The SPADE instrument has been designed for solar observations in mind and has been monitoring the solar activity in the last few months with really nice events.
Aside from the Sun, the solar system hosts another major source of radio emission: Jupiter. In the decametric range, energetic electrons trapped in the jovian magnetosphere produce intense radio emission. Unlike solar radio bursts, jovian radio emission occurrences have a certain degree of regularity, being modulated by the planet's rotation (in approximately 10 hours) and by the relatively position of Io with respect to the observer.
For test purposes, SPADE has been programmed to track Jupiter at night at the end of November / early December, with the following results.
They compare relatively well with the results of the DAM array at the Nançay Observatory, which has been monitoring these emissions since the 1980s.