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29:106/186 RADIO ASTRONOMY
Tenth Homework Set...April 24, 2000
Due: May 1, 2000

(1) An electron moves perpendicular to a magnetic field B with nonrelativistic velocity v. Give an expression for the radiation electric field as a function of time.

(2) This is a radio source count problem. Throughout the universe, radio sources have the same luminosity function

eqnarray9

where A has dimensions of #/cm tex2html_wrap_inline30 /ergs/sec.

Derive an expression for the differential radio source count tex2html_wrap_inline32 in such a universe.

(3) The radio galaxy 3C79 has a flux density of 2.5 Janskys at 1.4 GHz, a spectral index of -0.95 from 20 MHz to 10 GHz, and a redshift of 0.25. What is its luminosity over this frequency range?

(4) Magnetic fields in extended extragalactic radio sources are estimated to be of order tex2html_wrap_inline34 G. What are the energies of electrons responsible for emission at a frequency of 5 GHz?

(5) A radio source contains two populations of electrons. There are 100 electrons/cm tex2html_wrap_inline30 with an energy of 1 GeV, and 50 electrons /cm tex2html_wrap_inline30 with 1.41 GeV. The magnetic field is tex2html_wrap_inline40 Gauss. Assume the pitch angle of all electrons is tex2html_wrap_inline42 . Calculate the synchrotron radiation volume emissivity as a function of frequency.





Steve Spangler
Mon Apr 24 13:09:18 CDT 2000