$, though the air is so rarefied that sensible heat transfer is negligible. Solar radiation ionizes gas molecules, forming stratified electrical conductibility layers:
- D-Layer ($80–99 ext{ km}$): Absorbs medium and high-frequency radio waves; disappears at night.
- E-Layer / Kennelly-Heaviside Layer ($99–150 ext{ km}$): Reflects medium radio waves back to Earth.
- F-Layer / Appleton Layer ($150–400 ext{ km}$): Reflects short radio waves for global communication.
- Auroral Phenomena: High-energy solar wind protons and electrons trapped in Earth's geomagnetic field collide with nitrogen and oxygen atoms, generating luminous ethereal displays: Aurora Borealis (Northern Lights) and Aurora Australis (Southern Lights).
- 5. Exosphere & Magnetosphere (চৌম্বকমণ্ডল): Outermost tenuous boundary extending from $400 ext{ km}$ to $10,000 ext{ km}$, gradually merging into the interplanetary solar plasma. Dominated by ultra-light hydrogen and helium atoms. Beyond lies the Magnetosphere with the Van Allen Radiation Belts shielding the biosphere from deadly cosmic ray bombardment.