[RSM] W3LPL forecast Thu-Fri Apr 22-23
Art Boyars
artboyars at gmail.com
Thu Apr 22 09:18:12 EDT 2021
From: donovanf at erols.com
To: PVRC <pvrc at mailman.qth.net>
Cc:
Bcc:
Date: Thu, 22 Apr 2021 02:21:24 -0400 (EDT)
Subject: [PVRC] Mostly normal propagation through Friday
Long distance propagation forecast for Thursday and Friday, April 22-23
My propagation forecast derived from today's NOAA/SWPC web
pages is published five days a week (M-F) in the Daily DX.
Propagation at low and mid-latitudes is likely to be normal through
Friday. Propagation crossing the auroral oval and polar regions is
likely to be mostly normal with below normal intervals through Friday.
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.
The solar flux index (SFI) is likely to be about 78 through Friday.
Three active regions containing a total of 17 mostly tiny sunspots
are having minimal effects on HF propagation.
We are exiting the most disturbed weeks of the March-April
geomagnetic storm season when the earth is passing through the
part of the interplanetary magnetic field (IMF) with the most
frequent, longest duration southward oriented IMF. Approximately
twice as many brief minor and moderate geomagnetic storms occur
during March and April compared to the quieter IMF during June
and July. Brief minor to moderate geomagnetic storms may be
triggered with little warning when the IMF rotates to a southward
orientation and persists for several hours *coincident with* the effects
of earth directed coronal hole high speed streams and coronal mass
ejection (CME) enhancements in the solar wind.
160 and 80 meter short path propagation from North America to
VK/ZL is likely to be normal through Friday. 80 and 40 meter
short path propagation to south Asia is likely to be mostly normal
at about 0030Z Friday. 80 and 40 meter short path propagation
from North America to east Asia after about 0900Z is likely to be
mostly normal with below normal intervals through Friday.
30 meter propagation through the auroral ovals and across polar
regions is likely to be mostly normal with below normal intervals
through Friday. 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
propagation is likely to improve slightly through Friday due to
solar flux index of 78.
20 meter daytime and evening propagation through the auroral ovals
and across polar regions is likely to be mostly normal with below
normal intervals through Friday. 20 meter northern trans-polar
propagation within a few hours of sunrise and sunset will steadily
improve with gradually increasing electron density in the polar F2
region through June. 20 meter night time long distance propagation
in the northern hemisphere is likely to improve slightly through Friday
due to solar flux index of 78.
17 and 15 meter daytime long distance propagation in the northern
hemisphere is likely to improve slightly through Friday due to solar
flux of 78. 12 and 10 meter daytime long distance propagation is
likely to be mostly unreliable and limited to propagation from North
America to Southern Africa, South Atlantic, South America and
South Pacific regions.
Geomagnetic disturbances *caused by coronal hole high speed streams*
are likely to remain mostly brief, minor and less frequent through
at least late 2021. The north-south (Bz) component of the IMF plays
a crucial role in triggering brief minor to moderate geomagnetic
storms when it persists in a southward orientation (-Bz) with enhanced
field strength for several hours *coincident with* the effects of earth
directed coronal hole high speed stream or CME enhancements in
the solar wind.
IMF field strength, solar wind speed near earth and geomagnetic
activity are likely to be at close to background levels through Friday
with a possible enhancement late Friday due to coronal hole high
speed stream effects. There is a slight possibility that an M-Class
solar flare may cause a brief sudden ionospheric disturbance and
short-wave fadeout on the sun facing side of the earth late Thursday.
Geomagnetic storms and earth directed CMEs strong enough to affect
HF propagation are not likely through Friday.
Mid latitude northern hemisphere sunset is now 32 minutes later and
daylength is 81 minutes longer than it was on the March 20th.
Daylength is increasing by two minutes per day which is steadily
lengthening the duration of common daylight between distant
locations in the northern hemisphere. Solar elevation in the northern
polar region is increasing about three degrees per week, steadily
improving 20 meter northern trans-polar propagation through June.
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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