Earth's Energy Budget

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Across
  1. 5. A boundary separating two masses of air with different densities, typically associated with weather changes such as temperature shifts, precipitation, and wind patterns.
  2. 7. The second layer of the atmosphere, which contains most of the ozone in Earth’s atmosphere.
  3. 10. Variation or cycle that occurs daily, such as temperature or solar radiation changes between day and night
  4. 14. A molecule consisting of 3 oxygen atoms found primarily in the stratosphere. When created in the troposphere, it can be a harmful pollutant.
  5. 15. Half of the Earth, usually divided into Northern and Southern by the equator or Eastern and Western by the prime meridian.
  6. 16. Electromagnetic radiation emitted by the Sun that includes visible light and ultraviolet radiation, contributing to Earth's energy balance.
  7. 17. The lowest layer of the atmosphere extending from the surface to an altitude between 8 kilometers (at the poles) and 14 kilometers (in the tropics); most weather occurs in this layer.
  8. 19. Collections of water (in liquid or ice phase) in the atmosphere that are often classified by their shape and height.
  9. 20. The heat energy transferred between the Earth's surface and the atmosphere that causes a change in temperature without changing the phase of a substance.
  10. 22. The combined energy transfer from evaporation of water from the surface and transpiration of water by plants growing on that surface.
  11. 26. The amount of water vapor present in the air, often expressed as a percentage of the maximum amount of water vapor that the air can hold at a given temperature.
  12. 27. The mixture of gases that surrounds the Earth and some other planets. Biogeochemical processes, including human activities, determine the concentrations of the gaseous constituents of this
  13. 28. The rate of change of atmospheric properties, such as temperature, pressure, or humidity, over a specified distance, often influencing wind patterns and weather systems.
  14. 29. The redirection of light in all directions due to interactions with air molecules, aerosols, or clouds.
Down
  1. 1. An abbreviated term for incoming solar radiation.
  2. 2. The transfer of heat energy vertically through a medium through motion of matter. In the atmosphere, it may be seen visibly by cloud formation and thunderstorm development
  3. 3. The transfer of energy through a medium from molecule to molecule due to a gradient in temperature
  4. 4. A naturally occurring process that aids in heating the Earth's surface and atmosphere
  5. 6. The layer of Earth's atmosphere between the stratosphere and the thermosphere, known for temperatures that decrease with altitude.
  6. 8. The proportion of the incident light or radiation that is reflected by a surface, typically expressed as a percentage.
  7. 9. The balance between the incoming energy from the sun and the outgoing energy emitted by the Earth back into space. It determines Earth's climate and temperature
  8. 11. Shortwave electromagnetic waves having wavelengths between 0.1 and 0.4 micrometers that is harmful to plants and animals, including humans.
  9. 12. A solid particle suspended in the atmosphere. Volcanic eruptions, salt spray, dust storms and forest fires are natural sources of this
  10. 13. NASA instruments that provides direct measurements of reflected solar radiation and emission of thermal infrared radiation from the earth to space
  11. 15. The second most abundant element in the universe, it is found in higher concentrations in the upper atmosphere due to its lightness and low chemical reactivity.
  12. 18. Energy that is emitted from a source in the form of rays or waves
  13. 21. The heat energy absorbed or released during a phase change of a substance, such as from liquid to gas or vice versa, without changing its temperature
  14. 23. A form of electromagnetic radiation, with a wavelength that is observable to the human eye (about 400–750 nanometers).
  15. 24. A process by which energy penetrates the inner structure of a material, causing that material to gain energy.
  16. 25. The return of sound or light back to its source. In the atmosphere, the process where incoming solar rays are redirected back upward after striking particles.