Solar Wind and Magnetosphere

<p>The air pressure is lower at higher altitudes, allowing the charged particles to move more freely and interact with atmospheric molecules. (C)</p> Signup and view all the answers

<p>Thermosphere (D)</p> Signup and view all the answers

<p>The different types of gases in the atmosphere interact differently with the charged particles from the Sun, producing different colors. (D)</p> Signup and view all the answers

<p>Charged particles, including protons and electrons. (A)</p> Signup and view all the answers

<p>Northern Quebec is closer to the North Pole, where magnetic field lines are more concentrated. (D)</p> Signup and view all the answers

A stream of charged particles constantly released from the Sun's surface.

A protective shield surrounding Earth, created by Earth's magnetic field, that deflects harmful solar wind.

The colorful light display caused by solar wind particles colliding with Earth's atmosphere.

Aurora borealis, meaning "northern dawn", is the name given to polar auroras in the Northern Hemisphere.

Aurora australis, meaning "southern dawn", is the name given to polar auroras in the Southern Hemisphere.

The layer of Earth's atmosphere where polar auroras occur, above 90 km.

The stronger the solar activity, the more solar wind particles are released, increasing the chance of seeing auroras.

The magnetosphere funnels the solar wind particles towards the poles, where they collide with the atmosphere, creating auroras.