Sun's Magnetic Field and Plasma Dynamics

Sun's Magnetic Field and Plasma Dynamics

Assessment

Interactive Video

Physics

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video explores the magnetic nature of the Sun, starting with the concept of plasma, a charged gas formed when atoms lose electrons. It explains how the Sun's differential rotation affects its magnetic field, leading to the creation of sunspots. The tachocline, a boundary layer within the Sun, is identified as a key area for magnetic field generation. As the magnetic field becomes buoyant, it rises to the surface, forming visible sunspots.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary component of the Sun's magnetic field?

Ionized gases or plasma

Solid iron core

Carbon dioxide

Liquid water

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What happens to an atom when it becomes a plasma?

It becomes a solid

It loses or gains electrons

It turns into a liquid

It gains additional protons

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Where can plasmas be found naturally on Earth?

In the ocean

In the Earth's core

In glaciers

In the atmosphere during lightning strikes

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does the Sun's rotation vary?

It does not rotate

It rotates faster at the equator

It rotates faster at the poles

It rotates at the same speed everywhere

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is created when electrons travel in a circle?

A gravitational field

A magnetic field

A sound wave

A light beam

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the tachocline?

A layer of the Earth's atmosphere

A region in the Earth's core

A boundary layer in the Sun

A type of solar flare

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does the Sun's magnetic field reach its surface?

Through solar winds

By gravitational pull

By becoming magnetically buoyant

Through convection currents

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