0 a set of radio waves of similar length that are used for broadcasting radio programmes
Much of the chapter is devoted to a fairly exhaustive listing of launch dates, orbits and sensor wavebands for past and current remote sensing missions.
We have also carried out monochromatic imaging of individual narrow wavebands and compared the relative intensity of emission.
As a consequence of the different measurement conditions, there exists some disagreement in the selection of wavebands.
Infrared spectroscopy over the 2.9-3.9 mm waveband in biochemistry and astronomy.
An example of solar radio bursts is selected as evidence for envelope solitons in the electromagnetic waveband.
In addition, the proceeds of the wavebands should never be seen as a stealth tax.
Such provision would not interfere with wavebands or national broadcasting organisations.
We were given an answer yesterday on the number of wavebands still available.
