INTRO
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BUILDING THE TELESCOPE
SOFTWARE
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OBSERVING
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DATA ANALYSIS
 
 

Radio Telescope – Data Analysis

After setting up the Radio JOVE 2.1 receiver and the antenna system successfully, you are now ready to make radio observations and take data. We hope your setup is at a radio-quiet location where it is relatively free of radio frequency interference (RFI). We must recognize, however, that neither the antenna nor the radio receiver system has the capability to distinguish whether the detected signals are coming from Jupiter, the Sun, the Galactic radio background, or from radio stations or other local interference like fluorescent lights, a lawnmower, or a heat pump/air conditioner.

With practice you will be able to recognize many types of astronomical signals in your spectrograph data compared with terrestrial interference. Below are a few examples of spectrographs.

Example RJ spectrograph output
Example Radio JOVE spectrograph output using RSS display software with SDR Console and SDRc2RSS running in the background. Note the large increase in signal denoted by the colored background after the antenna is disconnected / connected. Horizontal bands are local interference, some very strong near 18 MHz. (C. Higgins, 2025)
Radio Jove spectrograph with solar bursts and sweepers
A Radio JOVE spectrograph showing multiple solar bursts as the near-vertical “wispy” bands. Spotty interference occurs at several frequencies, with more interference below about 18 MHz. A positively sloped “sweeper” radar signal is seen near the center of the spectrograph. (C. Higgins, 2021)
Radio Jove spectrograph with solar bursts and sweepers
An SDR spectrograph showing several solar bursts as the near-vertical “wispy” bands. Several positively sloped “sweeper” radar signals are seen. (L. Dodd, 2022)
24-hour spectrograph output
Example 24-hour Radio JOVE spectrograph output using RSS display software. Note the clear difference in the nighttime observations on the left and the daytime observations on the right. Local interference is more prevalent during the daytime. (C. Higgins, 2022)
Radio Jove spectrograph with jupiter radio bursts
A 4.5-hour wide band spectrograph from 16 – 32 MHz showing an excellent Jupiter Io-B emission event (D. Typinski, 2016).

Please check back here periodically for more examples of spectral features and for more information on spectrograph data processing.

For an excellent summary of data reduction techniques with the original Radio JOVE RJ1.1 receiver, see the material on this web page:
https://radiojove.gsfc.nasa.gov/radio_telescope/rj1.1/rj1.1_data_analysis.php

GIF of plots from AJ4CO
spectral display