[RSM] W3LPL: Mostly normal thru Tues/3

Art Boyars artboyars at gmail.com
Mon Jan 2 20:25:41 EST 2023


From: Frank W3LPL <donovanf at starpower.net>
To: PVRC <pvrc at mailman.qth.net>
Cc:
Bcc:
Date: Mon, 2 Jan 2023 01:57:26 -0500 (EST)
Subject: [PVRC] Propagation is likely to be mostly normal through Tuesday

My propagation forecast derived from today's NOAA/SWPC web pages
is published five days a week (M-F) in the Daily DX. All days and times in
this forecast are in UTC (Zulu) time.

Propagation crossing low and mid-latitudes is likely to be normal through
Tuesday.

Propagation crossing the auroral ovals and polar regions is likely to be
mostly normal through Tuesday.

Click *here* <https://services.swpc.noaa.gov/images/station-k-index.png>
for today’s
latest planetary Kp Index, updated every three hours.

Click *here* <http://www.hamqsl.com/solar.html> for N0NBH’s current HF Band
Conditions, updated regularly.
Today's solar flux index (SFI) is 153 and is likely to remain about the
same through Tuesday. The sun’s visible disk has two large, two medium and
two tiny active regions containing 34 sunspots with a total sunspot area of
1220 micro-hemispheres (about seven times the surface area of the Earth).
https://www.sidc.be/spaceweatherservices/applications/solarmap

160 and 80 meter propagation from North America to VK/ZL and
the south Pacific is likely to be normal through Tuesday.

40 meter short path propagation from North America to south Asia at about
0000Z is likely to be mostly normal through Tuesday. Short path propagation
from North America to east Asia after about 0800Z is likely to be mostly
normal through Tuesday. 40 meter long path propagation from North America
to east Asia after about 2130Z is likely to be normal through Tuesday.

30 meter propagation through the auroral ovals and polar regions is likely
to be mostly normal through Tuesday. 30 meter long path propagation from
North America to east Asia after about 2130Z is likely to be normal through
Tuesday. 30 meter propagation is always significantly degraded within a few
hours of local noon by E-region blanketing of long distance F2 propagation.

20 meter daytime and evening propagation through the auroral ovals
and polar regions is likely to be mostly normal through Tuesday. 20
meter transpolar propagation within a few hours of sunrise and sunset is
likely to be mostly normal through Tuesday.

17 and 15 meter long distance propagation is likely to be mostly normal
through Tuesday.

12 and 10 meter long distance propagation is likely to be mostly normal
through Tuesday. 12 and 10 meter long path propagation from North America
to east Asia from about 1200Z to 1400Z is likely to be mostly normal
through Tuesday. 12 and 10 meter F2 propagation crossing northern
hemisphere mid-latitudes is likely to be enhanced when the solar flux index
is about 120 or higher and geomagnetic activity is quiet to unsettled (K
index of 3 or less).

Very long distance 6 meter oblique trans-equatorial propagation (TEP) from
North America mostly to CQ Zone 32 is likely to occur infrequently through
early January from the southern tier of U.S. states during mid-afternoon at
the path mid-point (evening hours in the eastern U.S.) More northerly U.S.
locations may infrequently couple into trans-pacific oblique TEP via
occasional sporadic-E paths to W5 and XE. See K6MIO’s excellent article
beginning on page 66 at:
https://k5tra.net/TechFiles/2014%20Central%20States%20whole%20book.pdf

Persistent southward orientation (-Bz) of the north-south component of the
interplanetary magnetic field (IMF) plays a crucial but unpredictable role
in triggering all geomagnetic storms. Brief minor to moderate
geomagnetic storms may be gradually triggered when the IMF persists in a
southward orientation (-Bz) with IMF field strength of about 5 nanoteslas
for several hours coincident with the effects of an Earth directed
coronal hole high speed stream. More frequent, longer duration, minor
to severe geomagnetic storms may be triggered suddenly and
unpredictably when the IMF persists in a southward orientation (-Bz) with
IMF field strength significantly stronger than 5 nanoteslas for several
hours or more coincident with the effects of an Earth directed fast CME
(faster than 1000 km per second). Real time geomagnetic data including Bz
orientation, IMF field strength, solar wind speed and short term K Index
forecast are available here:
www.swpc.noaa.gov/products/geospace-geomagnetic-activity-plot

There is a chance of minor to moderate daytime radio blackouts caused by
unpredictable sudden bursts of X-ray radiation from M-class solar flares
through Tuesday due to the large number of active regions on the visible
disk.

Solar wind speed is likely to be slightly elevated on Monday and near
background levels on Tuesday due to waning coronal hole high speed stream
effects.

Geomagnetic activity is likely to be mostly quiet through Tuesday due to
waning coronal hole high speed stream effects. We are in the winter
solstice season when disturbed geomagnetic conditions occur about half as
often as during the spring and fall equinox seasons.

Mid-latitude northern hemisphere sunset is eight minutes later and day
length is four minutes longer than it was on December 21st.

Click *here* <https://www.spaceweather.gc.ca/solarflux/sx-4-en.php> for today’s
Penticton 10.7 cm solar flux index updated at 1800Z, 2000Z and 2200Z daily.

Click *here*
<https://spaceweather.gfz-potsdam.de/fileadmin/ruggero/Kp_forecast/forecast_figures/KP_FORECAST_CURRENT.png>
for today’s
three-day GFZ Planetary K Index forecast updated every three hours.

Click *here* <http://sidc.oma.be/products/meu/> for today's SIDC Daily
Bulletin on Solar and Geomagnetic Activity updated at 1230Z daily.

Click *here* <https://www.swpc.noaa.gov/products/forecast-discussion>
for today's
SWPC Solar Activity Forecast Discussion updated at 0030Z and 1230Z daily.

Click *here* <https://www.sws.bom.gov.au/Space_Weather/1/1> for today's
Australian Space Forecast Centre Summary and Forecast updated at 2330Z
daily.
Perhaps the most useful HF propagation pages for DXers can be found at:
http://dx.qsl.net/propagation and http://www.solarham.net


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