In your opinion what's the best band at this solar period. I just read on
Discovery that we are at the peak about now and it will get to its best until 2015 The 2 meter does not seen to be at risk, MC-kb7dpc _______________________________________________ Elecraft mailing list Post to: [hidden email] You must be a subscriber to post to the list. Subscriber Info (Addr. Change, sub, unsub etc.): http://mailman.qth.net/mailman/listinfo/elecraft Help: http://mailman.qth.net/subscribers.htm Elecraft web page: http://www.elecraft.com |
mc wrote:
> In your opinion what's the best band at this solar period. I just read > on Discovery that we are at the peak about now and it will get to its > best until 2015 > > The 2 meter does not seen to be at risk, > > MC-kb7dpc 20M during the day, Also 30M. 80 and 40 at night. However, Discovery had the "11 year" cycle a bit out of whack if that's what they say. We should be at the bottom of the cycle next year (2006), so by 2011-2012 we should be back working DX on 10M again. By 2015 it will be on the downslide, again. -- _ _ _ _ _ / \ / \ / \ / \ / \ John L. Sielke ( W ) ( 2 ) ( A ) ( G ) ( N ) http://w2agn.net \_/ \_/ \_/ \_/ \_/ "CRUSTY OLD CURMUDGEON - AND PROUD OF IT!" _______________________________________________ Elecraft mailing list Post to: [hidden email] You must be a subscriber to post to the list. Subscriber Info (Addr. Change, sub, unsub etc.): http://mailman.qth.net/mailman/listinfo/elecraft Help: http://mailman.qth.net/subscribers.htm Elecraft web page: http://www.elecraft.com |
In reply to this post by mc-20
MC:
We are either at or near the minimum of the sunspot cycle. Depending on whose projections you believe, we're there right now, or will be there within the next year. Since there is considerable weekly/monthly fluctuation in sunspot activity it will not be until maybe two years from now that the astronomers who do the curve fitting for Uncle Sam can look at the data after the fact and point to a time that was the definitive minimum. There are two practical effects of low sunspot activity. One is that the Maximum Usable Frequencies (MUF) are low, and solar flare activity is usually (but not always) low. The MUF is significant, because long distance HF propagation tends to produce the strongest signal near the MUF. Above the MUF, the band simply does not come open. Solar flare activity, and the consequent geomagnetic activity, typically disrupts long distance HF propagation, but will often cause unusual long distance openings on VHF. What does that mean in answer to your question? Local 2-meter activity will be unaffected by anything but extremely severe solar flare activity. Thus, local 2-meter activity will be largely reliable. The relative paucity of solar flares will also mean that long distance VHF modes like auroral propagation will be fairly uncommon for the next few years. For the next couple of years for long distance propagation at HF, 10 meters will open only rarely. 15 meters will be mostly limited to afternoon transequatorial openings. 20 meters will be open during the daytime, and extending into the evening especially during the summer. 40 meters will probably provide the most reliable long distance communication for the longest periods (i.e., During the winter 40 will go dead to long distance communications from about 9 am to 3 pm local time, but be open to DX the rest of the time.). However, there will be times when the MUFs along interesting paths will fall below 6 MHz, then 80 m will be the best bet. Note that on the gray line (both stations on the day-night terminator) brief openings on 80 or 40 meters can be remarkable. Historically, the sunspot cycle follows a 22 year period, and within that period there are two 11 year subcycles, one tending to have a weaker sunspot maximum that the other. This also means that solar minima recur about every 11 years. That means that conditions in 2016 should be a lot like they are right now. In 2015, they should be far down the hill, but not at rock bottom. 1991 seemed to be a relatively good solar maximum. Many hams with very simple gear and antennas were working spectacular DX on 10 meters. I was not active in the 2000-2 period, but I do not hear people telling war stories about their amazingly spectacular operating feats during that time. This is consistent with the historic pattern of a soso solar maximum following a very good one. This suggests that the next maximum, which should occur about 2011-2012, will be better than the last one and should produce very consistent DX on 10 meters, and frequent openings on 6 meters. 73, Steve AA4AK At 05:05 PM 10/15/2005 -0400, mc wrote: >In your opinion what's the best band at this solar period. I just read on >Discovery that we are at the peak about now and it will get to its best >until 2015 > >The 2 meter does not seen to be at risk, > >MC-kb7dpc > >_______________________________________________ >Elecraft mailing list >Post to: [hidden email] >You must be a subscriber to post to the list. >Subscriber Info (Addr. Change, sub, unsub etc.): >http://mailman.qth.net/mailman/listinfo/elecraft > >Help: http://mailman.qth.net/subscribers.htm >Elecraft web page: http://www.elecraft.com _______________________________________________ Elecraft mailing list Post to: [hidden email] You must be a subscriber to post to the list. Subscriber Info (Addr. Change, sub, unsub etc.): http://mailman.qth.net/mailman/listinfo/elecraft Help: http://mailman.qth.net/subscribers.htm Elecraft web page: http://www.elecraft.com |
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