The OVRO prototype
typically remains on-sun from dawn to dusk when not undergoing repair
or testing. Its field of view subtends the entire solar disk at all
frequencies from 245 MHz to 18 GHz. It may therefore contribute to
many coordinated observing campaigns pursued by the scientific community,
even those which concentrate on individual active regions. We encourage
all researchers to contact us to obtain data.
04/1998 - 07/2002 bursts
information and viewing software (in IDL)
will be available soon.