\n<\/p>\n
This event was associated with a Type II Radio Emission with an estimated velocity of 928 km\/h, suggesting a coronal mass ejection (CME) was produced.<\/p>\n
Additionally, a 10cm Radio Burst (tenflare) lasting 2 minutes and with a peak flux of 400 sfu was associated with the flare event.<\/p>\n
A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.<\/p>\n
Radio frequencies were forecast to be most degraded over the South Atlantic Ocean and Africa at the time of the flare.<\/p>\n \n