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Learning Module 2.1
Interaction of EMR with Earth's Atmosphere and Surfaces

Introduction

Sun

The Sun is the primary source of electromagnetic radiation measured in remote sensing techniques. In the previous section, we learned that the Sun radiates electromagnetic energy over a wide range of wavelengths and emits the most radiation in the visible portion of the spectrum. Before the electromagnetic energy from the Sun reaches the Earth’s surface, it must pass through the atmosphere. As the energy passes through the atmosphere, it interacts with the molecules and particles present in the atmosphere. Once it reaches the Earth's surface this energy can be reflected, absorbed or transmitted. In this section we will learn about how the atmosphere and the surfaces on the Earth interact with EMR and how this is fundamental to remote sensing.

Learning Outcomes

Readings

Presentations and Content

Lab 3

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