‰ Now 18 WPM transition file follows ‰ The Army, Air Force, Navy, Marine Corps and Coast Guard are co sponsoring the annual Military/Amateur Radio Crossband Communications Test in celebration of the 58th anniversary of Armed Forces Day, or AFD. Although the actual Armed Forces Day is celebrated on the third Saturday in May, which is May 17 in 2008, the AFD Military/Amateur Crossband Communications Test will be conducted on May 10 to prevent conflict with the Dayton Hamvention, scheduled for May 16 to 18. For several weeks we expected today, May 2 to have active geomagnetic conditions. For instance, if you look at a forecast from April 23 on the swpc.noaa.gov web site, it shows an expected planetary A index for May 1 to 3 of 10, 20 and 15. The next day, April 24 this changed to 8, 20 and 15, and on April 25 it was 10, 15 and 15. For May 1 we see the actual planetary A index for that day was 9, and for the following two days, the predicted values are 10 and 12, which are much more moderate. So obviously as we moved closer to this date, the return of a solar wind stream seemed less likely, although earlier today the planetary K index rose as high as 4, indicating unsettled to active geomagnetic conditions. The IMF, or Interplanetary Magnetic Field, pointed south when the K index was high, which means our planet was vulnerable to radiation from solar flares and wind streams. Later the IMF pointed north, and the K index dropped to 0, which is very quiet. Nine planetary K index readings from 1500z May 1 through 1500z May 2 went from quiet to active to quiet again, 0, 1, 3, 3, 4, 4, 4, 3 and 0. A solar wind stream flowing from a coronal hole is expected to reach earth on May 5. The expected planetary A index for May 2 to 11 is 10, 12, 12, 8, 10, 8, 5, 5, 5 and 5. That forecast is from the NOAA Space Weather Prediction Center and the U.S. Air Force. Those numbers are from the May 1 prediction. You can see the May 2 prediction some time after 2100z today by changing the last element of one of the URLs in the first paragraph from 042445DF.txt to 050245DF.txt. That same forecast from May 1 is now predicting a 10R7 cm solar flux reading of 70 for the next 45 days. But on April 28 they were predicting solar flux to rise to 75 from May 20 to 28. The Solar Department at the Ondrejov Observatory of the Prague Astronomical Institute, part of the Academy of Sciences of the Czech Republic, projects a 10R7 cm solar flux range of 66 to 73 and a sunspot number range of 0 to 25 for May 2 to 8. For the same period Geophysical Institute Prague predicts geomagnetic activity of unsettled to active May 2, active on May 3, unsettled May 4 to 6, quiet to unsettled May 7, and quiet May 8. Now that we have all the sunspot data for April, we can take our monthly look at our 3 month moving average of daily sunspot numbers to give us a hint on where this cycle may be heading. The March 08 figures are an average of daily sunspot data from February 1 through April 30. These numbers are available in teleprinter and packet versions of Propagation Forecast Bulletin ARLP019. We can see that a slight rise in sunspot activity from October levels has flattened. Although another digit isnt really significant, for readers who prefer to parse their parameters more precisely, the December through March averages may be expressed as 8R14, 8R52, 8R39 and 8R36. Sunspot numbers were 11, 0, 0, 0, 0, 0, and 0 with a mean of 1R6. 10R7 cm flux was 70R4, 69R8, 69, 68R1, 68R5, 68R6, and 67 with a mean of 68R8. Estimated planetary A indices were 18, 8, 10, 10, 11, 8 and 9 with a mean of 10R6. Estimated mid latitude A indices were 13, 7, 5, 7, 9, 4 and 4, with a mean of 7‚ ‰ End of 18 WPM transition file ‰