Most of these phenomena and certainly the most powerful ones, take place in plasma densities that correspond to plasma frequencies of 0.1 - 3 GHz. The whole disk is monitored in the 0.1 - 3 GHz range. It is the widest band currently available in astronomy. Events are identified and recorded in flux and polarization. The fully automatic and remotely controlled instrument is constantly improved.
Special emphasis is on user-friendly operation and easy data analysis.
Examples are given on our pretty picture page.