06060 r universo? ou r tupi 10k / curitiba brésil sud 0528 322 port yl
musique Jan18 05
michel lacroix
france
=
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Some corrections to messages posted by Tomas, NW7US (AAR0JA/AAA0WA)
This was a long duration X3.8 event originating in region 10720.
GOES-12, not GOES-10, is commonly used as the source for intensity
readings.
Two CMEs have been observed at ACE today, the first one arrived at 07:17
UTC. Its
Some corrections to messages posted by Tomas, NW7US (AAR0JA/AAA0WA)
The flare in question was a long duration X3.8 event originating in region
10720. GOES-12, not GOES-10, is commonly used as the source for intensity
readings.
Two CMEs have been observed at ACE today, the first one arrived at 07
Loggings from (CE) Craig Edwards, Townsville, Queensland, Australia
Icom R75 running off 12V, pre-amp, EWE to Asia.
Heard at home from January 10-16th 2005 (times UTC)
549 0845 CNR Fujian, China. Powerhouse from CC heard every evening and
morning, if you can't hear this at the sta
English Service Bangladesh Betar :
Eid-ul-Azha : A day of total submission to the will of Allah- A special
composite program on the occasion of holy Eid-ul-Azha.
Broadcasting Date : January 21 or 22, 2005 (depands on Moon may be 22.01.2005)
Frequencies : 7185 kHz, 9550 kHz
UTC : 1815-1900
Hard-Core-DX.com logs from 2005-01-17 UTC to 2005-01-18 UTC
-
Please visit http://log.hard-core-dx.com/ for the real time logs
and to submit your logs to the HCDX Online Log.
Oceania
11895 Jan 16 1100-1102 Guam:
bonsoir
04976 ouganda ds 10k 2048 333 vernac musique & dj Jan17 05
05015 turkmen r ds 100k / ashgabat 2055 333 turkm -fading - musique Jan17 05
michel lacroix
france 60
=
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World Radio TV Handbook 2005 is coming out. Preorder yours and support op
NW7US Propagation Update
17 January 2005 - 2030 UTC
The latest long-duration flare from active solar region 720 (the flare
measured X3.8 and X4.1, officially recorded as X3.8 at 0659 UTC
17-I-2005), which took 2 hours to reach maximum, and had a long decay as
well, unleashed such an intense
I have been trying to find RG-174U cable to rebuild the AL4 Drake Loop.
All I can find is RG-176/U. The difference I can find is the RG-174U
runs 50 ohms and the RG-176/U runs 75 ohms. Apparently the input of the
SPR4 runs 50 ohms where the loop plugs in. Do you think using 75 ohm
cable would make
Quito 17/1 2005
*** Monday edition:
*** Recording of 5975.00 kHz Radio Guiara,
Villarica (Levi P. Iversen)
This is the first guest-recording I have received
from Levi P. Iversen, Paraguay, I hope it is not
the last, thank you very much Levi!
Comments and recordings at:
http://www.malm-ecuador.co
Energetic Ion Enhancement Event ( see
http://www.agu.org/pubs/crossref/2004/2003JA010044.shtml )
At 0640 UTC 17-I-2005, ACE detected a proton flux exceeding 1.0e+05 p/cm2
- which simply indicates the probable arrival of the plasma cloud expected
from the flare events reported earlier. It i
On 17 Jan at 1430 noted coastal station Monaco Radio 3AC
on 8728U with canned IDs in French, English and Russian
promoting their maritime fax, e-mail etc services, playing an
interval signal between the announcements. Most interesting
about the interval signal was that it is an orchestral version o
Energetic Ion Enhancement Event ( see
http://www.agu.org/pubs/crossref/2004/2003JA010044.shtml )
At 0640 UTC 17-I-2005, ACE detected a proton flux exceeding 1.0e+05 p/cm2
- which simply indicates the probable arrival of the plasma cloud expected
from the flare events reported earlier. It i
FYI, 73 wb
TAIWAN According to Mr.Sapun Pak of Korean Shortwave Club, Korean staff of
Radio Taiwan International was noticed the sudden closure of Korean sce on
January 13. RTI will cease 3 foreign langs sces including Korean, and 2
Chinese dialects sces on January 31.
Mr.Pak and RTI Korean sta
NW7US Propagation Update
17 January 2005 - 1145 UTC
The solar wind speed is now (1145 UTC) exceeding 776 km/s with a
moderately southward orientation of the interplanetary magnetic field (Bz
= -6.6 nT). This rise in wind speed is rather sudden, after a long period
of it hovering around 600
Flare update - 0952 UTC
The entire HF spectrum is shut-down at the time of this e-mail, on the
sunlit side of the Earth. Recovery time is 1 hour, 37 minutes (approx.
1130 UTC). The flare from region 720 has maxed out at X4.1 (GEOS) (IPS
reports X3.8). The rise time was nearly two hours in
NW7US Propagation Bulletin Update
0930 UTC, 17 January 2005
It is clear now after analysis that the coronal mass ejection (CME)
associated with the X2.6-class X-ray flare of 2302 UTC 15 January 2005 has
arrived. The first detection was at 0640 UTC as an energetic ion
enhancement. The secon
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