The Earth's magnetic field is essential for protecting our planet from charged particles originating from the solar wind. These particles, often referred to as cosmic rays, are deflected and trapped by the Earth's magnetic field, forming what are known as radiation belts.
As these charged particles follow the Earth's magnetic field lines, they tend to accumulate near the poles. This accumulation leads to a higher concentration of particles at the poles compared to the equator.
This phenomenon, known as the auroral ovals, is where the charged particles interact with the Earth's atmosphere, producing the Northern and Southern Lights, also known as auroras.
List- I (Layer of atmosphere) | List- II (Approximate height over earth's surface) | ||
A. | F1-Layer | I. | 10 km |
B. | D-Layer | II. | 170-190 km |
C. | Troposphere | III. | 100 km |
D. | E-layer | IV. | 65-75 km |