— Ch. 1 · Defining Climate Systems —
Climate variability and change.
~5 min read · Ch. 1 of 7
The sun provides nearly all energy to Earth's climate system. This energy radiates back into outer space as heat. The balance between incoming solar radiation and outgoing thermal radiation is called the Earth's energy budget. When more energy enters than leaves, the planet warms. If more energy escapes than arrives, global temperatures drop. Long-term averages of weather patterns define a region's climate. Variations in these patterns lasting decades or longer constitute climate change. Individual weather events do not count toward this definition. Scientists distinguish natural internal variability from external forcing mechanisms. Internal processes include shifts in ocean currents and atmospheric circulation. External drivers involve changes in solar output or volcanic eruptions. The Intergovernmental Panel on Climate Change uses these distinctions to classify causes.
Natural Forcing Mechanisms
Ocean basins like the Pacific exhibit decadal oscillations that redistribute heat globally. The El Niño, Southern Oscillation cycle repeats every two to seven years. During warm phases, tropical sea surface temperatures rise across the eastern Pacific. Cold phases known as La Niña cool equatorial waters off South America. These cycles influence rainfall patterns and storm tracks worldwide. Volcanic eruptions inject sulfur dioxide into the stratosphere. Large explosions create sulfate aerosols that reflect sunlight away from Earth. The 1991 eruption of Mount Pinatubo lowered global temperatures by about 0.5 degrees Celsius for three years. Solar output varies over an eleven-year cycle. Sunspot numbers track these fluctuations in intensity. Changes in Earth's orbital tilt alter seasonal sunlight distribution. Milankovitch cycles describe these kinematic variations affecting glacial periods. Plate tectonics reconfigure continents over millions of years. This reshaping alters ocean circulation and regional climate patterns.