macdoc
Philosopher
Climate science fundamentals
http://www.ipcc.unibe.ch/publications/wg1-ar4/faq/wg1_faq-1.3.html
http://www.ipcc.unibe.ch/publications/wg1-ar4/faq/wg1_faq-1.3.html
http://www.ipcc.unibe.ch/publications/wg1-ar4/faq/wg1_faq-1.3.html
continuesFrequently Asked Question 1.3
What is the Greenhouse Effect?
The Sun powers Earth’s climate, radiating energy at very short wavelengths, predominately in the visible or near-visible (e.g., ultraviolet) part of the spectrum. Roughly one-third of the solar energy that reaches the top of Earth’s atmosphere is reflected directly back to space. The remaining two-thirds is absorbed by the surface and, to a lesser extent, by the atmosphere. To balance the absorbed incoming energy, the Earth must, on average, radiate the same amount of energy back to space. Because the Earth is much colder than the Sun, it radiates at much longer wavelengths, primarily in the infrared part of the spectrum (see Figure 1). Much of this thermal radiation emitted by the land and ocean is absorbed by the atmosphere, including clouds, and reradiated back to Earth. This is called the greenhouse effect. The glass walls in a greenhouse reduce airflow and increase the temperature of the air inside. Analogously, but through a different physical process, the Earth’s greenhouse effect warms the surface of the planet.
http://www.ipcc.unibe.ch/publications/wg1-ar4/faq/wg1_faq-1.3.html
