Its bar and disc are the source of very strong radio emissions.

Despite many attempts, no radio emission is detected from these sources.

As suggested by the name, the radio emission is erratic.

Nor would this explain the huge radio emissions that had led to its original detection.

They made the background noise, the radio emissions of stars.

To their surprise, they found that the radio emissions did not vary significantly.

As it was, we only detected your radio emissions a few hundred years ago.

The storm is a strong source of radio emissions.

However, the radio emissions around the jets may also trigger star formation.

After all, we have been observing Jupiter's radio emissions for only a few decades.