Types of Antenna Flashcards
Effective area can be increased by using
Yagi antenna
For v < 1GHz use
simple elements, i.e. dipoles
For v > 1GHz use
horns
Horn diagram
see notes
A large feed aperture (w) does what to the signal
it blocks it, so choose a small focal ratio (f/D)
Cassegrain Telescope diagram
see notes
longer effective focal length
easy access to feed
can modify secondary to improve performance
usual choice for ~ 30m dishes
Spherical mirrors diagram
see notes
Line-focus overcomes spherical aberration
Observations can be made up to ~20 degrees from the zenith
Spherical Irregularities diagram
see notes
rms surface error ε => phase error Φ = 2π/λ*2ε
Antenna arrays
Single antennas can be combined to make an antenna array with a larger collecting area Ae
If the antenna array is equally spaced it acts like a
diffraction grating
phase difference between adjacent antennas
Φ = 2π/λ*asinθ
A geometric progression
E = Eo exp( (iΦ/2)^(n-1)) * sin(nΦ/2)/sin(Φ/2)
There is a Fourier transform relationship between the distribution of apertures
The power pattern
P(θ) ∝ |+∞ ∫-∞ A(x) exp(iksinθx)dx |²
convolution theorem
f*g = f.g
the Fourier transform of a convolution is
the product of the individual Fourier transforms