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The K7RA Solar Update
SEATTLE, WA, Feb 10, 2006--Our sun is very quiet. The daily sunspot reading was zero each day from January 29 through February 7! The last time we saw 10 consecutive days with a sunspot number of zero was way back on the other side of the solar cycle, from December 24, 1996 to January 3, 1997. Prior to that, from September 13, 1996 through October 20 1996 were 38 days with a sunspot number of zero. Perhaps a year from now we'll again see a whole month with no sunspots. Compared with last week, the average sunspot number declined by more than 7 points to 1.7. Average daily solar flux was down more than 4 points to 76. Sunspot numbers and solar flux should rise over the next few days, but not by much. Geomagnetic conditions also look quiet, with the next period of high geomagnetic activity set for February 22. This is based upon the previous rotation of the sun. A fascinating e-mail arrived this week from Larry Putman, WB3ANQ, of Pasadena, Maryland. He described working VK6DI in Western Australia on 30 meters using very slow-speed CW (QRSS), while running just 961 microwatts--less than 1 mW--over an 11,558-mile path. Larry used an old Hewlett-Packard HP-3336 signal generator as a transmitter feeding a 30-meter half-wave inverted V. To achieve the low output power and measure it precisely, he used a precision attenuator and measured the signal with an HP-3586C selective level meter. But Larry didn't depend on the station at the far end to copy by ear. In QRSS mode Morse code elements are extended considerably, so the speed can work out to less than one WPM. Deciphering QRSS is accomplished by feeding the audio into a computer sound card, and detecting it with ARGO software. This is the same technique that many very low-frequency (VLF) operators use. There's more information on this mode of communication on the "QRSS and You" Web page. Larry details his operation on his own Web site. You can see the Web page of VK6DI on the receiving end too. And you can learn about the efforts of a group called the QRSS Knights. Also check out ON7YD's page on extreme narrowband techniques. For more information concerning propagation and an explanation of the numbers used in this bulletin see the ARRL Technical Information Service Propagation page. An archive of past bulletins is on the ARRL Web site. Sunspot numbers for February 2 through 8 were 0, 0, 0, 0, 0, 0 and 12, with a mean of 1.7. The 10.7 cm flux was 77.3, 78.7, 77, 76.3, 74.9, 74, and 74, with a mean of 76. Estimated planetary A indices were 3, 4, 4, 3, 12, 4 and 3, with a mean of 4.7. Estimated mid-latitude A indices were 1, 3, 3, 3, 11, 4 and 2, with a mean of 3.9. (K7RA, ARRL) dxAce Michigan USA |
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