SB PROP @ ARL $ARLP009
ARLP009 Propagation de K7RA
ZCZC AP09
QST de W1AW
Propagation Forecast Bulletin 9 ARLP009
From Tad Cook, K7RA
Seattle, WA March 2, 2018
To all radio amateurs
SB PROP ARL ARLP009
ARLP009 Propagation de K7RA
We've seen many days with no sunspots over the past year, especially
in more recent times. Periods with more than three days of blank Sun
include January 4-11, 2017, March 6-20, 2017, May 9-15, 2017, June
9-12, July 18-24, October 8-14, October 16-20, November 1-13,
November 19-24, December 1-5, December 13-19, December 28, 2017
through January 3, 2018, January 20-29, 2018, and February 18-25.
Sunspots have been visible every day, starting on February 26.
This reporting week (February 22-28) the average daily sunspot
number was 6, up slightly from 5.6 over the previous seven days.
Average daily solar flux declined from 70.1 to 68.3.
Average planetary A index, a geomagnetic indicator calculated from
values measured at multiple magnetometers around the world, rose
marginally from 10 to 10.4, and mid-latitude A index which is
measured by a single magnetometer on Wallops Island, Virginia
changed from 7.7 to 7.4. All of these values are moderate, or quiet.
The most active day was February 27, when planetary A index was 19
and the mid-latitude A index was 14.
Spaceweather.com reports that Earth is exiting a solar wind stream
which produced brief G-1 class geomagnetic storms (see February 27
in the previous paragraph). NOAA says (according to
Spaceweather.com) that the chance of additional storms is 25% on
March 1, declining to 15% on March 2. A new solar wind could appear
on March 3.
How does this prediction figure from other sources?
From the NOAA 45-day forecast on March 1, predicted planetary A
index is 7 on March 2, 5 on March 3-5, 8 on March 6, 5 on March
7-13, then 10, 8, 12, 15 and 18 on March 14-18, 5 on March 19-20,
then 12, 15, 10, 8, 24, and 12 on March 21-26, then 5 on March 27
through April 9, then 10, 8, 12, 15 and 18 on April 10-14 and 5 on
April 15.
So if any solar wind appears by March 3, the only correlation with
the NOAA 45-day forecast would be the brief rise in planetary A
index to 8 on March 6.
You can read daily updates of the NOAA forecast every afternoon (USA
time) at ftp://ftp.swpc.noaa.gov/pub/forecasts/45DF/ .
Predicted solar flux from the same 45-day forecast is 68 and 70 on
March 2-3, and 72 on March 4-8, then 73, 75, 76, 77, 75, 72, and 70
on March 9-15, 68 on March 16-26, then 70 and 75 on March 27-28,
then 78 on March 29 through April 8, then 75, 72 and 70 on April
9-11, and 68 on April 12-15.
Considering the source, here is an excellent article on solar
activity:
"Solar flares, intense bursts of radiation and light emitted from
the Sun, are usually followed by a coronal mass ejection, which is a
massive amount of solar material and the magnetic field energy being
blown into space. Both of these phenomena can be dangerous under the
right conditions. They can cause radiation poisoning, damage
electronics on Earth and in orbit, and they can be a serious threat
to the safety of astronauts. In an effort to better understand solar
flares and CMEs, NASA created the Solar Dynamics Observatory to
constantly watch the Sun. Launched back in 2010 the SDO is equipped
with a suite of instruments that observe ultraviolet light, Doppler
shifts, magnetic fields and more. In 2014, they were watching a
large sunspot group in hopes of seeing an eruption, but it never
happened and now three and a half years later, they think they know
why.
"Back on October 24, 2014, they were keeping an eye on a sunspot
group the size of Jupiter known as Active Region 12192. This complex
grouping of magnetic fields was pegged as a site that had a high
potential for solar activity and was the largest grouping of the
last two solar cycles. The region did produce an X-class flare but
never produced a CME, which usually follows a flare. Scientists
wanted to know why so they looked at the data and found that there
was a battle between two magnetic structures that ended up
containing the eruption. The structures are being referred to as a
twisted magnetic rope and a dense magnetic cage. The magnetic rope
built up energy in the sunspot region and became unstable. It was
able to lash through part of the magnetic cage and trigger a solar
flare but in the end, it was not strong enough to break through the
cage entirely and cause an eruption. This event has given scientists
a wonderful opportunity to learn more about the Sun and how these
events work. The data collected by SDO will be invaluable in
expanding our knowledge of the Sun."
See http://bit.ly/2FITwQo
Here is the geomagnetic activity forecast for March 2-27, 2018 from
F.K. Janda, OK1HH.
"Geomagnetic field will be:
Quiet on March 3, 6-7, 10, 12-13, 20
Mostly quiet on March 11
Quiet to unsettled on March 2, 5, 19, 23-24, 27
Quiet to active on March 4, 8-9, 14-16, 21-22, 25
Active to disturbed on March 17-19, 26
"Amplifications of the solar wind from coronal holes: cannot be
predicted for the period before March 10, but I do not expect any
significant upsurge. Then solar wind will intensify on March (10,)
16-18, (19-20, 25-26).
"Remark:
- Parenthesis means lower probability of activity enhancement.
- With regard to ongoing changes, current forecasts remains less
reliable especially in the first half of March."
"F. K. Janda, OK1HH"
Don't forget, the ARRL International SSB DX Contest is this weekend.
See http://www.arrl.org/arrl-dx .
Here is the March 1 report from Dr. Tamitha Skov:
https://www.youtube.com/watch?v=CNs7oEQZEEQ
If you would like to make a comment or have a tip for our readers,
email the author at, k7ra@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
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 February 22-28, 2018 were 0, 0, 0, 0, 16, 15,
and 11, with a mean of 6. 10.7 cm flux was 68.4, 67.6, 68.2, 67.2,
69.8, 67.9, and 68.8, with a mean of 68.3. Estimated planetary A
indices were 11, 16, 9, 4, 7, 19, and 7, with a mean of 10.4.
Estimated mid-latitude A indices were 9, 11, 6, 2, 6, 14, and 4,
with a mean of 7.4.
NNNN
/EX
