Radio Astronomy Cold Load Question

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SUMMARY

The discussion centers on the use of a cold load in radio astronomy to mitigate thermal noise when measuring low-level signals, such as those from the cosmic microwave background radiation. The cold load, cooled with liquid helium, allows for a comparison between the power from the antenna and the known thermal noise produced by the cold load. This method effectively cancels out the electrical noise from the amplifier circuits, enabling accurate measurements of the signal strength from astronomical sources. The importance of cooling receiver electronics with liquid nitrogen in both radio telescopes and commercial ground-based receiving stations is also highlighted.

PREREQUISITES
  • Understanding of thermal noise in electronic circuits
  • Familiarity with radio astronomy principles
  • Knowledge of liquid helium and its properties
  • Basic concepts of signal processing in radio receivers
NEXT STEPS
  • Research the principles of thermal noise and its impact on radio signal detection
  • Explore the design and function of cold loads in radio telescopes
  • Learn about the cooling techniques used in radio astronomy, specifically liquid nitrogen and liquid helium
  • Investigate the methods for measuring cosmic microwave background radiation
USEFUL FOR

Astrophysicists, radio astronomers, engineers involved in signal processing, and anyone interested in the technical aspects of measuring low-level radio signals from space.

racshot65
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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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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
 
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
 

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