Physical Science 101
Solar Interactions
Energy
The capacity to do work.
Common forms of energy include:
Kinetic Energy:
Potential Energy:
Thermodynamics
The study of the behavior of heat and heat transfer.
Heat always flows from warmer areas to cooler areas
T
hermal energy flows from areas of higher energy to areas of lower energy
Heat is transferred by:
Incoming Solar Radiation
Radiation transmitted by the Sun and received on Earth:
Earth only receives radiation from the Sun on one half of the sphere.
9% ultraviolet radiation
41% visible radiation
50% infrared radiation
Outgoing Radiation: Earth into Space
Approximately 1/3 of all incoming radiation is reflected directly back into space.
Visible, IR and UV radiation are absorbed by Earth, reemitted as infrared radiation.
Radiation is lost to space on both the night side and day side of the sphere.
Three major dips in the outgoing radiation curve occur.
What's Missing?
Heat Budget
Global Radiation Balance: The amount of incoming solar radiation equals the amount of outgoing radiation.
Changes in the amounts of incoming radiation vs. outgoing radiation can have dramatic effects on the global climate.
Incoming Solar Radiation
What happens to solar radiation?
Absorption:
Transmission:
Redirection:
Radiation Pathways
Incoming Radiation
Outgoing Radiation
Net Radiation
The Global Energy Balance is a global average.
Radiation is only received on one half of the globe.
Energy is being lost on all parts of the globe.
Equatorial regions receive more radiation than polar regions.
Polar regions loose more radiation than they receive.
Excess energy from the equator must be moved to the polar regions.