Kilometric Radio Emissions from WIND/WAVES as a tool to improve Space Weather Forecasts

F. A. IGLESIAS; H. CREMADES; O. C. ST. CYR; M. L. KAISER

CASLEO, San Juan

Workshop; 4th El Leoncito School on Solar Physics; 2008

For decades, space environment forecasters have used the appearance of metric Type II radio emission as a proxy for eruptions in the solar corona. The drift rate of these near-Sun emissions is often turned into a speed, commonly assumed to be that of an MHD shock. However, their utility to forecast shock arrival times has not proved to be conclusive. Metric emissions can be detected by ground-based antennas, however, lower-frequency components of these slowly-drifting emissions can only be tracked by spacecraft in interplanetary space, as far down in frequency as that of the local plasma frequency. For a spacecraft at L1, this corresponds to about 25 kHz, or an electron density of about 7 cm-3 in the ambient solar wind. Here we report a recent study that aims to improve the predictions of shock arrival time at L1 by means of the low frequency emissions detected by WIND/WAVES. This novel technique, based on the drift rate of hectometric and kilometric type II radio bursts, has yielded promising results.