Solar Energy and Heating the Atmosphere Radiation Energy

Solar Energy and Heating the Atmosphere

Radiation Energy comes from the sun as radiant energy Radiation from the Sun can be visible (light) or invisible (infrared, UV, etc. )

Radiation – energy that travels as waves or rays through space between objects and materials ex. Sun radiates energy to Earth Campfire radiates energy to your hands

Radiation When radiant energy strikes a molecule in sand, soil, water, or air, the molecule gains energy and begins to move faster. In other words, the molecule absorbed radiant energy.

Heat While Temperature is a measure of the average kinetic energy of the molecules in a sample of matter, Heat is the sum of all the energy from the molecules in a sample of matter. For example, while a candle flame and bonfire have the same temperature, the bonfire creates more heat because more molecules are moving!

Differential Heating – different materials heat up at different rates For example, this accounts for the difference in temperature of water and soil after they have both been in the lamp light for the same length of time.

Conduction – energy transfer between molecules when they come in contact with each other

Convection – transfer of energy from one place to another in a gas or liquid via a current

Putting it all Together How does energy transfer via radiation, conduction, and convection heat the atmosphere?

Radiation, Conduction, & Convection Energy Transfer

Re-radiation

Heating the Atmosphere 1. Radiation from Sun absorbed by surface 2 a. Surface reradiates energy to the air 2 b. Surface conducts energy to air molecules 3. Air molecules conduct energy to other air molecules, resulting in convection currents