THE DIRECTIVITY OF SOLAR KILOMETRIC TYPE-III BURSTS - ULYSSES-ARTEMISOBSERVATIONS IN AND OUT OF THE ECLIPTIC-PLANE

Comparing the records of the radio spectrographs ARTEMIS (100-500 MHz) on the ground and URAP (1-1000 kHz) on the Ulysses spacecraft, we fin d that most type III bursts extend from the corona to the solar wind. Using the positions of the associated flares, and assuming an average intensity ratio between these two frequency ranges, we derive for the first time the average radiation pattern of interplanetary type III bu rsts. We find that at 800 kHz it is shifted east of the radial directi on by 30 degrees and has a half-width of about 80 degrees at maximum/1 0; the shift and width increase towards Lower frequencies. Ulysses hig h-latitude observations show that the cross-section perpendicular to t he heliospheric equator is about the same. We interpret these properti es by refraction effects in local density gradients.