1.10.8: Speed of Radio Waves
- Page ID
- 128487
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)tanding waves of UHF radio are used to measure the speed of radio waves, which we then compare with the measured speed of light. This is an important comparison: Maxwell realised that the waves that are a solution to the equations for electricity and magnetism had a speed similar to that measured for light. This was persuasive evidence that light was an electromagnetic wave. This page supports the multimedia tutorial The Nature of Light.
- The experiment
- Standing waves
- Light, electromagnetism, time, space and relativity
- Electromagnetic waves
The experimentFor this experiment, we set up a horizontal dipole antenna on a pole and powered it with a 300 MHz oscillator to radiate UHF radio waves. A second dipole antenna in my hand is connected to the oscilloscope whose screen we see at left. The wavelength is one metre, so both antenna are one half a wavelength long. The waves are transverse and are polarised with the electric field parallel to the antenna, as we show in Transverse Electromagnetic Waves.
On the ground we have spread aluminium foil. Aluminium is a conductor, so this reflects the electric wave with a phase change of 180°, giving approximately zero electric field in the conductor. The receiving antenna measures the superposition of the incident and reflected waves. In the animation, the incident (electrical) wave is blue, the reflected wave is red, and the purple wave is the superposition: the total electric field at that point. The horizontal scale is arbitrary, the vertical scale is pretty accurate and time has been slowed down by a hundred million or so for us to see it. |
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Standing wavesBefore we look more closely at the interference pattern, you may like to review the multimedia tutorial on interference.The amplitude of the wave decreases as 1/r, where r is the distance from the transmitter. At the point of reflection, the incident and reflected waves have the same amplitude, but elsewhere the incident wave has a larger amplitude than the reflected one. Thus the nodes in the combined wave do not have an amplitude of zero (except at the point of reflection); rather, they are local minima in the interference pattern.
So here is the experiment. Two video cameras were used. They were synchronised to within a frame or two by zooming out and waving an arm in front of both. One gives the view at left, the other was focussed on the oscilloscope screen, whose (simultaneous) image was shown at right. The nodes are easiest to see near the bottom, where the incident and reflected amplitudes are most similar in amplitude. As we saw in interference, the nodes are separated by half a wavelength, which is here L = λ/2 = 0.50 m. The oscilloscope setting had 2 ns per division, giving 20 ns across the screen. The period of the wave is measured at T = 3.3 ns (the oscillator was set at 300 MHz), so the speed is λ/T = 3.0 X 108 m.s−1. (Thanks to Barry Perczuk, Pat McMillan and the UNSW third year physics lab for lending both the UHF oscillator and the 500 MHz oscilloscope.) It's interesting to compare this measured speed of radio waves with the measured speed of light. Maxwell noted that the speed of the wave solution to the equations of electromagnetism was similar to that measured for light. This was persuasive evidence that light was an electromagnetic wave. |

