Noise Removal in Radio Telescope Observations

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Discussion Overview

The discussion revolves around methods for removing noise and disturbances in radio telescope observations, focusing on various sources of interference such as man-made devices and atmospheric effects. Participants explore both theoretical and practical aspects of noise reduction techniques in radio astronomy.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants inquire whether "noise" refers to interference from man-made devices or from the telescope's own amplification stages.
  • There is mention of various electromagnetic signals that could interfere with observations, including AM, FM, GPS, and Bluetooth, suggesting a pervasive background of radio frequency noise.
  • Fourier transform is proposed as a method for noise removal, with a request for clarification on its application in this context.
  • One participant notes that narrow frequency bands can help isolate astronomical signals from nearby noise sources, emphasizing the importance of carefully designed receivers.
  • Concerns are raised about poorly maintained commercial transmitters that can generate harmonics and drift out of frequency, complicating noise removal efforts.
  • Participants discuss the atmospheric effects on radio signals, noting that short wavelengths are affected by solar signals and water vapor, while low frequencies are influenced by ionospheric conditions.
  • Frequency shifting is mentioned as a challenge, with suggestions that compensating for this involves focusing on weaker signals to reduce interference.
  • A question is posed regarding whether focusing on narrow frequency bands might lead to missing unique information present in broader commercial bands.

Areas of Agreement / Disagreement

Participants express a range of views on the sources of noise and the effectiveness of different noise removal techniques. There is no consensus on the best approach or the implications of using narrow frequency bands.

Contextual Notes

Limitations include potential missing assumptions about the nature of noise, the dependence on specific definitions of frequency bands, and unresolved details regarding the application of Fourier transforms in this context.

pseudo
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while dealing with radio telescopes how can we remove the noise and other disturbances like microwave radiation etc.
 
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When you say "noise" do you mean noise induced by man made devices such as cell phones, microwave ovens and washing machines? Or noise caused by amplifying stages of the telescope's receiver?
 
I have often wondered the same thing myself. I think pseudo meant radio frequency noise such as radio transmissions. We're bathed in electromagnetic signals: AM, FM, XM, VHF, UHF, Shortwave, GPS, Digital Pager waveband, Mobile Phone waveband, Wireless internet waveband, 2.4 GHz, 5.8 GHz, Bluetooth come to mind. Some of these signals must get out to the large array fields.
 
sysreset said:
I have often wondered the same thing myself. I think pseudo meant radio frequency noise such as radio transmissions. We're bathed in electromagnetic signals: AM, FM, XM, VHF, UHF, Shortwave, GPS, Digital Pager waveband, Mobile Phone waveband, Wireless internet waveband, 2.4 GHz, 5.8 GHz, Bluetooth come to mind. Some of these signals must get out to the large array fields.

there u got me sysreset. there is somthing called as fouriertransform which removes noise . can sm1 tell me how it is used ?
 
pseudo said:
there u got me sysreset. there is somthing called as fouriertransform which removes noise . can sm1 tell me how it is used ?

radio signals have no atmospheric disturbance. then why does the radio flux has disturbance. why do we use atmospheric extinction for radio flux and not for radio signals.whats d difference ?
 
The main way to remove background noise is to look at very narrow frequency bands.
By having very carefully designed receivers you can look at a faint astronomicla signal at 890Mhz and ignore the cell phone tower next door at 900Mhz.
There are international agreed quiet bands but a big problem is poorly maintained commercial transmitters that generate harmonics or drift out of frequency. Wide spectrum noise sources are a problem, car engines were a pain especially before electronic ignition.

Depending on the wavelength the sky does have an effect. At short wavelengths (high frequency) such as micrtowaves both the signal from the sun and water vapour in the air are a problem and so microwave telescopes are built on the same remote, high and dry sites as optical telescopes - this also gets them well away from artificial noise sources.
Low frequency (long wavelength) are sensitive to large scale waves in the ionosphere whihc cause 'seeing' like the shimmer of atmosphere seen by optical telescopes.
 
There is also the problem of frequency shifting. Radio waves I believe bounce off the ionosphere, and are slightly shifted.

I think they compensate by looking for lower signals. The interference produces a lot of strong signal lines. By looking for weaker ones, that can eliminate a lot of the interference.
 
Is it true that looking at narrow bands of frequency means that we are missing out on unique information carried on the bands we use for commercial purposes? Or is the consensus that the narrow bands give a good representation of what is out there?
 

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