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24.1 and 24.3 Vocabulary

Published on Nov 18, 2015

From Prentice Hall Earth Science Text Book; "Studying the Sun" Chapter 24

PRESENTATION OUTLINE

24.1 and 24.3 Vocabulary

by Shannon Fogarty

24.1: The Study of Light

Photo by Werner Kunz

Electromagnetic Spectrum

  • The arrangement of electromagnetic radiation according to wavelength
Photo by CLS Rob

Photon

  • A small packet of light energy
Photo by AliaK

Spectroscopy

  • The study of the properties of light that depend on wavelength
Photo by The^Bob

Continuous Spectrum

  • An uninterrupted band of light emitted by an incandescent solid, liquid, or gas under pressure
  • (Spectrum is similar to that of a rainbow, so the background makes sense)
Photo by alx_chief

Absorption Spectrum

  • A continuous spectrum produced when white light is passed through a cool gas under low pressure
  • The gas absorbs selected wavelengths of light, and the spectrum looks like it has dark lines superimposed
Photo by The^Bob

Emission Spectrum

  • A series of bright lines of particular wavelengths produced by a hot gas under low pressure
  • (Background is example of spectrum)
Photo by Alfredo Louro

Untitled Slide

Doppler Effect

  • The apparent change in frequency of electromagnetic or sound waves caused by the relative motions of the source and the observer
Photo by brewbooks

24.3: The Sun

Photo by rishibando

Photosphere

  • The region of the sun that radiates energy to space; visible surface of the sun

Chromosphere

  • The first layer of the solar atmosphere found directly above the photosphere

Corona

  • The outer weak layer of the solar atmosphere

Solar Wind

  • Streams of protons and electrons ejected at high speed from the solar corona
  • (Background is of someone wind-surfing, so it makes sense)
Photo by Bemep

Sunspot

  • A dark spot on the sun, which is cool by contrast to the surrounding photosphere

Prominence

  • A concentration of gases above the solar surface that appears as a bright arch-like structure

Solar Flare

  • A sudden and tremendous eruption in the solar chromosphere

Aurora

  • A bright display of ever-changing light caused by solar radiation interacting with the upper atmosphere in the region of the poles
Photo by marceloquinan

Nuclear Fusion

  • The way in which the sun produces energy
  • Occurs when less massive nuclei combine into more massive nuclei, releasing tremendous amounts of energy