TED-Ed: How epic solar winds make brilliant polar lights - Michael Molina

The video explains the journey of polar lights, known as auroras, from the sun to Earth. It describes how high-energy particles from the sun form solar wind, which is diverted by Earth's magnetosphere. When overwhelmed by coronal mass ejections, particles reach Earth's atmosphere, creating auroras through interactions with oxygen and nitrogen atoms. The video also provides tips for viewing auroras, emphasizing the importance of clear nights and understanding solar activity.

What is the velocity at which matter is blasted from the sun?

Describe the process that leads to the creation of the northern and southern lights.

What role does the magnetosphere play in the journey of solar particles?

Explain what happens during a coronal mass ejection.

How do the colors of the auroras depend on the type of atom involved?