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Slide Notes

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24.1 & 24.3

Published on May 10, 2016

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PRESENTATION OUTLINE

24.1 & 24.3

Electromagnetic Spectrum

  • The range of wavelengths or frequencies over which electromagnetic radiation extends.
Photo by davidsancar

Photon

  • A particle representing a quantum of light or other electromagnetic radiation. A photon carries energy proportional to the radiation frequency but has zero rest mass.
Photo by Rick Bolin

Spectroscopy

  • The branch of science concerned with the investigation and measurement of spectra produced when matter interacts with or emits electromagnetic radiation.
Photo by ptc24

Continuous Spectrum

An emission spectrum that consists of a continuum of wavelengths.

Absorption Spectrum

  • A spectrum of electromagnetic radiation transmitted through a substance, showing dark lines or bands due to absorption of specific wavelengths.

Emission Spectrum

A spectrum of the electromagnetic radiation emitted by a source.

Doppler Effect

  • An increase (or decrease) in the frequency of sound, light, or other waves as the source and observer move toward (or away from) each other. The effect causes the sudden change in pitch noticeable in a passing siren, as well as the redshift seen by astronomers.
Photo by Serge Melki

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
Photo by whale05

Corona

The outer weak layer of the solar atmosphere
Photo by i_yudai

Solar Wind

  • Stream of protons and electrons ejected at high speed from the solar corona

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 archlike 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 cfaobam

Nuclear Fusion

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