types of antennas Flashcards

1
Q

for v<1 GHz we can use

A

simple wire elements or arrays of elements

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2
Q

back reflector gives waves

A

a second chance

increases Ae

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3
Q

effective area can also be increased using

A

yagi, log periodic and helical antennas

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4
Q

for v> 1Ghz, more common are

A

horns

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5
Q

why are horns good

A

horn antenna patterns can be calculated accurately

good calibration and absolute measurements of bright sources

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6
Q

reflectors can increase

A

Ae

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7
Q

the feed horn must

A

illuminate the reflector

but illumination must taper at the edges so it doesn’t pick up the ground

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8
Q

theta =D/f and horn beamwidth=lambda/w so to minimise spillover

A

W > lambda f/ D

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9
Q

why is a small focal ratio (f/D) chosen

A

a large feed aperture (W) would block the signal

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10
Q

Typically, f/D is approx

A

0.4
which gives a more rigid structure

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11
Q

aperture efficiency is usually

A

0.6 to 0.65

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12
Q

cassegrain telescopes

A

longer effective focal length
easy access to feed
can modify secondary to improve performance
common choice for 30m dishes

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13
Q

no dish is perfect so it

A

can distort as it moves

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14
Q

is the rms surface error is epsilon then an rms phase error over the dish is

A

2pi/lambda . 2 epsilon

(factor of 2 due to reflection)

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15
Q

resultant amplitude is approx

A

ideal amplitude x cos (phase error)

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16
Q

antenna arrays has a larger

A

collecting area

17
Q

antenna array has a smaller

A

beam

18
Q

if antenna in an array are equally spaced, the array is

A

mathematically similar to a diffraction grating

19
Q

if a > lambda, then secondary responses

A

appear, spaced by lambda/a

20
Q

usually choose Pa so that

A

the grating reponses are reduced to around zero

just one beam present

21
Q

there is a fourier transform relationship between

A

the arrangement of apertures and the resultant power pattern

22
Q

the power pattern is

A

the squared-modulus of the fourier transform of A(x)

23
Q

A(x) could either be

A

the position of the antenna

the electric field distribution over a wide aperture

24
Q

the fourier transform of a convolution is

A

the product of the individual fourier transforms

25
Q

concolving single aperture functions with arrays of delta function helps

A

construct complicated apertures

26
Q
A