Antennas and noise Flashcards

1
Q

antennas

A

devices that turn incident radiation into a corresponding electrical signal

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2
Q

astronomical signals are

A

noise-like

total power received is roughly proportional to bandwidth

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3
Q

why we simply add the powers received from each part of the source to get the total power

A

the radiation is from incoherent sources

the signals received from different parts of the source are uncorrelated

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4
Q

font end of antenna

A

antenna and low noise preamplifier

determines the strength of the signal and instrumental noise

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5
Q

back end of the antenna

A

cable, local oscillator, mixer, detector

performs the signal processing

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6
Q

as well as the noise-like signal itself, there is additional unwanted noise from

A

equipment
ground
atmosphere
galaxy

(sum of which is usually much stronger than the signal)

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7
Q

in a well-designed system,

A

no further noise is generated by the back end

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8
Q

large antennas are more

A

sensitive and directive

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9
Q

can think loosely of an antenna beam

A

the solid angle over which it collects signal

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10
Q

normalised power pattern

A

p(theta, thi) normalised so that Pmax=1

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11
Q

if we have an antenna that detects only one polarisation (1/2 the total power from an unpolarised source)

A

need to define effective area Ae

power received = 1/2SAe delta v

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12
Q

aperture efficiency

A

n= Ae/Ageo

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13
Q

if the source is not on the axis of the antenna but at (theta, thi) then power=

A

1/2 S Ae P(theta, thi) delta v

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14
Q

reciprocity theorem

A

antenna power patterns are the same for transmitters and receivers so can think in terms of either

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15
Q

simplest antenna - the dipole

A

E-field of radiation sets up currents in the antenna –> voltages over the resistor

these are relatively short and only sensitive to one polarisation

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16
Q

can a reversible antenna be sensitive to all the radiation

A

no
this would contradict the second law of thermodynamics

17
Q

consider a resistor at temp T - thermal motion of the electrons in the resistor…

A

generate a fluctuating voltage over its end

18
Q

Nyquist noise theorem

A

available power = kbT

very useful

19
Q

in equilibrium, there can be no

A

overall transfer of power between the two cavities

20
Q

the noise power (per unit frequency) generated by the antenna is

A

kbT

21
Q

if an antenna’s beam is filled with a blackbody source of temp T, the power the source delivers over a small bandwidth is

A

w=kbT delta v

22
Q

a dipole (or any antenna) in a cavity at T produces a power of

A

kbT delta v

23
Q

we can do away with the cavity if

A

the source at temp T fills the beam of the antenna

24
Q

antenna temp = true temp of the source if and only if

A

the source fills the beam

the source is blackbody, with a Planck spectrum

25
Q

antenna temp

A

just a useful unit with which to measure the power Hz^-1 received by a telescope

26
Q

if Ta=Tb then Ae=

A

lambda^2 / omega A

27
Q
A
27
Q

the effective area and beam solid angle are

A

inversely related

28
Q

big antennas have

A

small beams

29
Q

small antennas have

A

wide beams

30
Q

directive gain

A

angular selectivity an antenna has over an isotropic antenna

31
Q

beam efficiency

A

power in main beam lobe / total power

ie excludes sidelobes

32
Q

sidelobes are a worry because

A

they pick up stray radiation eg from the ground

33
Q
A