The Ionosphere.
The area around the poles.
The area extending from 80km above the eart's surface to the edge of the atmosphere--the second-most outer layer, second only to the exosphere. Here free electrons can exist for short periods of time before they are captured by a nearby positive ion. The existence of charged particles at this altitude and above, signals the beginning of the ionosphere a region having the properties of a gas and of a plasma.
If the sun's rays hit the Earth's surface at a direct spot, which is usually around the equator, that area would be the warmest. Any area that is far away from the sun's rays is usually cold.
If the sun's rays hit the Earth's surface at a direct spot, which is usually around the equator, that area would be the warmest. Any area that is far away from the sun's rays is usually cold.
The illustration that represents the largest reservoir of nitrogen on earth should display the atmosphere. The atmosphere of earth contains around 78.09 % nitrogen.
The Aurora.
Van Allen belts
The magnetosphere, an area of charged particles that interact with the solar wind.
Such areas are called Van Allen belts.
No. Charged particles come closest to Earth at the poles. This is because the Earth's magnetosphere has magnetic field lines that are generated from and reenter the poles. As such, the area near the equator is most protected by the magnetosphere, as it extends outward from the poles, surrounding the Earth. And the magnetosphere is weakest at the points of intersection at the poles. When charged particles are deflected by the magnetosphere, they follow these magnetic field lines, and reenter our atmosphere at the poles. High-energy radiation generated by these charged particles interacting with gases in the atmosphere is the reason for the auroras (Northern and Southern lights). This is why, subsequent to a solar flare that sends a strong wind of particles toward the Earth, you are likely to see more intense auroras. Because of the nature of fusion (which makes the sun what it is, as an active star), the most common particles composing the solar wind are: neutrinos (neutral particles, very small masses), electrons (negatively charged, often easily deflected by the magnetosphere), and protons (positively charged, the largest danger to us from the solar wind, because they counter the charge of the magnetosphere and reenter our atmosphere most easily).
Auroras have no definite size. They occur when charged particles from the Sun ionize particles in the upper atmosphere as they spiral in toward Earth's magnetic field. Auroras may be localized in one area, or may extend from horizon to horizon in the sky.
Neils Bohr, in 1913. He depicted an atom as a small area of positively charged particles in the middle and electrons circulating this in orbits around the outside.
The area around the poles.
A.) magnetic north and south poles B.) north magnetic pole C.) north pole D.) north and south poles E.) south magnetic pole these are the options ^^
electric field
This is called diffusion, but it is a purely statistical process - randomly moving particles have a higher probability of spreading from an area of high concentration to an area of low concentration than the other way around, simply because there are more of them in the area of high concentration.
because the surface area of the larger particles propels them faster which has a recipical effect on the water around the particles