ay45c3-page34 - 3.6.2 Thermal bremsstrahlung Thermal...

Info iconThis preview shows page 1. Sign up to view the full content.

View Full Document Right Arrow Icon
This is the end of the preview. Sign up to access the rest of the document.

Unformatted text preview: 3.6.2 Thermal bremsstrahlung Thermal electrons (i.e. electrons with Maxwell-Boltzman distributions) moving near positive ions (e.g. H nuclei). Coulomb interactions cause the acceleration. e p Radiation is less intense; almost unpolarized; very at spectrum in radio, \thermal" in X-ray (Planck-like). typical X-ray: typical radio: log Iν ν −0.1 e−ν/ν0 ν 2.5 log ν ν Usually associated with hot gas: X-rays from clusters of galaxies; HII regions; surface of sun. Bremsstrahlung is usually associated with hot gas: X-rays from clusters of galaxies, HII regions, or the surface of the Sun, e.g. Synchrotron radiations and thermal bremsstrahlung are two of the common continuum emission mechanisms of gas. (Solids, e.g. surface of the Earth, are di erent.) 3.6.3 Line emission from atoms Electrons jumping from higher to lower levels in atoms emit excess energy as line radiation. The distribution of the lines in frequency and intensity are characterisic of the chemical element involved. 58 ...
View Full Document

This note was uploaded on 12/29/2011 for the course AST 350 taught by Professor Dion during the Fall '09 term at SUNY Stony Brook.

Ask a homework question - tutors are online