At 1955Z, 4-XI-2003, an X-class flare peaked from region 486. Initial data from GEOS 12 indicates that the flare is an X18, while GEOS 10 shows it as X17. However, there is speculation (i.e., Thomas Giella (KN4LF), others) that it might be much stronger, as this event saturated the sensor for 11 minutes. I have viewed preliminary images of this very bright and significant flare, and it is truly amazing.
If the flare is larger than the X17 flare from recent activity, this will become one of the two most powerful flares recorded. The flare has caused extensive radio blackout conditions on most of the HF radio spectrum. Ground wave communications is not significantly impacted, nor is line-of-sight VHF and above. A type II Radio Emission began at 1942Z 4-XI-2003 with an estimated velocity of 1268 km/s. Interplanetary type II bursts are statistically strongly associated with fast CME and interplanetary shock waves (Cane, Shelley & Howard 1987). Thus, there is a chance that we will have at least a glancing blow from the side of the possible CME associated with this new flare. I will update when more data is known. 73 de Tomas, NW7US (AAR0JA/AAM0EWA) -- : Propagation Editor, CQ/CQ VHF/Popular Communications Magazines : : http://hfradio.org/ -- http://prop.hfradio.org/ -- Brinnon, WA : : 122.93W 47.67N - CW / SSB / DIGITAL / DX-Hunting / Propagation : : A creator of solutions -- http://accessnow.com/ -- Perl Rules! : : Washington State MARS Emergency Operations Officer - (AAM0EWA) : : WA State Army MARS Webmaster for http://wa.mars.hfradio.org/ : : 10x56526, FISTS 7055, FISTS NW 57, A.R. Lighthouse Society 144 : ---[Start Commercial]--------------------- World Radio TV Handbook 2004 is coming out! Preorder yours now! Only $20.97 through us. http://www.amazon.com/exec/obidos/ASIN/0823059685/hardcoredxcom ---[End Commercial]----------------------- ________________________________________ Hard-Core-DX mailing list [EMAIL PROTECTED] http://dallas.hard-core-dx.com/mailman/listinfo/hard-core-dx http://www.hard-core-dx.com/ _______________________________________________ THE INFORMATION IN THIS ARTICLE IS FREE. It may be copied, distributed and/or modified under the conditions set down in the Design Science License published by Michael Stutz at http://dsl.org/copyleft/dsl.txt