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The SolarCycle24.com Daily for September 5, 2010

SolarCycle24.com Latest Update

Solar Update - B-Class flare activity continues as Region 1105 remains a fairly decent cluster of small sunspots. There is a chance for a C-Class flare.

Sunspot 1101 is about to rotate onto the western limb and will soon be out of direct earth view.

A CME took place on Saturday, but was a limb event. This will have no impact on earth.

Sunspots (Sunday)



WWV
:Product: Geophysical Alert Message wwv.txt
:Issued: 2010 Sep 05 1206 UTC
# Prepared by the US Dept. of Commerce, NOAA, Space Weather Prediction Center
#
#          Geophysical Alert Message
#
Solar-terrestrial indices for 04 September follow.
Solar flux 82 and mid-latitude A-index 1.
The mid-latitude K-index at 1200 UTC on 05 September was 1 (5 nT).

No space weather storms were observed for the past 24 hours.

No space weather storms are expected for the next 24 hours.






Previous 5 Days Solar Data
:#                         Sunspot       Stanford GOES14
#           Radio  SESC     Area          Solar  X-Ray  ------ Flares ------
#           Flux  Sunspot  10E-6   New     Mean  Bkgd    X-Ray      Optical
#  Date     10.7cm Number  Hemis. Regions Field  Flux   C  M  X  S  1  2  3
#---------------------------------------------------------------------------
2010 08 31   75     27      220      0    -999   A6.7   0  0  0  0  0  0  0
2010 09 01   76     51      270      2    -999   A6.4   0  0  0  0  0  0  0
2010 09 02   77     52      180      1    -999   A5.9   0  0  0  0  0  0  0
2010 09 03   77     54      180      0    -999   A7.2   0  0  0  0  0  0  0
2010 09 04   82     53      200      0    -999   B1.0   0  0  0  4  0  0  0


Daily Flux Reading
fluxdate    fluxtime    fluxjulian    fluxcarrington  fluxobsflux  fluxadjflux  fluxursi  
----------  ----------  ------------  --------------  -----------  -----------  ----------
20100901    170000      2455441.197   2100.846        0076.6       0078.0       0070.2    
20100901    200000      2455441.322   2100.851        0076.3       0077.7       0069.9    
20100901    230000      2455441.447   2100.855        0075.8       0077.1       0069.4 


NOAA Solar Report
Prepared jointly by the U.S. Dept. of Commerce, NOAA,
Space Weather Prediction Center and the U.S. Air Force.
Updated 2010 Sep 04 2201 UTC

Joint USAF/NOAA Report of Solar and Geophysical Activity
SDF Number 247 Issued at 2200Z on 04 Sep 2010

IA.  Analysis of Solar Active Regions and Activity from  03/2100Z
to 04/2100Z:  Solar activity was very low. Regions 1105 (N18W36) and
1101 (N12W70) produced several B-class x-ray events during the
period. The largest event, an impulsive B6 flare, occurred at
04/07Z.  A filament was observed on SDO AIA 193 lifting from the
north west quadrant at 04/1430Z. A limb event CME was visible in
SOHO LASCO C3 shortly after with an estimated speed of 368 km/s. The
same event was visible on the STEREO-A coronagraph and produced a
partial halo in the southeast quadrant.

IB.  Solar Activity Forecast:  Solar activity is forecast to be low
with C-class flares likely for the next 3 days (5-7 September).

IIA.  Geophysical Activity Summary 03/2100Z to 04/2100Z:
The geomagnetic field was quiet.

IIB.  Geophysical Activity Forecast:  The geomagnetic field is
forecast to be quiet to unsettled with the chance for active
conditions for the next 3 days (5-7 September) due to recurrent
coronal hole effects.

III.  Event Probabilities 05 Sep-07 Sep
Class M    15/15/15
Class X    01/01/01
Proton     01/01/01
PCAF       Green

IV.  Penticton 10.7 cm Flux
Observed           04 Sep 082
Predicted   05 Sep-07 Sep  084/084/082
90 Day Mean        04 Sep 078

V.  Geomagnetic A Indices
Observed Afr/Ap 03 Sep  003/004
Estimated Afr/Ap 04 Sep  001/005
Predicted Afr/Ap 05 Sep-07 Sep  008/008-008/008-008/008

VI.  Geomagnetic Activity Probabilities 05 Sep-07 Sep
A.  Middle Latitudes
Active                40/40/40
Minor storm           10/10/10
Major-severe storm    05/05/05
B.  High Latitudes
Active                50/50/50
Minor storm           20/20/20
Major-severe storm    10/10/10










W1AW Propagation Bulletin de K7RA (Updated every Friday)

Over this past week, four new sunspot groups appeared. Group 1101 was already in place since August 24, and 1102 emerged on August 29. On September 1, two new sunspot groups -- 1103 and 1104 -- appeared, and on September 2, sunspot group 1105 arrived. Through August 26-September 2, the daily sunspot numbers were 23, 11, 11, 25, 28, 27, 51 and 52 and these same eight days saw the relative total size of all the spots (in millionths of a solar hemisphere) at 100, 100, 130, 170, 180, 220, 270 and 180. The average daily sunspot numbers for August 26-September 1 rose more than 17 points to 25.4, when compared to the previous seven day period. Geomagnetic indicators began the week showing unsettled conditions, but they calmed down to quiet levels again.

Now that August is over, we can look at average sunspot numbers for the previous few months. The three month trailing average of daily sunspot numbers ending in August was 23.2. This is up from the previous two periods ending in June and July, but lower than earlier this year. The three month trailing averages of daily sunspot numbers ending in March-August was 25.7, 22.3, 18.9, 16.4, 20.4 and 23.2.

US Navy and NOAA predict solar flux values of 78 for September 3-4, 76 on September 5-10, 8 on September 11 and 80 on September 12-14. The predicted planetary A index for the same period is 5 on September 3-4, 8 on September 5-7 and 5 on September 8-14. Geophysical Institute Prague predicts quiet conditions on September 3-4, unsettled September 5, quiet September 6, quiet to unsettled September 7 and quiet September 8-9.

Robert Wood, W5AJ, of Midland, Texas, wrote: “Are we now two Sun rotations from the famed WW SSB contest weekend? And is that any indication of conditions for that weekend?”

Two solar rotations is about 55 days, which would be Thursday, October 28, just before the CQ World Wide SSB weekend. I don’t think we can project ahead based on current conditions because we’re not seeing any pronounced recurring activity; solar activity is still very low. Two rotations back is Saturday, July 10. Looking back since July 1, we saw sunspot numbers above 40 on July 23-24, August 5-13 and September 1-2. The number 40 is purely arbitrary, of course, but there is no pattern there based on period of solar rotation.

For geomagnetic activity, since July 1 we had planetary A index over 15 on July 27, August 3-4 and August 24-25. The last period is about one solar rotation after July 27, but there wasn’t a period of geomagnetic activity corresponding to early August in early July. In decades past, we’ve seen periods of intense activity that would come around for several solar rotations, but we aren’t currently witnessing any pronounced solar activity.

In an e-mail, Ron Alexander, KD8ID, of Lansing, Michigan wrote: “One of the complaints that fascinates me is ‘the higher bands are not open, or the bands are very poor.’ I have not found this so; there is always a contact to be made during the early morning, day (weekends) or evening on 40 through 10. The key to good propagation, as you know, is the antenna. Amateurs buy top-of-the-line transceivers and don’t put any money into the antenna. Sunspots help a lot, but antenna selection has a lot to do with making contact. Also, power helps, but it does not help you hear someone better. The antenna does and always will. I consistently work VKs and ZLs in the early morning with 200-300 W on 40 phone. I use an antenna at 72 feet that has a 36 foot boom, nine elements, 3 active on 40, 4 active on 20, 17, 15 and 12, and 6 active on 10. They come in loud and strong unless we are having a K index in excess of 4.Of course, not everyone has the luxury of a large beam based on the area they live. The point I am making is, the bands are open, it’s just a matter of having the right thing up in the air to make a go of it. Additionally, one must understand the practice of propagation to know where to go to find contacts. There is a wealth of information out there including SEC/NOAA education on understanding solar cycles, sun spots and solar flux, along with A and K indexes.”

Ah, to have such a nice antenna high in the air! As Ron says, not everyone has the advantage of a large beam, but he is correct that the antenna is all important. Get a nice look at Ron’s antenna and be sure to click on the photo in the upper-right corner for a larger view.

I found a more dramatic view of Ron’s antenna here. On the upper left click, on “Aerial” then select “Bird’s Eye” in the drop-down menu. Ron’s house is the seventh house south of River Ridge Drive, on the east side of Boxwood Lane. Now click on the “+” in the upper left to zoom in and see the antenna clearly. By clicking on E, W or S on the compass rose in the upper left, you can get completely different views of his location. It is a relatively big antenna on a modest sized residential lot.

David Moore sent in an item from the National Science Foundation that mentions lower levels of ultraviolet radiation from the Sun and the effect on the outer atmosphere.

The autumnal equinox is on September 23 this year. This is a great time for HF propagation, and this year we will probably see higher levels of sunspot activity compared to the equinox in 2009. Running comparative studies on W6ELprop between an average sunspot number of 5 and a more optimistic 25 for this year shows improvement from last year’s propagation.

All times, unless otherwise noted, are UTC.

Amateur solar observer Tad Cook, K7RA, of Seattle, Washington, provides this weekly report on solar conditions and propagation. This report also is available via W1AW every Friday, and an abbreviated version appears each Thursday in The ARRL Letter. You can find a guide to articles and programs concerning propagation here. Check here for a detailed explanation of the numbers used in this bulletin. An archive of past propagation bulletins can be found here. You can find monthly propagation charts between four USA regions and 12 overseas locations here. Readers may contact the author via e-mail.