[DX-NEWS] ARLP024 Propagation de K7RA

2013-06-14 Thread jjreisert
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 14, 2013
To all radio amateurs

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

Average daily sunspot numbers declined over 32 points this week to
39.6.  Average daily solar flux was down more than 8 points to 99.2.
Tuesday's solar flux at 89.5 was the lowest since June 22-25 of last
year, when values ranged from 84 to 88.6. Likewise, Tuesday's
sunspot number of 14 was also the lowest since June 25, 2012 when
the sunspot number was also 14. Since then both numbers have been
recovering, with Wednesday and Thursday's sunspot numbers at 27 and
45, and solar flux at 93.3 and 98.9.

The latest prediction has solar flux at 105 on June 14-17, 100 on
June 18-19, 105 and 110 on June 20-21, 115 on June 22-24, 110 on
June 25, 105 on June 26-28, and 110 on June 29 through July 4.
Solar flux is expected to reach a minimum of 95 around July 7-8 and
another peak at 115 on July 18-21. Note that ARRL Field Day is June
22-23, right when solar flux is expected to be highest.

The predicted planetary A index is 5 on June 14-16, 8 on June 17-18,
5 on June 19-20, then 25, 18, 10 and 8 on June 21-24, 5 on June
25-27, then 30, 20, 10 and 8 on June 28 through July 1, 5 on July
2-4, 10 on July 5-6, 8 on July 7, and 5 on July 8 through mid-month.

A geomagnetic forecast comes to us this week from Petr Kolman,
OK1MGW, who sees quiet to unsettled conditions June 14, mostly quiet
June 15-18, quiet to unsettled June 19-20, quiet to active June
21-23, quiet to unsettled June 24, quiet June 25-26, quiet to active
June 27, active to disturbed June 28-29, quiet to unsettled June 30
through July 2, quiet to active July 3-4, mostly quiet July 5-6.

Word has come that the link to the W6ELprop installation file at
http://www.qsl.net/w6elprop/ is broken. Until it is restored you can
find it at ftp://150.214.111.198/pub/ham/propag/W6ELPropInst270.EXE.

Unfamiliar with FTP? FTP is File Transfer Protocol, and you can
paste that link into your web browser URL window, hit Enter, and a
download dialog should appear. W6ELprop works only on Windows
computers, and with it you can predict propagation from your station
to anywhere else, on any frequency between 3-30 MHz. If you have any
trouble installing, try right-clicking the file and running as
administrator.

The latest NASA prediction for Cycle 24 moves the sunspot peak back
to Summer 2013, but NOAA predicts the peak for the end of this year.
Check pages 16 and 17 at
http://www.swpc.noaa.gov/weekly/pdf/prf1970.pdf and note the highest
smoothed sunspot and solar flux numbers are predicted in November
and December 2013. These are smoothed international sunspot numbers,
with a scale quite a bit lower than the Boulder numbers reported
here.

If you would like to make a comment or have a tip for our readers,
email the author at, k...@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. More good
information and tutorials on propagation are at http://k9la.us/.

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 June 6 through 12 were 71, 76, 27, 41, 21, 14,
and 27, with a mean of 39.6. 10.7 cm flux was 109, 109.8, 103.2, 96,
93.3, 89.5, and 93.3, with a mean of 99.2. Estimated planetary A
indices were 17, 32, 10, 9, 13, 6, and 5, with a mean of 13.1.
Estimated mid-latitude A indices were 16, 26, 9, 8, 12, 6, and 5,
with a mean of 11.7.

/EX



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[DX-NEWS] ARLP024 Propagation de K7RA

2012-06-15 Thread jjreisert
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP25
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 15, 2012
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

Solar activity was lower this week, although for the past few days
sunspot numbers and solar flux were rising.

Average daily sunspot numbers declined over 14.3 points to 116.1,
and average daily solar flux was off by 14.5 points to 115.9.  There
were five new sunspot groups this week, two each on June 9-10, and
one more on June 13.

The latest prediction has solar flux at 150 on June 15-16, 145 on
June 17-18, 140 on June 19-20, 130 and 120 on June 21-22, 110 on
June 23-26, 105 on June 27-28, followed by a climb back to 120 on
July 1-12.

Predicted planetary A index is 5 on June 15-16, 18 on June 17, 8 on
June 18, and 5 on June 19-25. The next peak of geomagnetic activity
is predicted for June 30 to July 4 with planetary A index at 8, 15,
12, 10 and 8. Following that is a similar peak on July 15-17 of 15,
12 and 8.  Looking further out, planetary A index of 8, 15 and 12 is
predicted for July 27-29.

The geomagnetic forecast from OK1MGW has quiet to unsettled
conditions June 15-17, quiet to active June 18, active June 19-20,
quiet to unsettled June 21, mostly quiet June 22-23, quiet to
unsettled June 24-29, quiet to active June 30, and active conditions
July 1-3.

The most active days over the past week were June 11-12, when the
planetary A index was 14 and 13.  The high latitude college A index
was 22 and 8 on those days, but the mid-latitude A index numbers
from Fredericksburg, Virginia were only 11 and 10.

We often get messages about Cycle 19, the huge solar cycle which
peaked in 1959, but not so often about the peak of Cycle 18.  W7LTQ,
who lives on Fidalgo Island (IOTA NA-065) in the San Juan
Archipelago and signs his messages "Old Chief Lynn" wrote, "Indeed
Cycle 19 was hot, and perhaps even hotter, judging by 10 meter
operations, was Cycle 18! There were a couple of weeks in the spring
of 1948 when the 10 meter phone band was just one howling mess of
heterodynes (AM was king).  During Cycle 19, working the Tucson
local 10 meter 'short skip' net, there were a couple of early
evenings when stations across town in Tucson, AZ, were working short
skip AND long path propagation simultaneously. That was a strange
echo sounding mess. Turning our beams towards a short skip contact
and 180 degrees away confirmed the phenomenon. I think we were
probably on the so-called Grey Line."

Yes, in the days before SSB phone, a pile of AM signals could sound
quite messy.  By the way, 1948 was the year W7LTQ turned 16 years
old. You can have a look at Cycles 18 and 19 and many others on the
WM7D Historical Solar Charts at
http://wm7d.net/hamradio/solar/historical.shtml.  Cycles 18 and 19
are the fifth and sixth cycle peaks from the left side of the page
in the chart of "Monthly Sunspot Numbers 1900 to 1999."

Regarding the link in last week's Propagation Forecast Bulletin to
the researcher who believes modern sunspot numbers are inflated, Ken
Grimm, K4XL of Amherst, Virginia wrote, "Regardless of what Prof.
Svalgaard's charts and tables show, those of us who lived through
the late 50s and enjoyed the benefits of something that he thinks
didn't happen, know what we experienced.  Nothing since has come
even close to the conditions on the HF bands during those wonderful
days.  Fifty watts of AM on 10 meters was enough to work the world
with honest 5x9 sigs!  Twenty meters was open 24 hours a day and DX
was commonplace, etc.  Nothing can convince me that the late 50s
weren't unusual!"

An interesting article in the popular press appeared this week,
suggesting that long term prediction of solar cycles is impossible.
Read it at,
http://www.telegraphindia.com/1120612/jsp/frontpage/story_15600043.jsp.

Also note toward the end of the article that the student, Bidya
Binay Karak, authored a paper explaining why sunspots disappeared
for a time in 2008-2010.  When I look at his curriculum vitae I see
a paper about the Maunder Minimum, but not about the more recent
quiet Sun. You can check Karak's CV at
http://www.physics.iisc.ernet.in/~bidya_karak/.

Don't miss Carl Luetzelschwab's interesting article in the current
(July 2012) issue of QST, "Our Recent Solar Minimum and Sunspot
Cycle 24 Progress." You'll find it on page 33.

Phil Platt, of the Bad Astronomy blog has a link to a video of an
active sunspot, complete with dramatic music at,
http://blogs.discovermagazine.com/badastronomy/2012/06/14/what-a-dramatic-sunspot/.

Also check
http://cosmiclog.msnbc.msn.com/_news/2012/06/14/12227124-incoming-solar-storms-on-the-way
for a piece on upcoming solar storms.

On June 12, Jeff Hartley, N8II of Shepherdstown, West Virginia
reported, "12 meters has been open to unexpected areas on F2 and
combination Es/F2 paths recently. On the June 9 at 2317 I worked
OM3EY with a S9 CW signal followed by HL2WP S7 at

[DX-NEWS] ARLP024 Propagation de K7RA

2011-06-17 Thread jjreisert
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 17, 2011
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

The average daily sunspot number for the past week declined by more
than half, nearly 52 points to 35.1, when compared to the previous
week.  Average daily solar flux declined nearly 12 points to 90.1.
Note that from Wednesday (the last day for the data reported at the
end of this bulletin) to Thursday of this week the solar flux went
from 101.5 to 103.3 and the sunspot number rose from 48 to 62.

NOAA and the USAF predict rising solar flux for the near term, with
solar flux at 105 on June 17-20, to 110 on June 21-23, 105 on June
24-26 then dipping below 100 after June 28.

Predicted solar flux for ARRL Field Day weekend is 105 on June
24-26.

Predicted planetary A index for June 17-25 is 10, 8, 5, 8, 8, 5, 18,
15 and 10, followed by 5 on each day through the end of June.  It
seems that a recurring coronal hole may disturb our Earth's
geomagnetic field, with the maximum effect on June 23, two days
before Field Day, but geomagnetic conditions should be very quiet by
Sunday, June 26.

Geophysical Institute Prague predicts quiet conditions for June
17-18, quiet to unsettled June 19, active conditions June 20, and
unsettled conditions June 22-23.  For some reason they don't offer a
prediction for June 21.

Big news this week was the report issued from a meeting of the Solar
Physics Division of American Astronomical Society at New Mexico
State University in Las Cruces predicting another Maunder Minimum -
many decades with hardly any sunspots.  There seems to be a
convergence of several lines of thought which all predict this, but
fortunately there are dissenting experts.

Here is the text of the release:

http://www.boulder.swri.edu/~deforest/SPD-sunspot-release/SPD_solar_cycle_release.txt

This contains text and images:

http://www.boulder.swri.edu/~deforest/SPD-sunspot-release/

The web site for the conference:

http://astronomy.nmsu.edu/SPD2011/

Douglas Biesecker of NOAA's Space Weather Prediction Center
questions this hypothesis of disappearing sunspots.  You can read
his notes here:

https://docs.google.com/viewer?a=v&pid=explorer&chrome=true&srcid=0B88iFXWgVKt-NzU0Y2I3M2QtNGNkNS00ZTcyLWIxN2UtOWEwMzNmOTMzOTAx&hl=en_US&pli=1

Or if that doesn't work for you, try this:

http://snurl.com/5qzxf

A slideshow accompanies the notes:

http://www.slideshare.net/Revkin/why-there-is-no-evidence-for-a-new-maunder-minimum-8318340

Here are several articles on related subjects, the first two
contributed by Scott Bidstrup, TI3/W7RI:

http://esciencenews.com/articles/2011/06/14/new.insights.how.solar.minimums.affect.earth

http://www.physorg.com/news/2011-06-scientists-magnetic-ropes-solar-storms.html

http://www.wired.com/wiredscience/2011/06/solar-minimum-climate/

Peter Laws, N5UWY of Norman, Oklahoma wrote: "On the morning of
Memorial Day, May 30, I was alerted to a potential opening on the 2
meter band. I went to the radio room and tuned around. Sure enough -
a W8! I worked W8BYA in EN70 about 1230 km from me in EM15.  My
question is this: Was that a Tropospheric Ducting event or was it
sporadic-E?  It seems to me to be long for Tropo but I don't really
know the upper end for Tropo over land.  Is there some rule of thumb
that operators can use to try to determine which mode made the
contact possible?

"As exciting to me as 2 meter DX contacts are, W8BYA was the only
station I heard on the band!!"

My suspicion is that the mode was sporadic-E, but I don't know.
Maybe some experienced VHF ops can lend an opinion on this.

The July 2011 issue of QST has an informative article by Joel
Hallas, W1ZR on pages 37-38 titled, "Solar Indices - What do they
Mean?"  In the article Joel explains solar flux, sunspot numbers, A
index and K index, and what they mean for the radio amateur.  The
article also gives a nice plug for this bulletin.

Lawrence, GJ3RAX from the Isle of Jersey writes: "Last Friday I had
a phone call from GJ3YHU. That is not unusual as he lives about a
mile from me. This time he was down in Meze in the south of France
where he spends time regularly. He said that he had been hearing
signals on 10 meters and wanted to see if there was a path between
us. I was doubtful that it would be possible as my typical
sporadic-E QSOs are usually to the south of Spain, Gibraltar and
North Africa. The south of France would probably be too close. We
chose a frequency and tried, resulting in a QSO at 5/9 each way.
That lasted for nearly 5 minutes before fading out.

"His equipment was an IC-7000 to a mobile whip. I was using an
IC-756-Pro2 to a Cushcraft R5 which is mounted 10 feet above the
ground here. Using Google Earth I estimated the distance as 485
miles.

"By the time I get to replace my broken beam for 6 m the sporadic-E
season will be over but I should be back on that band and the hi

[DX-NEWS] ARLP024 Propagation de K7RA

2010-06-18 Thread jjreisert
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 18, 2010
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

Average daily sunspot numbers were up 2.5 points from last week,
despite the fact that there were no sunspots at all this week on
June 15-16.  A new sunspot group 1082 emerged yesterday, June 17,
and yielded a daily sunspot number of 14.  A nice thing about this
spot is that it is all the way over on the east side of the visible
solar disk, meaning we will probably see its effects as it moves
across the sun.  All other recent sunspots emerged toward the west
side, which meant that they went over the horizon fairly quickly and
disappeared.

Last week there were four sunspot groups visible at different times.
Group 1078 disappeared on June 12, 1079 and 1080 both were gone on
June 14, and on June 15 1081 was gone.  Geomagnetic activity peaked
on June 16 with the planetary A index at 19 and high latitude
college A index at 42.  This should decline over the next couple of
days.

We did not receive a prediction from Geophysical Institute Prague
this week, but NOAA/USAF say that the expected planetary A index for
June 18-28 is 10, 5, 5, 5, 5, 5, 8, 12, 15, 15 and 8.  This shows
unsettled to active geomagnetic conditions for Field Day weekend,
June 26-27.  The same prediction shows solar flux at 70 on June
18-24, then 75 for June 25-30.

Glen Stuart, N7NRA of Mesa, Arizona sent this in about recent 10
meter activity.  "N7YU, Dave, in Chandler, AZ, and I had QSOs into
Rarotonga last evening on 28.445 at about 0045Z, 14 June.  The op on
the other end was E51JD, Jim.  There was some QSB, but we were
reporting 57 on both ends.  I don't know how much power Dave was
running.  I was using 100W.  We both use Butternut HF-9Vs.  His is
ground mounted, mine is roof mounted with the base at about 15 feet
above ground.  When I built my shop I had the roofers install a
carpet of chicken wire between the shingles and the tar paper. My
counterpoise is about 16 x 50 feet and works well. Things are
looking up for the higher frequencies".

On that same date, June 14, the K0KP six-meter beacon was copied in
the Netherlands.  Rex Greenwell, K0KP lives in Duluth and operates a
100 watt beacon on 50.073 MHz at the 50 foot level on a commercial
broadcast tower in grid square EN36wt.  Here is the message from
Rex.

"This is an email I received from PF7M today - Netherlands.  This
was at 01:50 AM Central time.  6M - Europe to Minnesota in the wee
hours of the AM. - Rex K0KP EN36 20 mi. NW of Duluth, MN.

Hello Rex, This morning round 06.50 UTC I have received your K0KP/B
beacon on 50.073MHZ. Just audible at 419 with my 6 element Yagi at
20 meters.  Locator here: JO33BA.  6 meters was open from here to GM
and OY, so think it was some extended Es into EN36.  Not any NA
present on 6M at this time.  73's Johan - PF7M"

Several readers sent in links to articles on our sun's recent
strange behavior, including this one, http://tinyurl.com/27nogws and
this one http://shar.es/myBSb on the NASA Solar Observatory.  In
last week's bulletin we raised the question about adjusted solar
flux values, and why they are adjusted to compensate for the
variation in the distance between earth and sun.  The solar flux
values we present here are the values as measured at the observatory
in Penticton, British Columbia.  You can see them at
http://tinyurl.com/ks8tvn.  They come from the 2000z reading in the
third column from right, with the heading fluxobsflux.  The next
column to the right, fluxadjflux, is the adjusted value.  They are
adjusted up or down to reflect a value based on the average distance
of our planet from our sun.

On 6-17-2010 at 2000z the raw observed value was 70.4, and the
adjusted value was 72.7.  This is because we are now further away
from the sun than other times of the year.  Of course, we are
interested in the observed value, because that is a measure of the
radiation hitting our ionosphere.  But if we wanted to keep track of
adjusted solar flux to gauge solar activity, this would show us more
realistically what the sun is actually doing.  Back on April 5 the
observed and adjusted readings show the same value, but in January,
we were closer to the sun, so the value was adjusted downward.

This weekend is the All Asia CW DX Contest, and HF conditions should
be fair.  There are no predicted geomagnetic disturbances.

The new issue of WorldRadio online should be out this Sunday, June
20, and there is always an informative column on propagation by
K9LA.  Check it on Sunday at http://www.worldradiomagazine.com/.
 
If you would like to make a comment or have a tip for our readers,
email the author at, k...@arrl.net.

For more information concerning radio propagation, see the ARRL
Technical Information Service at
http://arrl.org/propagation-of-rf-signals. For an explanation of the
numbers used in this bulletin,

[DX-NEWS] ARLP024 Propagation de K7RA

2009-06-12 Thread jjreisert
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 12, 2009
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

Sunspot numbers from May 31 through June 5 ranged from 13 to 23,
then the Sun was blank for two days, followed by sunspot numbers of
12 for both June 8 and 9.  This fleeting sunspot was number 1020,
and like last week's spot, 1020 had the magnetic signature of a new
Cycle 24 spot.  Alas, it was another of the frequent sunspots we've
seen lately which appear briefly, then vanish.

The last Cycle 23 spot was number 1016, which appeared April 29-30.

Leonard Halversen, WA2AMW of Princeton, New Jersey asked how Cycle
24 spots are differentiated from Cycle 23 spots, and we last
mentioned this in Propagation Forecast Bulletin ARLP044 from 2008,
so now is a good time to go over it again.

The sunspots have a magnetic signature.  As you watch them move from
left to right, they lead with a dark patch in front and a white tail
in the rear.  That is how Cycle 24 spots appear above the equator,
and it is just the opposite south of the Sun's equator.  Also, new
cycle spots tend to appear at higher northern or southern latitudes
away from the equator, while old cycle spots appear nearer the
equator.

Go to http://sohowww.nascom.nasa.gov/data/realtime/ to look for
images.  Click on the "Search and Download Images" link, and select
MDI Magnetogram from the image types.  Try entering start/end dates
of April 28 and April 30 of this year, and click Search.  Select one
of the links from the middle of the list, and note that the sunspot
on the right side is near the equator, indicating a spot from the
old cycle, and that it leads with black on the right.  Because it is
slightly below the equator, this indicates a Cycle 23 spot.  If it
were above the equator, a Cycle 23 spot would lead with white on the
right side.

Now go back and search dates June 1 through June 3.  Note that you
can up the resolution to 1024 from 512.  Select one of these images,
and note the large sunspot above the equator has a Cycle 24
signature.

Still more comments arrived this week about how dead bands may be an
illusion.  Guy Cossette, VA2WT of Saint Roch de Mekinac in Quebec
wrote to tell us about his 80 and 40 meter operation.  Using 100
watts CW and a 40 meter dipole, he worked Crete, Cyprus and Tunisia
at 2200z and he also worked Cyprus on 80 meters at 2300z.

Ken Sturgill, WS4V in Marion, Virginia says he likes to use the
intelligent features at http://www.ve7cc.net/.  If you wish, you can
set it for the countries you are looking for, and you can also set
it to only accept spots from tipsters in your country, so you get
the spots you can work.  He recommends hitting the "Tell Cluster"
button often, so the info isn't lost.  He also recommends reading
the manual.

Jim Sullivan, N7TCF of Phoenix, Arizona likes to use "DX Sherlock,"
at http://www.vhfdx.net/spots/map.php.  He uses it to check out band
conditions, mainly on 6 meters.  One feature I like is the Es MUF
tab, where you can see the MUF in various places.  I believe this
data comes from ionospheric sounders (ionosondes), which fire a
sweeped RF signal straight up and then measure the strength and
frequency of the signals bouncing back.

Mark Lunday, WD4ELG of Hillsborough, North Carolina sent a link to a
nice map mash-up of 6 meter beacon stations at,
http://www.k9mu.com/map/.  Mark wrote:

"I have also been experimenting with WSJT weak signal software from
Joe Taylor, K1JT.  It's pretty neat to tinker with meteor scatter on
6 meters, and very challenging with my modest station.  But I have
really gotten addicted to JT65A mode on 20 meters.  There always
seems to be somebody on the air in the vicinity of the calling
frequency of 14076 kHz, and I have worked some terrific DX that I
normally would struggle with from here with 20 watts.  I have also
heard DU on JT65A for the first time ever on any band or mode!  All
of my QSOs have been with 40 watts or less, mostly with 20 watts.
In just two months of part-time operation, I have worked 25
countries on JT65A including VK, JA, CX, lots of Europeans.  Also, I
worked ZS6 on 80 meter WSJT last weekend!  There were horrendous
thunderstorms all up and down the east coast, but the software
decoded just fine.  I could barely see the DX on the WSJT spectrum
waterfall, and decoded his CQ almost by accident while doing
something else in the shack."

For this week, geomagnetic conditions should remain very quiet.
Solar flux is estimated to be about 68, rising above 70 June 24
through July 1.

If you would like to make a comment or have a tip for our readers,
email the author at, k...@arrl.net.

For more information concerning radio propagation, see the ARRL
Technical Information Service web page at,
http://www.arrl.org/tis/info/propagation.html.  For a detailed
explanation of the numbers used in this bulletin, see
http:/

[DX-NEWS] ARLP024 Propagation de K7RA

2008-06-06 Thread jjreisert
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 6, 2008
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

We had seven days of no sunspots this week, but a sunspot was
emerging on Thursday, June 5.  Helioseismic holography revealed a
high latitude sunspot on the opposite side of the Sun.  Until
recently, we had no idea what was happening on the far side of the
Sun, the side directed away from earth.  Go to
http://www.spaceweather.com/glossary/farside.html and to
http://solarscience.msfc.nasa.gov/Helioseismology.shtml for more
information on helioseismology.

Sorry about my mix-up last week, which some readers saw in some
versions of the bulletin regarding Labor Day.  No, it is not
celebrated in May.  If you didn't see it, then you read a version
edited by the very capable and wide awake staff at ARRL HQ.

As promised last week, here is an update to the three-month moving
averages of sunspot numbers.

Sep 05 39.3
Oct 05 28
Nov 05 36
Dec 05 40.6
Jan 06 32.4
Feb 06 18.1
Mar 06 27.7
Apr 06 38.5
May 06 39.7
Jun 06 28.9
Jul 06 23.3
Aug 06 23.5
Sep 06 21.2
Oct 06 24.1
Nov 06 23.1
Dec 06 27.3
Jan 07 22.7
Feb 07 18.5
Mar 07 11.2
Apr 07 12.2
May 07 15.8
Jun 07 18.7
Jul 07 15.4
Aug 07 10.2
Sep 07  5.4
Oct 07  3
Nov 07  6.9
Dec 07  8.1
Jan 08  8.5
Feb 08  8.4
Mar 08  8.4
Apr 08  8.9

I was able to calculate the value for April because we have all the
data for March, April and May.  The total of all daily sunspot
numbers for those three months was 818.  Divide that value by 92
days gives us approximately 8.891 as the average.

Note the average sunspot number has increased only slightly since
last Fall.

Jeff Lackey, K8CQ of St. Simons Island, Georgia noted that in the
table of zero-sunspot days presented last week, there was at least
one error.  They counted as 36 days the period from May 27 to July
31, 1996.  You can look at the whole website, not just the page we
linked to last week at,
http://users.telenet.be/j.janssens/Spotless/Spotless.html.  Jeff
checked data in the table against an archive of sunspot data on the
ftp site, ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SUNSPOT_NUMBERS/.
He found that the 66 days they reported as 36 days were actually
over two periods, but neither was over 20 days.  Jeff wrote,
"Indeed, the run that ended on 31 July began on 8 July, thus it was
a 14 day run.  The beginning date of 27 May was for a run that ended
on 7 June.  Between 7 June and 8 July, the sunspot numbers were all
non-zero."

The NOAA Space Weather Prediction Center sees a constant and quiet
geomagnetic planetary A index of 5 through June 14.  Geophysical
Institute Prague predicts quiet conditions for June 6, quiet to
unsettled June 7-8, and quiet again June 9-12.

If you would like to make a comment or have a tip for our readers,
email the author at, [EMAIL PROTECTED]

For more information concerning radio propagation, see the ARRL
Technical Information Service web page at,
http://www.arrl.org/tis/info/propagation.html.  For a detailed
explanation of the numbers used in this bulletin see,
http://www.arrl.org/tis/info/k9la-prop.html.  An archive of past
propagation bulletins is at http://www.arrl.org/w1aw/prop/.  Monthly
propagation charts between four USA regions and twelve overseas
locations are at http://www.arrl.org/qst/propcharts/.

Instructions for starting or ending email distribution of this
bulletin are at, http://www.arrl.org/w1aw.html#email.

Sunspot numbers for May 29 through June 4 were 0, 0, 0, 0, 0, 0, and
0 with a mean of 0.  10.7 cm flux was 68.1, 67.1, 66.9, 66.6, 67.1,
66.3, and 65.2 with a mean of 66.8.  Estimated planetary A indices
were 9, 11, 8, 8, 5, 4 and 4 with a mean of 7.  Estimated
mid-latitude A indices were 7, 7, 8, 6, 4, 3 and 2, with a mean of
5.3.

/EX




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[DX-NEWS] ARLP024 Propagation de K7RA

2007-06-08 Thread jjreisert
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 8, 2007
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

After five days of no sunspots from May 24-28, spots returned on May
29, and have increased since in number and size.  There are
currently several sunspots visible, and the sunspot number for the
past five days (Sunday through Thursday) was 58, 58, 63, 47 and 59.
Coupled with quiet and stable geomagnetic indicators, this is good
for HF propagation.  Our reporting week for this bulletin (the
numbers reported at the end) runs from Thursday through Wednesday,
and the average daily sunspot number for May 31 to June 6 rose
nearly 43 points to 46.1 when compared to the prior seven days.
Average daily solar flux rose nearly 15 points to 83.7.

Last week's Propagation Forecast Bulletin ARLP023 mentioned ARRL
Field Day, now just two weeks away.  The bulletin reported (in some
uncorrected versions) that the event is always held on the last full
weekend in June, but Don Jackson, AE5K of Marion County, Arkansas
pointed out that the rules specify the fourth full weekend.  Both
fourth and last are on the same weekend this year (June 23-24),
which is usually the case, but not always.  In 2002, the fourth full
weekend was June 22-23, but the last full weekend was June 29-30.
This occurs whenever June 1 is a Saturday, as it will be again in
2013 and 2024.

Last week the latest projection looked like no sunspots around Field
Day with a declining geomagnetic disturbance, but this week the
forecast looks a little better.  Including the Friday before (the
event doesn't begin until Saturday) the projected solar flux last
week for June 22-24 was 65 for all three days, with a planetary A
index of 20, 12 and 5.  This week's prediction for those dates shows
the same A index, but a solar flux 10 points higher, at 75 for all
three days.

A check of recent sunspot numbers alongside solar flux values on the
same dates at, http://www.sec.noaa.gov/ftpdir/indices/DSD.txt, shows
no sunspots when the solar flux was down around 65, but at 75 the
sunspot number can be in the 40s.

For the next few days expect continued quiet geomagnetic activity,
with the same moderate (for the low point of the sunspot cycle)
sunspot count.

Alex Mendelsohn, AI2Q in Kennebunk, Maine sent a link to an article
about a solar burst last December 6, which caused problems for GPS
receivers.  You can read it at, http://tinyurl.com/389ngn.  See how
we reported the same flare at,
http://www.arrl.org/w1aw/prop/2006-arlp051.html.  Our bulletin shows
that the solar flux observatory in British Columbia also had
problems from that event.

If you would like to make a comment or have a tip for our readers,
email the author at, [EMAIL PROTECTED]

For more information concerning radio propagation, see the ARRL
Technical Information Service at,
http://www.arrl.org/tis/info/propagation.html. For a detailed
explanation of the numbers used in this bulletin, see
http://www.arrl.org/tis/info/k9la-prop.html. An archive of past
propagation bulletins is at, http://www.arrl.org/w1aw/prop/ .
Monthly propagation charts between four USA regions and twelve
overseas locations are at, http://www.arrl.org/qst/propcharts/.

Sunspot numbers for May 31 through June 6 were 11, 41, 45, 58, 58,
63 and 47 with a mean of 46.1. 10.7 cm flux was 74.6, 79.4, 83.2,
87, 85.7, 88.8, and 87.1, with a mean of 83.7. Estimated planetary A
indices were 4, 6, 7, 10, 8, 3 and 2 with a mean of 5.7. Estimated
mid-latitude A indices were 2, 5, 5, 7, 8, 2 and 2, with a mean of
4.4.

/EX




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[DX-NEWS] ARLP024 Propagation de K7RA

2006-06-16 Thread W1AW
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 16, 2006
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

Solar activity continues at very low levels. Andy Gudas, N7TP of
Nevada (see http://www.n7tp.org) was wondering about the bottom of
the solar cycle, and noted that we still see solar flux values in
the seventies. We're probably not at the bottom of the cycle yet,
because during long periods of 0 sunspots at solar minima, we
observe solar flux values around 66-67.

Check out the numbers at the bottom of Propagation Forecast Bulletin
ARLP043 from 1996, when there were no sunspots for weeks on end. It
is located at, http://www.arrl.org/w1aw/prop/1996-arlp043.html.

Five days from now is the longest day of the year in the Northern
Hemisphere. We're moving from spring to summer propagation
conditions. A couple of things you might notice compared to a few
months ago. 80, 60 and 40 meters will be open for shorter hours due
to less hours of darkness. You can also look forward to long
distance 20 meter openings later into the evening.

This becomes more noticeable at northern latitudes, where the days
are longer than down south. For instance, on the summer solstice
next Wednesday, Costa Rica will have about 12 hours and 33 minutes
from sunrise to sunset, but the same day in Vancouver, British
Columbia will be about 16 hours long.

6 meter reports continue to roll in. Chip Margelli, K7JA passed
along a rumor that ARRL President Joel Harrison, W5ZN worked 123
Japanese stations on 6 meters in one evening recently. I've been
unable to confirm this directly.

David Greer, N4KZ of Frankfort, Kentucky writes, "6 meters continues
to dazzle from Frankfort, KY, EM78. I worked 17 stations in
Washington, Oregon and Idaho on SSB between 0025 and 0130z on June
15. Most signals were strong."

David continues, "On June 9 at 2208z, I worked CT3FT, Madeira
Islands, for my first Africa QSO on 6 meters. What a thrill that
was. I even managed to catch a very brief European E-skip opening at
1700z on June 3 and worked IK5MEJ and IW5DHN in Italy, a new country
for me."

On 6 meters Dave runs 100 watts to a 4-element Yagi at 60 feet.
Many other reports for that band came in from the VHF contest last
weekend. Don't forget ARRL Field Day coming up a little over a week
from now.

Nick Elias, N3AIU in Flagstaff, Arizona says that on June 9 on 6
meters he worked P4/W1XP on CW by loading up his full wave 80 meter
horizontal loop.

This weekend is the All Asia DX CW Contest. From the U.S. West
Coast, 20 meters may open all night to the Far East. 40 meters looks
good from 0900-1400z. From Texas, the 20 meter opening should be
much shorter, from about 0630-1400z, and a 40 meter opening may also
be short, around 0930-1200z. From the center of the 48 contiguous
United States, check 20 meters toward the Far East around
0800-1330z, and 40 meters from 0930-1200z.

>From Chicago, 20 meters toward Japan looks best 0800-1230z, and
little chance of a 40 meter shot at all, perhaps around 1030-1100z.
>From Cleveland no band looks good toward Japan, but 20 meters has
possibilities 0700-1400z.  New York also does not look promising,
but may see some 20 meter Far East propagation around 0700-1300z.
Atlanta shows a possible 40 meter opening around 1030z, and 20
meters 0700-1330z.

If you would like to make a comment or have a tip for our readers,
email the author at, [EMAIL PROTECTED]

For more information concerning radio propagation, see the ARRL
Technical Information Service at,
http://www.arrl.org/tis/info/propagation.html. For a detailed
explanation of the numbers used in this bulletin, see,
http://www.arrl.org/tis/info/k9la-prop.html. An archive of past
propagation bulletins is at, http://www.arrl.org/w1aw/prop/ .

Sunspot numbers for June 8 through 14 were 67, 42, 46, 46, 32, 23
and 35 with a mean of 41.6. 10.7 cm flux was 80, 77.6, 76.1, 74.4,
74.2, 77.1, and 75.3, with a mean of 76.4. Estimated planetary A
indices were 20, 10, 8, 5, 4, 3 and 7 with a mean of 8.1. Estimated
mid-latitude A indices were 18, 9, 7, 4, 2, 2 and 6, with a mean of
6.9.

/EX

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[DX-NEWS] ARLP024 Propagation de K7RA

2005-06-10 Thread W1AW
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 10, 2005
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

Sunspot and solar flux readings were up this week while geomagnetic
K and A indexes were down a bit, which is generally what HF
operators want. There were no big events triggering geomagnetic
storms this week, as indicated by the low A index numbers at the end
of this bulletin. A solar wind stream last weekend only drove
geomagnetic indices up to moderately active levels. But two big new
sunspots, 775 and 776, are rotating to the most effective position
for affecting earth. Solar flux for this weekend, June 10-12, is
expected to be around 110-115. Geomagnetic conditions should be
quiet, although the new sunspots are magnetically complex, and could
hold a surprise.

We're moving now toward summer propagation from the recent spring
conditions we've been experiencing. Summer solstice in the Northern
Hemisphere is set for June 21 at 0646z. Today we are 80 days past
the equinox, and the bands are behaving differently than they were a
few months ago. For instance, paths from the continental U.S. to
South America are open much later on 17 and 20 meters. You can run
two instances of W6ELprop, located on the web at,
http://www.qsl.net/w6elprop/, and run some tests.

For instance, perform a test from the center of the Continental U.S.
(by entering W for the prefix) to Brazil for any date this week, and
enter an average of several days of sunspot numbers (from the end of
this bulletin). You can do the same for a date in late March, and
get the numbers from past bulletins at,
http://www.arrl.org/w1aw/prop/. Even though average sunspot numbers
were lower in late March than they've been this week, propagation
possibilities to Brazil during mid-day on 10, 12 and 15 meters in
March were much better than they are now. But signals over the same
path show better current openings much later into the evening on
those same bands than they were in late March. Plot from the central
U.S. to Hawaii as the target, and 20 meter signals drop out in the
evening in March, but are currently strong all night long.

The ARRL Contest Calendar, located at,
http://www.arrl.org/contests/calendar.html, shows this weekend, June
11-13, is the ARRL June VHF QSO Party. The object is to get as many
contacts in as many grid squares as possible. Many HF radios these
days come with 6-meter capability, so it isn't much of a stretch for
HF operators without a 6-meter antenna to just toss up a dipole at
the last minute. A half-wave dipole is only about 9 feet and 3
inches long on 6-meters, and when the band opens up, a simple
antenna can do quite well. If you don't know your grid-square,
calculate it at http://www.arrl.org/locate/grid.html. If you hear
stations reporting unfamiliar grid squares, at least for the United
States there is a good map at
http://www.icomamerica.com/downloads/usgridsq.pdf. You can find the
rules for the contest on the calendar mentioned above.

There have been many nice 6-meter openings recently, mostly via the
sporadic-E layer skip that is common this time of year, and Frank
Fascione, KB1LKB of Manchester, Connecticut sent in a report for
last Sunday, June 5. He reports an all day opening to the Caribbean
on 6-meters, as well as Georgia, Florida and Alabama. Among stations
heard but not worked were FG5FR, FM5JC, FM5AD, 9Y4AT, YU4DDK, and
PZ5RA. Frank contacted several new ones for him, including FJ5DX,
YV4DYJ, PJ2BVU, HK4SAN and J69EN.

Doug, CO8DM uses 100 watts to a 2 element quad at 65 feet on 6
meters. He reports that around the first of the month he copied
European stations, including Italy and Sicily, and on CW, Malta.
The next morning he heard M0BJL in the UK.

Regarding the urging above to get on 6-meters, Eric Hall, K9GY wrote,
"... please mention for people to get on with their radios that can
work VHF and be active in the ARRL VHF contest. It doesn't take a
lot of stuff to make QSOs!" Eric made his first 6-meter QSO on June
5 with an FT-817 and a 6-meter Hamstick whip antenna. He was in FM18
and he worked N4OX in EM60 on 50.130 MHz SSB. Then he worked KA4DPF
in EM81 about 20 minutes later. People like me who are unfamiliar
with grid squares can look on the map mentioned above to see where
FM18, EM60 and EM81 are.

Bill VanAlstyne, W5WVO in DM65 seemed almost giddy about the opening
on Tuesday, May 31. He says it was "one of the most incredible 6M Es
openings I've ever been part of since moving to New Mexico a few
years ago. 6M was open from before 7 AM local time until nearly
midnight, with only a couple hours of rest around mid-day. I think
we're all still catching our collective breath from this one!"

Bill runs 100 watts to an 18 foot 5 element Yagi up 25 feet. He made
over 75 contacts and worked 13 new grids to boost his total above
300. He says he "ran pile-ups of calling statio

[DX-NEWS] ARLP024 Propagation de K7RA

2004-06-11 Thread W1AW
SB PROP @ ARL $ARLP024
ARLP024 Propagation de K7RA

ZCZC AP24
QST de W1AW  
Propagation Forecast Bulletin 24  ARLP024
>From Tad Cook, K7RA
Seattle, WA  June 11, 2004
To all radio amateurs 

SB PROP ARL ARLP024
ARLP024 Propagation de K7RA

Solar activity remains low. As the sunspot cycle declines, we are
inevitably headed toward a year or two of quiet sun. The sunspot
minimum is several years off, however.

This week average daily sunspot numbers were up slightly by over 7
points to 68.3. Average daily solar flux was down nearly 10 points
to 87.4. Geomagnetic conditions remained quiet to slightly
unsettled.

The chance of any geomagnetic upset this weekend seems very remote.
The sun is nearly blank, but today two sunspots peeked around to the
visible face. Solar flux is expected to remain low, declining to
around 80 next week. Solar flux is expected to rise above 100 once
again between June 19-22.

Regional Warning Center Prague (http://rwcprague.ufa.cas.cz/)
predicts quiet geomagnetic conditions on June 13, 14 and 17, quiet
to unsettled conditions on June 12, and unsettled conditions on June
11, 15 and 16. On June 9, the sun spewed a coronal mass ejection,
but the energy was aimed away from earth. It caused no geomagnetic
upset.

Remember that in all this, what most HF operators will want is more
sunspots and higher solar flux, but low geomagnetic A and K indices.
Note that geomagnetic conditions are much quieter than they were for
many months, when it seemed that solar flares and geomagnetic storms
would never stop.

Reader David Moore passed along an interesting article on sources of
solar hazards in interplanetary space. Read it on the web at,
http://www.spaceref.com/news/viewpr.html?pid=14324.

For more information concerning propagation and an explanation of
the numbers used in this bulletin see the ARRL Technical Information
Service propagation page at,
http://www.arrl.org/tis/info/propagation.html.

Sunspot numbers for June 3 through 9 were 77, 55, 59, 60, 82, 72 and
73 with a mean of 68.3. 10.7 cm flux was 90, 89.4, 84.5, 88.4, 88.5,
86 and 85.2, with a mean of 87.4. Estimated planetary A indices were
8, 11, 11, 11, 8, 9 and 14, with a mean of 10.3.  Estimated
mid-latitude A indices were 6, 14, 8, 12, 7, 6 and 13, with a mean
of 9.4.

/EX


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