Radio Astronomy Cold Load Question

In summary: Cosmic Microwave Background Radiation: In summary, it was found that there was a discrepancy in the power readings of the amplifier circuits used in the discovery of the cosmic microwave background radiation. This discrepancy was due to the electrical noise in the circuits. By measuring the power coming from the antenna against the power produced by an artificial source chilled with liquid helium, they were able to eliminate the electrical noise and thus achieve a more accurate reading of the signal.
  • #1
racshot65
7
0
Hi,

I'm reading about the discovery of the cosmic microwave background radiation and don't understand this part ...


... It seemed likely this discrepancy was due to a slight excess of electrical noise in the amplifier circuits. In order to eliminate such problems they made use of a device know as a cold load.

The power coming from the antenna was compared with the power produced by an artificial source cooled with liquid helium.

The electrical noise in the amplifier circuit would be the same in both cases and therefore cancel out in the comparison. Allowing a direct measurement of the power coming from the antenna.


What power does a source called with liquid helium produce and how is it related to the amplifier circuits ?

I don't get what they did and why ?



Thanks !
 
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  • #2
I understand what they are doing ... I am just trying to think of a ways to easily describe it to you.

Thermal noise is a major problem when trying to detect very low level radio signals from deep space, that may only be say 20 Kelvin. The thermal noise of Helium is known, so measuring that noise level with your receiver, you get a given signal noise from the receiver. You can then determine what the thermal noise created by the receiving electronics is. Then when you switch the receiver to the antenna and measure the thermal noise from the deep space object ... even the widespread cosmic background radiation, you have already worked out what the thermal noise of your receiver is and it can be taken away (subtracted) from the received noise level when looking at your object.
The noise remaining is therefore the noise level (signal strength) of your object.

cheers
Dave
 
  • #3
as a further response, it is normal for receiver electronics in radio telescope use to be substantially cooled by liquid nitrogen during operation.

actually this is done even in commercial situations like ground based receiving stations for Earth orbiting satellites etc.


D
 

1. What is a cold load in radio astronomy?

A cold load in radio astronomy is a reference source used to calibrate and measure the sensitivity of a radio telescope. It is typically a metal object at room temperature that emits thermal radiation, which can be used to determine the noise temperature of the telescope's receiver.

2. How is a cold load used in radio astronomy?

A cold load is placed in the beam of the telescope and the resulting signal is measured. The known temperature of the cold load is then compared to the measured signal, allowing for the calibration and adjustment of the telescope's sensitivity.

3. What is the purpose of a cold load in radio astronomy?

The main purpose of a cold load in radio astronomy is to provide a standard reference source for calibrating the sensitivity of a radio telescope. It also helps to reduce the effects of temperature fluctuations and other sources of noise in the receiver.

4. How is the temperature of a cold load determined?

The temperature of a cold load is typically measured using a thermometer or thermal sensor. The temperature can also be calculated based on the known physical properties of the object, such as its composition and size.

5. Are there different types of cold loads used in radio astronomy?

Yes, there are different types of cold loads used in radio astronomy, including blackbody loads, open loads, and short loads. Each type has its own advantages and is used for different purposes, such as measuring different frequency ranges or providing a more accurate reference signal.

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