To: | propagation <propagation@contesting.com>,"PropNET-Online@yahoogroups.com" <PropNET-Online@yahoogroups.com> |
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Subject: | [Propagation] NW7US Propagation Update Bulletin 16-I-2005 0430 UTC |
From: | "NW7US, Tomas" <nw7us@hfradio.org> |
Date: | Sat, 15 Jan 2005 20:50:52 -0800 |
List-post: | <mailto:propagation@contesting.com> |
NW7US Propagation Update Bulletin 16-I-2005 0430 UTC At the time of this bulletin, we've just witnessed another long-duration flare. This is the strongest of the flares so far unleashed by active sunspot region 720 (NOAA 10720). This flare was a major X2.6-class event that peaked at 2302 UTC 15-I-2005. A Type II radio burst was detected, and a proton event is currently underway, as well. A very fast coronal mass ejection was associated with this X2.6 flare. It looks like the majority of the plasma mass will just miss the Earth, yet we expect at least a glancing blow. We expect this to occur sometime on 17 or 18 January 2005, riding on the heels of the CME from the M-class long-duration flare from earlier (refer to my last bulletin). This will cause the geomagnetic storm to be prolonged. The storm will begin at any time in the next 24 hours, and last well past 17 January 2005. We expect minor storm levels on 16 January, severe storm levels on 17 and 18 January. The solar activity has significantly risen as a result of the active solar regions. The 10.7-cm Flux has reach 145, and is expected to increase to perhaps 150 by 17 and 18 January 2005. This has opened up paths on frequencies as high as 10 meters. This translates to disrupted HF conditions caused by shortwave fadeouts for the next three days due to active solar region 720 (and possibly from flares from 718). When the CME clouds arrive and impact our environment we expect the Maximum Usable Frequencies on most signal paths to become very depressed in coming days. HF communication may become very difficult if this active solar region continues to flare, while at the same time we have the storm conditions in the geomagnetic field around the Earth. Look for active visual Aurora starting tonight and through the next few days (even in mid- to low-latitude regions). Energetic pulses will occur. Aurora-E / Aurora-mode propagation is likely. Active region 720 unleashed a total of 20 flares during 15 January 2005. These are: Event Begin/Max/End Level Reg# ------------------------------- 2690 + 0022 0043 0102 X1.2 0720 2740 + 0234 0239 0244 C2.9 0720 2750 + 0316 0340 0357 C4.2 0720 2760 + 0409 0416 0422 M1.3 0720 2770 + 0426 0431 0436 M8.4 0720 2780 + 0554 0638 0717 M8.6 0720 2820 + 1141 1148 1150 M1.2 0720 2830 + 1227 1231 1234 C7.4 0720 2890 + 1352 1357 1359 C5.5 0720 2900 + 1408 1423 1439 M3.2 0718 2940 + 1650 1657 1702 C8.0 0720 3000 + 1703 1707 1709 C7.2 0720 2960 + 1749 1816 1824 C4.2 0720 3010 1757 1802 1805 C2.9 0720 2970 1812 1815 1818 C4.4 ? 3020 + 1842 1853 1901 C8.8 0720 3040 + 1944 1949 1954 C3.5 0720 3050 + 2008 2022 2027 C5.4 0720 3080 + 2201 2208 2216 M1.0 0720 3090 + 2225 2302 2331 X2.6 0720 Updates will be posted if and when warrented. 73 de Tomas, NW7US (AAR0JA/AAA0WA) : Propagation Editor for CQ, CQ VHF, Popular Communications : : Creator; live propagation center http://prop.hfradio.org/ : : Associate Member of Propagation Studies Committee of RSGB : : US Army Miltary Affiliate Radio Service (MARS) SMD AAA0WA : : 122.93W 47.67N / Brinnon, Washington USA CN87 CW/SSB/DIGI : : Website/software/database design http://newwebmakers.com/ : : 10x56526, FISTS 7055, FISTS NW 57, Lighthouse Society 144 : _______________________________________________ Propagation mailing list Propagation@contesting.com http://lists.contesting.com/mailman/listinfo/propagation |
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