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Introduction to Solar Observing |
Course Overview | Course Syllabus | Course Schedule |
| Index of Course Sessions |
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Session 1 Review
| Glossary: | |
| Absorption lines | - dark lines in a continuous spectrum of white light caused by
absorption by a gaseous element. The lines correspond to the same light frequencies that would be emitted by the gaseous element. |
| Continuous spectrum | - one which shows continuous non-discrete changes of intensity with
wavelengths or particle energy. |
| Diffraction | - the spreading out of light passing through an aperture or opening or opaque object |
| Diffraction Grating | - optical device made of glass or metal etched with thousands of closely-spaced lines . The grooves produce interference patterns in light. There are two types; transmission gratings allo the light to pass through, while reflection gratings reflect the light away. |
| Dispersion | - the dependence of wave velocity on the frequency of wave motion; a property of the medium in which the wave is propagated. In the visible region of the electromagnetic spectrum, dispersion manifests itself as the variation of refractive index of a substance with wavelength (colour) of the light. It is on account of its dispersion that a prism is able to form a spectrum. |
| Emission line spectrum | - a spectrum that contains bright emission lines |
| Reflection | - the return of light rays by a surface |
| Refraction | - bending of light rays when they pass from one transparent medium to another |
| Spectrograph | - an instrument for photographing a spectrum |
| Spectrometer | - any device that produces a spectrum by dispersion and is calibrated to measure transmitted energy with respect to wavelengths of radiation, refractive indices of prism materials, or radiant intensities at various wavelengths. |
| Spectroscope | |
| Spctroscopy | - the analysis of the ways in which matter emits and absorbs radiation |
| Spectrum | (1) A distribution of entities or properties arrayed in order of
increasing or decreasing magnitude. For example, a beam of ions passed through a mass
spectrograph, in which they are deflected according to the charge-to-mass ratios, will
have a range of masses called a mass spectrum. A sound spectrum is the distribution of
energy over a range of frequencies of a particular source. (2) A range of electromagnetic energies arrayed in order of increasing or decreasing wavelength or frequency. The emission spectrum of a body or substance is the characteristic range of radiations it emits when it is heated, bombarded by electrons or ions, or absorbs photons. The absorption spectrum of a substance is produced by examining, through the substance and through a spectroscope, a continuous spectrum of radiation. The energies removed form the continuous spectrum by the absorbing medium show up as black lines or bands. With a substance capable of emitting a spectrum, these are in exactly the same positions in the spectrum as some of the lines and bands in the emission spectrum. Emission and absorption spectra may show a continuous spectrum, a line spectrum or a band spectrum. A continuous spectrum contains an unbroken sequence of frequencies over a relatively wide range; it is produced by incandescent solids, liquids and compressed gases. Line spectra are discontinuous lines produced by excited atoms and ions as they fall back to a lower energy level. Band spectra (closely grouped bands of lines) are characteristic of molecular gases or chemical compounds. |
| Wavelength | - the horizontal distance between crests of two adjacent waves. |
| References: Kaufmann, W.J. and Freedman,
R.A., Universe, 5th Edition, 1998, W.H. Freeman and Company, New York |
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| Page last updated 10/29/01 | Copyright © 2001 M.C.Gino |