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Solar Flares and CMEs Overview

Solar Flares and CMEs Overview

Assessment

Interactive Video

Physics

9th - 10th Grade

Practice Problem

Hard

Created by

Patricia Brown

FREE Resource

The video tutorial discusses solar flares and coronal mass ejections (CMEs), explaining their characteristics and impacts. Solar flares are bursts of electromagnetic radiation from the sun, while CMEs involve large-scale ejections of plasma. Both phenomena can affect Earth, causing auroras and disrupting technology. The video also covers the classification of solar flares, highlighting the potential dangers of high-intensity flares.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What are solar flares primarily composed of?

Plasma and electromagnetic radiation

Solid particles

Carbon dioxide

Water vapor

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the difference between a filament and a prominence?

Filaments are bright, prominences are dark

Filaments are on Earth, prominences are on the sun

Filaments are gaseous, prominences are solid

Filaments are dark against the sun, prominences are visible against space

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a coronal mass ejection (CME)?

A small solar flare

A large explosion of plasma from the sun

A minor solar event

A type of solar wind

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How do CMEs affect Earth's magnetic field?

They have no effect

They strengthen it

They can cause magnetic storms

They make it disappear

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What natural phenomenon can be caused by particles from CMEs interacting with Earth's atmosphere?

Volcanic eruptions

Tornadoes

Auroras

Earthquakes

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What was a significant impact of the 1989 solar storm in North America?

Widespread power outages

Massive earthquakes

Increased temperatures

Severe flooding

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How are solar flares classified?

By their duration

By letter, indicating intensity

By their color

By their size

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