types of antennas Flashcards
for v<1 GHz we can use
simple wire elements or arrays of elements
back reflector gives waves
a second chance
increases Ae
effective area can also be increased using
yagi, log periodic and helical antennas
for v> 1Ghz, more common are
horns
why are horns good
horn antenna patterns can be calculated accurately
good calibration and absolute measurements of bright sources
reflectors can increase
Ae
the feed horn must
illuminate the reflector
but illumination must taper at the edges so it doesn’t pick up the ground
theta =D/f and horn beamwidth=lambda/w so to minimise spillover
W > lambda f/ D
why is a small focal ratio (f/D) chosen
a large feed aperture (W) would block the signal
Typically, f/D is approx
0.4
which gives a more rigid structure
aperture efficiency is usually
0.6 to 0.65
cassegrain telescopes
longer effective focal length
easy access to feed
can modify secondary to improve performance
common choice for 30m dishes
no dish is perfect so it
can distort as it moves
is the rms surface error is epsilon then an rms phase error over the dish is
2pi/lambda . 2 epsilon
(factor of 2 due to reflection)
resultant amplitude is approx
ideal amplitude x cos (phase error)