[RSM] W3LPL: Mostly normal propagation is likely through Tuesday July 20th
Art Boyars
artboyars at gmail.com
Mon Jul 19 01:36:05 EDT 2021
From: donovanf at erols.com
To: Reflector PVRC <pvrc at mailman.qth.net>
Cc:
Bcc:
Date: Mon, 19 Jul 2021 00:43:30 -0400 (EDT)
Subject: [PVRC] Mostly normal propagation is likely through Tuesday July
20th
My propagation forecast derived from today's NOAA/SWPC
web pages is published five days a week (M-F) in the Daily DX.
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/planetary-k-index.gif>
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.
We are in the quiet geomagnetic activity season, only about half
as many geomagnetically disturbed days occur in June and July
compared to the more geomagnetically active equinox seasons.
Sporadic-E propagation occurs every day during June and July
at mid-latitudes in the northern hemisphere making long distance
propagation up to 15,000 km sporadically available in the
17, 15, 12, 10 and 6 meter bands from sunrise through midnight
and occasionally somewhat later.
The solar flux index (SFI) is likely to be at least 80 through Tuesday.
There are three small active regions on the solar visible disk with
twelve tiny sunspots.
https://sdo.gsfc.nasa.gov/assets/img/latest/latest_1024_0171.jpg
160 and 80 meter propagation from North America to VK/ZL and
the south Pacific is likely to be seasonably normal through Tuesday.
40 meter short path propagation to south Asia at about 0015Z is
likely to be mostly normal through Tuesday. 40 meter short path
propagation from North America to east Asia after about 0930Z
is likely to be mostly normal through Tuesday.
30 meter propagation through the auroral ovals and polar regions
is likely to mostly normal through Tuesday. 30 meter propagation
is always significantly degraded within a few hours of local noon
because of E-region blanketing of long distance F2 propagation.
30 meter night time long distance propagation in the norther
hemisphere is likely to improve due to increased ionizing solar
radiation in the northern high latitude regions caused by increased
sunspot activity, higher solar elevation angles and short nights
with no source of ionizing solar radiation.
20 meter daytime and evening propagation through the auroral
ovals and polar regions is likely to be mostly normal through
Tuesday. 20 meter northern transpolar propagation within a
few hours of sunrise and sunset is improving with longer duration
solar ionizing radiation on the northern polar region caused by
high solar elevation angles 24 hours per day during the midnight
sun season. 20 meter long distance propagation is significantly
degraded from mid-morning through late afternoon at low and
mid-latitudes in the northern hemisphere by F1 region midday
blanketing of low angle long distance propagation during the
summer. 20 meter late afternoon, nighttime and early morning
long distance propagation in the northern hemisphere is likely
to improve due to increased ionizing solar radiation in the northern
high latitude regions caused by increased sunspot activity,
higher solar elevation angles and short nights with no source
of ionizing solar radiation.
17 and 15 meter daytime long distance propagation in the northern
hemisphere is likely to improve due to increased ionizing solar
radiation in the northern high latitude regions caused by increased
sunspot activity, high solar elevation angles and long days.
17, 15, 12, 10 and 6 meter sporadic-E propagation up to 15,000 km
is likely to be sporadically available from sunrise through midnight
and occasionally later through late July.
Geomagnetic disturbances *caused by coronal hole high speed stream*
effects are likely to remain mostly brief, minor and somewhat less
frequent through at least late 2021. The southward oriented (-Bz)
component of the 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 enhanced IMF
field strength 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 enhanced IMF field strength
or several hours or more *coincident with* the effects of an Earth
directed fast CME.
The solar wind is expected to be near background state through
Tuesday. The geomagnetic field is likely to be mostly quiet through
Tuesday. Coronal hole high speed stream and CME effects,
geomagnetic storms and solar flares are not likely through Tuesday.
Mid-latitude northern hemisphere sunset is now 6 minutes earlier
and daylength is 22 minutes shorter than it was on the June 21st.
Daylength and solar elevation angle in the northern polar region
are slowly declining due to gradually waning summer solstice effects.
Click *here* <https://www.spaceweather.gc.ca/solarflux/sx-4-en.php> for today’s
Penticton 10.7 cm solar flux index updated at 1700Z, 2000Z and 2300Z 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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