Earth: An Introduction to Physical Geology (12th Edition)

Published by Pearson
ISBN 10: 0134074254
ISBN 13: 978-0-13407-425-2

Chapter 21 - Section 21.4 - Heating the Atmosphere - Concept Checks - Page 644: 1

Answer

Incoming solar radiation follows three main paths when it interacts with the Earth's atmosphere: absorption, reflection, and scattering. Absorption: Some of the solar radiation is absorbed by the atmosphere's gases, such as water vapor, carbon dioxide, ozone, and other trace gases. This absorbed energy warms the atmosphere, contributing to its temperature and energy balance. Reflection: A portion of the incoming solar radiation is reflected back into space by clouds, aerosols, and the Earth's surface itself. This reflection, known as albedo, varies depending on the surface characteristics. For example, snow and ice have high albedo, reflecting more sunlight, while dark surfaces, like forests or oceans, have lower albedo, absorbing more sunlight. Scattering: Particles and molecules in the atmosphere scatter solar radiation in various directions. Rayleigh scattering, which occurs when solar radiation interacts with air molecules, leads to the blue color of the sky. Mie scattering, caused by larger particles like water droplets and dust, contributes to the scattering of sunlight, especially in the lower atmosphere. The percentage of solar radiation taking each path can vary due to several factors. For instance, cloud cover plays a significant role in altering the balance of absorption and reflection. On cloudy days, more solar radiation is reflected back into space by the clouds, reducing the amount of energy reaching the Earth's surface and subsequently affecting temperatures.

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