Natural processes cycle carbon dioxide through the atmosphere. The burning of fossil fuels increases the concentration of carbon dioxide above historic levels.
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"Greenhouse gases" help to regulate the Earth's temperature. When out of natural balance, they restrict the reflection of infrared energy back into space, trapping heat in the atmosphere. View animation
The maximum velocity of hurricanes is restricted by natural limits of vertical temperature gradient, evaporation, friction, and heat transfer of sea spray. View animation
Air moves toward low-pressure regions and away from high-pressure regions. The Coriolis force deflects these air masses in opposite directions around high and lows. View image
When conditional instability exists, air parcels are stable if they are dry and unstable if they are saturated. Conditional instability can help to generate storms by causing parcels of moist air to rise and form towering clouds. View image
The Coriolis force is created by Earth's rotation, which deflects air masses as they move over long distances. It is strongest near the poles and nonexistent at the equator. View image
Cirrus clouds permit most of the sunlight that reaches them to pass through to Earth's surface, while thicker cumulus clouds reflect much of the sunlight that strikes them back into space. Both types block some of the heat radiating from Earth, warming the planet's surface. View image
Differential heating of Earth produces distinct patterns of rising and descending air masses, winds, and storms in well-defined cells around the globe. View image
Geostrophic flow is more common in the upper atmosphere than at the surface, where friction between air and land slows the movement of air parcels. View image
Hurricane wind speeds range from 74 miles per hour (the minimum for a Category 1 storm on the Saffir/Simpson scale) to more than 155 miles per hour for Category 5 storms. View image
CO2 is the most important anthropogenic greenhouse gas, but other gases also make significant contributions to climate change. Other pollutants, such as fine particulates, also affect how much solar radiation is retained in Earth's atmosphere. View image
Under current conditions bicarbonate is the most abundant form of CO2. All three forms are important for biological processes carried out by marine organisms. The green arrows in this diagram show the range of pH (7.5 to 8.5) that is likely to be found in the oceans now and in the future. View image
Sea breezes are caused by temperature differences between land at the surface and adjoining water, which cause air to flow in opposite directions during the day and at night. View image
Atmospheric pressure decreases exponentially as altitude increases, while temperature rises with altitude in some layers and decreases in others. View image
The Sun is much hotter than Earth, so it emits radiation at shorter wavelengths. The solar spectrum x 10-6 applies at the surface of the Sun, not at Earth's orbit. Solar energy flux is lower by a factor of 50,000 at Earth's orbit. View image
Carbon cycles constantly between land, oceans, and the atmosphere, although its residence time in various reservoirs can vary greatly. Black arrows in this image show natural fluxes and red arrows show anthropogenic contributions. View image
Sinking air near high-pressure systems inhibits the formation of clouds, so highs are associated with clear, dry weather. Rising air near low-pressure systems produces clouds and rain. View image