Just a sample of the Echomail archive
Cooperative anarchy at its finest, still active today. Darkrealms is the Zone 1 Hub.
|    LS_ARRL    |    Bulletins from the ARRL    |    3,036 messages    |
[   << oldest   |   < older   |   list   |   newer >   |   newest >>   ]
|    Message 2,555 of 3,036    |
|    Daryl Stout to All    |
|    ARRL Propagation Bulletin    |
|    07 Jan 22 12:14:10    |
      TZUTC: -0600       MSGID: 88.fidonet-ls_arrl@1:2320/33 263db94a       PID: Synchronet 3.19a-Win32 master/4c726caf5 Jan 1 2022 MSC 1928       TID: SBBSecho 3.14-Win32 master/4c726caf5 Jan 1 2022 MSC 1928       BBSID: TBOLT       CHRS: ASCII 1       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, 2022       To all radio amateurs              SB PROP ARL ARLP001       ARLP001 Propagation de K7RA              Sunspot activity was substantially lower this week, but new sunspot       groups emerged on December 31, January 1, January 4, and January 5.       Average daily sunspot number dropped from 110.1 to 36.4, while       average daily solar flux went from 124 to 91.4.              Geomagnetic activity was still fairly quiet, even with a number of       flares and CMEs, with the average daily planetary A index changing       from 6.4 to 7.7, and average middle latitude A index from 4.4 to 6.              Predicted solar flux over the next month shows 10.7 cm flux values       peaking at 120 on January 16-24, and again at 120 in mid-February.              The daily predicted values are 94 on January 7, 96 on January 8-14,       115 on January 15, 120 on January 16-24, 110 on January 25, 100 on       January 26-27, 95 and 90 on January 28-29, 88 on January 30-31, 85       on February 1-5, then 90, 95 and 100 on February 6-8, 115 on       February 9-11, and 120 on February 12-20.              The predicted planetary A index is 5 on January 7-8, then 12, 14 and       8 on January 9-11, 5 on January 12-14, then 8 and 12 on January       15-16, back to 8 again on January 17-18, 5 on January 19-22, 10 on       January 23, 8 on January 24-26, 5 and 10 on January 27-28, 8 on       January 29-30, 5 on January 31 through February 6, 10 on February       7-8, 5 on February 9-10, then 8, 12, 8 and 8 on February 11-14.              From F.K. Janda, OK1HH:              "Weekly Commentary on the Sun, the Magnetosphere, and the Earth's       Ionosphere-January 6, 2022.              "Free continuation of Earth's magnetic field activity predictions,       published between 1978-2022.              "Solar activity is declining as expected. The last of the chain of       active areas on the Sun, which gradually set behind the western limb       of the solar disk, still contributed to the increase in the speed of       the solar wind in the first three days of the new year.              "The activity of the Earth's magnetic field has decreased since       January 4, and MUF values are gradually declining.              "The solar coronal holes, which now extend along the southern half       of the central meridian, should contribute to a slight increase in       the speed of the solar wind in the coming days.              "Best news in conclusion: we expect a recurrent increase in solar       activity around mid-January.              "Note: The website https://www.solarham.net/ is long-term valued not       only by radio amateurs but also by professional astronomers."              I frequently check https://stereo.gsfc.nasa.gov/ to peer over the       Sun's horizon to see what might emerge over the next few days. I       look for those messy white splotches, which may indicate magnetic       complexity and perhaps a returning or emerging sunspot.              Although the image is constantly updated (every few minutes)       presenting views of the Sun in real time, in October 2014       communication with the STEREO-B spacecraft was lost, so we no longer       see a full 360 degree image of the Sun.              https://stereo-ssc.nascom.nasa.gov/behind_status.shtml              I've been wondering how much it would cost to replace the failed       spacecraft, and if there might be any plans to do so. I checked with       someone at NASA, and received this interesting response:              "I don't know exactly how much it would cost to build a single       spacecraft to replace STEREO-B at this point.              "The two spacecraft combined (A and B) were about $550 million back       before STEREO launch in 2006.              "There is no plan to replace STEREO-B, but based on the success of       the STEREO mission there are a lot of people proposing missions       observing the Sun and solar wind from spacecraft at the relatively       stable Sun-Earth L4 and/or L5 points or else other spacecraft       orbiting the Sun. We will see if any of them are funded. The exact       cost would depend on the details of the mission."              L4 and L5 refer to Lagrange points:              https://solarsystem.nasa.gov/faq/88/what-are-lagrange-points/              Jon Jones, N0JK in Lawrence, Kansas wrote:              "January 3 was a big day for the VHF bands.              "The Quadrantid Meteor shower appeared to peak around 2030 UTC       January 3 as per the NASA prediction.              "I logged N0LL/P DM89 (353 miles) at 1950 UTC on 50.260 MHz MSK144.       Then KE8FD (EN80, 779 miles) also 50.260 MSK144. Logged KA9CFD       (EN40, 993 miles) on FT8, too far for ground wave. May have been       meteor enhanced.              "That evening there was a strong sporadic-E opening across North       America. I had a 6 Meter PSK flag from ZF1EJ (EK99, 1573 miles) at       2357 UTC. Later worked N7BHC in rare EL15 (829 miles, Brownsville,       Texas) at 0246 UTC.              "73, Jon N0JK"              Jon writes the monthly "World Above 50 MHz" column in QST, and       operates from EM17 grid square:              https://www.arrl.org/the-world-above-50-mhz              More good 10 meter news from Greg Mitchell, KB1AWM, in Goose Creek,       South Carolina:              "Just wanted to report a very favorable afternoon on 10 meters       12/27. Worked 4 VK stations back to back from South Carolina       starting about 3:30pm local time. Antenna was a simple long wire.       VK4ZC started the run; he copied me at a -06 and I gave him a -15.       VK3BOX, VK2HFP and VK3KJ followed, with the last one issuing me a       +04. Great Christmas surprise on 10M. Over the past several years, I       have never worked that easily into the south Pacific on 10."              On January 6, WJ5O posted to an HF beacon email list:              "It's mid-morning in Southern Alabama and I'm hearing beacon signals       a bit earlier than usual.              "1549-1559 UTC, 6 January 2022, I can hear/identify five 10 meter beacon       signals into EM71as.              "28.2082 AK2F RANDOLPH, NJ 885 miles       28.234 K4DP COVINGTON, VA 534 miles       28.236 W8YT MARTINSBURG, WV 691 miles       28.270 WA3NFV FAIR HILL, PA 838 miles       28.296 W3APL LAUREL, MD 733 miles"              Al, W1VTP in New Hampshire wrote on January 5:              "Don't know if you are interested in 75m local comm or not but last       night was the pits. We did all our communications using the       Washington SDR receiver and it was mostly successful. Point to point       comm useless."              I think what happened was the ionosphere directly above his area was       not dense enough to reflect 75 meter signals. We may think of local       75 meter signals depending on ground wave propagation, but in fact       it may depend on high angle signals reflected from the overhead       ionosphere.              If you would like to make a comment or have a tip for our readers,       please email the author at, k7ra@arrl.net.               For more information concerning shortwave radio propagation, see       http://www.arrl.org/propagation and the ARRL Technical Information       Service web page at, http://arrl.org/propagation-of-rf-signals. For an       explanation of 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. More good       information and tutorials on propagation are at http://k9la.us/.              Instructions for starting or ending email distribution of ARRL       bulletins are at http://arrl.org/bulletins .              Sunspot numbers for December 30, 2021 through January 5, 2022 were       77, 53, 52, 25, 12, 12, and 24, with a mean of 36.4. 10.7 cm flux       was 102.4, 101.5, 93.9, 89, 84, 85.5, and 83.7, with a mean of 91.4.       Estimated planetary A indices were 8, 4, 11, 10, 12, 6, and 3, with       a mean of 7.7. Middle latitude A index was 7, 2, 9, 7, 9, 5, and 3,       with a mean of 6.       NNNN       /EX       --- SBBSecho 3.14-Win32        * Origin: The Thunderbolt BBS - Little Rock, Arkansas (1:2320/33)       SEEN-BY: 1/123 14/0 15/0 19/33 90/1 105/81 106/201 120/340 123/131       SEEN-BY: 153/7715 226/30 227/114 229/424 426 664 700 240/5832 249/206       SEEN-BY: 249/317 266/512 282/1038 301/1 317/3 320/219 322/757 342/200       SEEN-BY: 633/280 712/848 2320/33 105       PATH: 2320/33 229/426           |
[   << oldest   |   < older   |   list   |   newer >   |   newest >>   ]
(c) 1994, bbs@darkrealms.ca