Prove that the group velocity o, of electromagnetic waves in a dispersive medium with refractive index n is given by dn n+ a da where c is the free-space velocity of light and w is the angular frequency of the waves. A pulsar is a star which emits very sharp pulses over a broad range of radio frequencies. These travel through the interstellar medium in a straight line before arriving at Earth. Radio observations show that the arrival time of a particular pulse measured at 400 MHz is 700 ms later than the arrival time of the same pulse measured at 1400 MHz. The refractive index of the interstellar medium is given by Ne? Eomar where e and m are the charge and mass of an electron, and N is the electron density, which is known to have an approximately uniform value of 3 x 10' m- in the space between the Earth and the pulsar. Calculate the distance to the puksar.
Prove that the group velocity o, of electromagnetic waves in a dispersive medium with refractive index n is given by dn n+ a da where c is the free-space velocity of light and w is the angular frequency of the waves. A pulsar is a star which emits very sharp pulses over a broad range of radio frequencies. These travel through the interstellar medium in a straight line before arriving at Earth. Radio observations show that the arrival time of a particular pulse measured at 400 MHz is 700 ms later than the arrival time of the same pulse measured at 1400 MHz. The refractive index of the interstellar medium is given by Ne? Eomar where e and m are the charge and mass of an electron, and N is the electron density, which is known to have an approximately uniform value of 3 x 10' m- in the space between the Earth and the pulsar. Calculate the distance to the puksar.
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Transcribed Image Text:Prove that the group velocity o, of electromagnetic waves in a dispersive
medium with refractive index n is given by
dn
n+ a
da
where c is the free-space velocity of light and w is the angular frequency
of the waves.
A pulsar is a star which emits very sharp pulses over a broad range of
radio frequencies. These travel through the interstellar medium in a
straight line before arriving at Earth. Radio observations show that the
arrival time of a particular pulse measured at 400 MHz is 700 ms later
than the arrival time of the same pulse measured at 1400 MHz. The
refractive index of the interstellar medium is given by
Ne?
where e and m are the charge and mass of an electron, and N is the
electron density, which is known to have an approximately uniform value
of 3 x 10' m- in the space between the Earth and the pulsar. Calculate
the distance to the puksar.
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