Radio Astronomy

by VU2FD

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Getting Started with Radio JOVE Observations

Jupiter's Decametric Radio Emissions

Solar Radio Bursts

Observing Tips - Solar Radio Bursts

The Radio JOVE antenna when configured the direct phasing configuration, is most sensitive near the zenith.
-- Observe between 11 and 3 local time, when the sun is near or directly above you.
Solar bursts are much less predictable than Jupiter storms and may last only for a few seconds.
-- Observe as often as possible and look at NASA's website (SOHO spacecraft) for increases in solar activity.
Solar bursts often look "fin" shaped and have two peaks when using Jove chart. You should also notice a rapid increase in intensity of the background and a slow decrease when a solar burst is detected using Radio JOVE.
-- Look at sample data for image and sound files on our website of solar bursts to better familiarize yourself with what they look like.
If you think you have recorded a solar burst, check with other observers.
-- Check NOAA website and the Radio and Plasma Wave Investigation (WAVE) instrument on the WIND spacecraft available at nasa website.
If you observe before or after 11 to 3 -
-- Setup your antenna anti-phase because this gives the antenna more sensitivity to the sun's lower angle position in the sky.
If it is cloudy and rainy outside, this should not prevent you from solar observing.
-- Solar bursts are very intense and usually penetrate the atmosphere unaffected by weather patterns.