A SHOCK ASSOCIATED (SA) RADIO EVENT AND RELATED PHENOMENA OBSERVED FROM THE BASE OF THE SOLAR CORONA TO 1 AU

We present for the first time an almost complete frequency coverage of a Shock Associated (SA) radio event and related phenomena observed on May 6, 1996 at 9:27 UT. It is observed from the base of the solar cor ona up to almost 1 Astronomical Unit (AU) from the Sun by the followin g radio astronomical instruments: the Ondrejov spectrometer operating between 4.5 GHz and 1 GHz (radiation produced near the chromosphere); the Thermopyles Artemis-N spectrograph operating between 600 MHz and 1 10 MHz (distance range about 1.1-1.4 R-. from sun center); the Nancay Decameter Array operating between 75 and 25 MHz (distance range about 1.4-2 R-.); and the RAD2 and RAD1 radio receivers on the WIND spacecra ft covering the range from 14 MHz to about 20 kHz (distance range betw een 3 R-. and about 1 AU). Observations at the Nancay Decameter Array clearly show that the SA event starts from a coronal type II radio bur st which traces the progression of a shock wave through the corona abo ve 1.8 R-.-2 R-. from the sun center. This SA event has no associated radio emission in the decimetric-metric range, thus there is no eviden ce for electron injection in the low/middle corona.