Chapter 4

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Across
  1. 3. is a description of the average kinetic energy of the molecules in a substance (strictly speaking, the average “back and forth” or translational kinetic energy of the molecules).
  2. 4. is what makes “stuff” move. For example, it takes energy to cause something to move faster, change direction, or break apart.
  3. 5. refers to energy that transfers from one object or substance to another because of a difference in temperature.
  4. 7. Wavelengths of radiation just shorter than the human eye can sense, from about 0.01 to 0.4 micrometers, make up the ultraviolet (UV) portion of the electromagnetic spectrum.
  5. 11. (incoming solar radiation) received at the top of the atmosphere is believed to be constant when averaged over a year, although it may vary slightly over long periods of time with fluctuations in the Sun’s temperature.
  6. 12. The human eye is sensitive to radiation wavelengths of only a fairly narrow band of the electromagnetic spectrum known as visible light— wavelengths between about 0.4 and 0.7 micrometers (om; 1 micrometer = one-millionth of a meter).
  7. 13. Scale The temperature scale that is most widely used—and announced in public weather reports—in the United States is the Fahrenheit scale (named after Gabriel Daniel Fahrenheit, the eighteenth-century German physicist who devised it).
  8. 14. Wavelengths of radiation just longer than the human eye can sense, between 0.7 and about 1000 micrometers (1 millimeter), make up the infrared (IR) portion of the electromagnetic spectrum.
  9. 15. refers to force acting over distance.
Down
  1. 1. sometimes referred to as radiant energy.
  2. 2. is entirely in the thermal infrared portion of the spectrum and is referred to as longwave radiation.
  3. 6. the energy of movement
  4. 8. Scale In most other countries the Celsius scale (named for Anders Celsius, the eighteenth-century Swedish astronomer who devised it) is used either exclusively or predominantly.
  5. 9. under extremely high temperatures and pressures, nuclei of hydrogen fuse together, forming helium.
  6. 10. or emission—is the process by which electromagnetic energy is emitted from an object.