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Polarisability and Scattering in Interstellar Medium

This article discusses the concept of polarisability and its relation to scattering in interstellar gas and dust clouds.

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Polarisability and Scattering in Interstellar Medium

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  1. Harry Kroto 2004

  2. P = E

  3. P = E E = Eocos2πωt

  4. P = E E = Eocos2πωt P = Eocos2πωt

  5. Harry Kroto 2004

  6. this shows a Hertz osci http://en.wikipedia.org/wiki/File:Dipole.gif-oli Harry Kroto 2004

  7. http://www.ccpo.odu.edu/~lizsmith/SEES/ozone/class/Chap_4/index.htmhttp://www.ccpo.odu.edu/~lizsmith/SEES/ozone/class/Chap_4/index.htm

  8. P = α E Total polarisability

  9. P = α E Total polarisability α = αo + (∂α/∂q)q Molecular polarisability - function of coordinate

  10. P = α E Total polarisability α = αo + (∂α/∂q)q Molecular polarisability - function of coordinate E = Eocos 2πωet Electric Field radiation frequency ωe

  11. P = α E Total polarisability α = αo + (∂α/∂q)q Molecular polarisability - function of coordinate E = Eocos 2πωet Electric Field radiation frequency ωe q = qo cos 2πωqt coordinate of the molecular motion ωq

  12. P = α E Total polarisability α = αo + (∂α/∂q)q Molecular polarisability - function of coordinate E = Eocos 2πωet Electric Field radiation frequency ωe q = qo cos 2πωqt coordinate of the molecular motion ωq P = [αo + (∂α/∂q) q] E

  13. P = α E Total polarisability α = αo + (∂α/∂q)q Molecular polarisability - function of coordinate E = Eocos 2πωet Electric Field radiation frequency ωe q = qo cos 2πωqt coordinate of the molecular motion ωq P = [αo + (∂α/∂q) q] E P = [αo + (∂α/∂q) q] Eocos 2πωet

  14. P = α E Total polarisability α = αo + (∂α/∂q)q Molecular polarisability - function of coordinate E = Eocos 2πωet Electric Field radiation frequency ωe q = qo cos 2πωqt coordinate of the molecular motion ωq P = [αo + (∂α/∂q) q] E P = [αo + (∂α/∂q) q] Eocos 2πωet P = [αo + (∂α/∂q) qo cos 2πωqt] Eocos 2πωet

  15. P = α E Total polarisability α = αo + (∂α/∂q)q Molecular polarisability - function of coordinate E = Eocos 2πωet Electric Field radiation frequency ωe q = qo cos 2πωqt coordinate of the molecular motion ωq P = [αo + (∂α/∂q) q] E P = [αo + (∂α/∂q) q] Eocos 2πωet P = [αo + (∂α/∂q) qo cos 2πωqt] Eocos 2πωet P = αo Eocos 2πωet + (∂α/∂q) qo Eocos 2πωqt cos 2πωet

  16. P = α E Total polarisability α = αo + (∂α/∂q)q Molecular polarisability - function of coordinate E = Eocos 2πωet Electric Field radiation frequency ωe q = qo cos 2πωqt coordinate of the molecular motion ωq P = [αo + (∂α/∂q) q] E P = [αo + (∂α/∂q) q] Eocos 2πωet P = [αo + (∂α/∂q) qo cos 2πωqt] Eocos 2πωet P = αo Eocos 2πωet + (∂α/∂q) qo Eocos 2πωqt cos 2πωet P = αo Eocos 2πωet + ½(∂α/∂q) qo Eo[cos 2π(ωe+ ωq)t + cos 2π(ωe- ωq)t]

  17. P = E E = Eocos2πωt P = Eocos2πωt

  18. P = E E = Eocos2πωt P = Eocos2πωt

  19. P = E E = Eocosωt P = Eocosωt

  20. Attenuation due to scattering by interstellar gas and dust clouds Harry Kroto 2004

  21. Harry Kroto 2004

  22. Harry Kroto 2004

  23. P =  E

  24. P =  E

  25. P =  E

  26. P =  E

  27. Bill Madden 559 2123

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