|Subject:||[CQ-Contest] X-class flares, propagation, and... aurora?|
|From:||"NW7US, Tomas" <firstname.lastname@example.org>|
|Date:||Fri, 16 Jul 2004 08:19:47 -0700|
at the time of writing this NW7US Propagation Bulletin, we are recovering from an X3-class X-ray Flare. This is the fifth X-class flare in the last day and a half. This flare measured X3.6, the strongest of the five. And there is more on the way.
Active Region 649 (as numbered by NOAA, 10649) is about to cross the central part of the Sun. Within about 3 days it will directly facing us. Although this region is not particularly large (it is not visible to the unaided eye), it is demonstrating its volatility. Each of these flares has been spaced by approximately 8 hours of relative inactivity.
Region 649 maintains its beta-gamma-delta topology indicating that more strong flaring activity is very likely. Meanwhile, a new, very dynamic, active region is popping up from around the East limb promising continued strong flaring activity.
The compact magnetic structure known as a "magnetic delta," is where opposite polarity sunspot umbrae are located within a single penumbra. This particular type of magnetic configuration supports unusually high magnetic gradients as well as strong levels of magnetic shear. This is what we're seeing in the beta-gamma-delta topology of Region 649.
When we see strong atmospheric pressure gradients in Earth's atmosphere, combined with changes in wind direction with height (wind shear), we typically see the formation of tornadoes. This is the same sort of thing that is happening on the Sun. Strong magnetic gradients along with strong magnetic shear with the complex twisting produce powerful magnetic explosions.
So far, these X-class flares eruptions have not apparently been associated with significant coronal mass ejection (CME) activity. We don't yet know from this latest flare if there was a CME associated with this one. It is expected that one or more of these events will be associated with a coronal mass ejection. If that happens in the next few days and into next week, we'll see an increase in auroral activity (northern lights). Those of you interested in this phenomenon are encouraged to stay informed during the next week.
These flares cause nearly immediate disruption of HF ionospheric radio communications. The stronger the x-ray flare is, the higher the frequencies will be that are absorbed. X-class flares are in the strongest flare category. Flares are classified by their intensity, the lowest category being A, followed by categories B, C, M, and finaly X.
X-class flares can cause the absorption of radio signal energy well past 20 MHz. Minor solar flares (C-class) will not affect frequencies much beyond 5 MHz. The x-rays from these events penetrate into the lower ionosphere and ionize the D layer, that layer which acts as a sponge, soaking up radio signals. The more ionized the D layer, the higher the frequencies that are absorbed. Thus, radio signals from distant locations that travel through the daylit ionosphere that is influenced by a flare's x-ray radiation are absorbed and become inaudible. These fade-outs last only minutes for minor flares, to maybe an hour or so for the largest of flares. Once the flare is exhausted, the x-ray radiation fades, and the ionosphere recovers to its normal level of ionization.
If a CME arrives, however, we could see the geomagnetic activity turn stormy, which will cause longer-term degradation of HF propagation, as well as trigger auroral conditions. Geomagnetic activity has the affect of lowering the ionization of the various ionospheric layers, which brings down the maximum usable frequency over a given signal path. This lowering is much like what happens at night, when the ultraviolet radiation of the sun is blocked, and the ionosphere settles down. The stronger and longer the geomagnetic storm, the more depressed the ionospheric propagation becomes.
So, over the course of the next few days, we can expect periods of radio fade-out. If there are coronal mass ejections associated with this flare or new flares, we can expect next week to become a bit rough in terms of overall propagation on MW and HF. However, the stronger the geomagnetic activity, the more likely-hood of some VHF activity via aurora.
The good news? The increase in solar activity is opening up the middle and high portion of the HF radio spectrum. We expect the 10.7cm radio flux to increase to 150 or better over the next week. This is great for DXing on the higher frequencies. Will there be any F layer VHF openings? It is possible!
Let's see what transpires. Tune in and stay alert!
73 de Tomas, NW7US (AAR0JA/AAA0WA)
: Propagation Editor for CQ, CQ VHF, and Popular Communications : : Quarterly Propagation Columnist for Monitoring Times Magazine : : Creator of live propagation center - http://prop.hfradio.org/ : : Member, US Army Miltary Affiliate Radio Service (MARS) AAR0JA : : 122.93W 47.67N / Brinnon, Washington USA - CN87 - CW/SSB/DIGI : : Website, software, database design - http://newwebmakers.com/ : : Washington State Army MARS, State Army MARS Director - AAA0WA : : 10x56526, FISTS 7055, FISTS NW 57, AR Lighthouse Society 144 : _______________________________________________ CQ-Contest mailing list CQ-Contest@contesting.com http://lists.contesting.com/mailman/listinfo/cq-contest
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