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|    Message 153 of 3,036    |
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|    ARLP001    |
|    07 Jan 11 18:45:02    |
      SB PROP @ ARL $ARLP001       ARLP001 Propagation de K7RA              ZCZC AP01       QST de W1AW        Propagation Forecast Bulletin 1 ARLP001       From Tad Cook, K7RA       Seattle, WA January 7, 2011       To all radio amateurs               SB PROP ARL ARLP001       ARLP001 Propagation de K7RA              Average daily sunspot numbers were up nearly 24 points this week to       50, and average daily solar flux rose over 9 points to 89.5. The       lagging 3-month average of daily sunspot numbers was down 3.5 points       from last month's average of the previous three months. The three       month moving average of daily sunspot numbers, ending on June       through December was 16.2, 20.4, 23.2, 28.9, 33, 35.6 and 32.1.              The latest forecast from NOAA/USAF for the near term has a solar       flux of 88 on January 7, 86 on January 8-9, 84 on January 10, 82 on       January 11, 80 on January 12-15 and 78 on January 16-18, 80 again on       January 19-25, 88 on January 26-30, and 90 on January 31 through       February 2. Planetary A index is predicted at 7 on January 7, 10 on       January 8-10, 8 on January 11 and 5 on January 12-19.              The geomagnetic prediction from Geophysical Institute Prague is       quiet to unsettled January 7, unsettled January 8-9, quiet to       unsettled January 10, and quiet January 11-13.              Yekta Gursel, KJ6DRO alerted us to an article in the February 2011       issue of "Sky and Telescope" titled "The Perfect Solar Superstorm."       You can read most of it online by going to       http://www.nxtbook.com/nxtbooks/newtrack/st_201102/#/28 and clicking       on "Preview" if you are not a subscriber. Your local library may       also provide online access to the magazine. The article begins on       page 28.              David Moore, who is not a radio amateur but has a keen interest in       all things solar, sent a link to a National Science Foundation       article on why the corona of the Sun is millions of degrees hotter       than the surface. You can read it at       http://www.nsf.gov/news/news_summ.jsp?cntn_id=118338.              Ken Lappe, W1YO of Leesburg, Florida is puzzled by the lack of HF DX       during this time when we have sunspot activity. He wrote, "The past       few days Jan 3, 4 and 5, the sunspot number has been in the 50 range       and the solar flux in the low 90s with very low A and K indices.       All indications suggest at least fair conditions on the higher       bands. But this is not the case. Yes we hear some sporadic-E at       times and some trans-equatorial propagation at times on 12 and 10       meters. But otherwise the bands are dead, or so it seems. ZL4WW was       weak here in central Florida on 12 meters yesterday around 1900z,       but nothing else was heard. Even 17 meters has been quiet in the       afternoon and nothing special in the mornings. So, the question is:       If we have sunspots and solar flux and quiet As and Ks where is the       DX?"              It may just be a combination of seasonal Winter conditions and       sunspot activity not high enough to support much long distance       propagation. A look at a propagation program, such as W6ELprop, is       instructive.              Using a predicted smoothed sunspot number of 39 for January 5 (see       http://www.swpc.noaa.gov/weekly then go to page 11 of the January 4       edition for the source) from Ken's Florida location to New Zealand,       12 meters looks marginal. 17 meters looks good over that path, but       only from 0200-0500z.              Look a few months ahead to April, and with a smoothed sunspot number       of 51, conditions look considerably better.              Now 12 meters opens 1930-0300z, and 17 meters is open during Ken's       local evening until 0530z.              But perhaps Ken is accustomed to better HF openings at this time of       year with this level of solar activity. In that case, I don't know.              Walt Knodle of Bend, Oregon wrote on January 2, "I had an       interesting experience on 40 meters this morning, interesting       because of the timing relative to reading an article by K9LA on skew       paths in the January 2011 World Radio Online.              "That article was directed toward 160 meter propagation, but seemed       appropriate for conditions on 40 meters today. While listening for       VU2GSM I noticed his signal was stronger along the long path than       the short path. However, the LP was almost entirely in daylight so       something else was at play. In swinging the beam toward the LP I       could hear Kanti's signal pass through a very definite peak between       the SP and LP headings. The best heading was directly SW of my QTH       and along the grey line. Assuming a refraction point near the       equator, this would follow Carl's example from the WRO article and       implicate the equatorial ionization anomaly. One side benefit of the       skew path was that it placed the Chinese OTH radar at 90 degrees to       my beam heading."              If you would like to make a comment or have a tip for our readers,       email the author at, k7ra@arrl.net.              For more information concerning radio propagation, see the ARRL       Technical Information Service web page at       http://arrl.org/propagation-of-rf-signals. For an explanation of the       numbers used in this bulletin, see       http://arrl.org/the-sun-the-earth-the-ionosphere. An archive of past       propagation bulletins is at       http://arrl.org/w1aw-bulletins-archive-propagation. Find more good       information and tutorials on propagation at       http://mysite.ncnetwork.net/k9la/index.html.              Monthly propagation charts between four USA regions and twelve       overseas locations are at http://arrl.org/propagation.              Instructions for starting or ending email distribution of ARRL       bulletins are at http://arrl.org/bulletins.              Sunspot numbers for December 30 through January 5 were 24, 23, 65,       38, 51, 54, and 50, with a mean of 43.6. 10.7 cm flux was 82.9,       90.9, 91, 91.1, 92.1, 90.6 and 87.7 with a mean of 89.5. Estimated       planetary A indices were 5, 4, 3, 3, 4, 4 and 2 with a mean of 3.6.       Estimated mid-latitude A indices were 4, 2, 2, 3, 3, 3 and 2 with a       mean of 2.7.       NNNN       /EX              ---        ========              IF you have questions or concerns regarding the accuracy       of information posted, or the opinions expressed, contact the content       originators directly. All publications retransmitted as       fidonet echomail without alteration other than the removal of       email header and other control information which       is not part of the actual publication.              Providing emergency communications assistance to your       neighbors and community isn't just a good thing to do, it's       the first and foremost activity recognized in the U.s. rules       governing amateur radio in 47 CFR section 97.1. IF you enjoy       amateur radio remember that this is an obligation you       tacitly agreed to when you acquired your license.                            ---        * Origin: RRN BBS: Your fidonet ham radio connection! (1:116/901)    |
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