CLE 200 Results

The CLE 200 event this past weekend once again delivered mediocre propagation on all three evenings. In spite of Sunday night's G1-class geomagnetic storm and high K values, Sunday's overnight period proved to be the best of the weekend's generally 'below average' conditions ... this is the time of the year that LF propagation is usually at its best. Thankfully, there are still several months ahead that could offer some really great mid-winter prop.

The following NDBs were logged using the Perseus SDR along with my LF inverted L, resonated at 300kHz:

28 09:00 335 CC Concord, CA, USA
28 09:00 335 CVP Helena, MT, USA
28 08:00 335 YUT Repulse Bay, NU, CAN
28 06:00 335 YLD Chapleau, ON, CAN
28 09:00 336 LF La Salle, MB, CAN
28 13:00 337 FF Fergus Falls, MN, USA
28 09:00 337 7D Hudson Bay, SK, CAN
28 12:00 338 CMQ Campbell Lake, ALS
28 09:00 338 ZU Whitecourt, AB, CAN
28 12:00 338 RYN Tucson, AZ, USA
30 08:00 338 SHL Sheldon, IA, USA
28 07:00 338 TU Tulsa, OK, USA
28 12:00 338 YPX Puvirnituq, QC, CAN
28 12:00 338 K Port Angeles, WA, USA
28 10:00 339 6X York Landing, MB, CAN
28 10:00 339 MKR Glasgow, MT, USA
29 06:00 340 YY Mont Joli, QC, CAN
28 13:00 341 ELF Cold Bay, ALS
28 10:00 341 OIN Oberlin, KS, USA
29 06:00 341 YYU Kapuskasing, ON, CAN
28 09:00 341 DB Burwash, YT, CAN
28 09:00 342 PFT Pinecreek, MN, USA
28 09:00 343 YZH Slave Lake, AB, CAN
28 09:00 344 YOP Rainbow Lake, AB, CAN
28 09:00 344 XX Abbotsford, BC, CAN
28 09:00 344 FCH Fresno, CA, USA
28 09:00 344 BKU Baker, MT, USA
28 09:00 344 POY Powell, WY, USA
30 08:00 345 GF Grand Forks, ND, USA
30 08:00 346 OLT Soldotna, ALS
28 09:00 346 YXL Sioux Lookout, ON, CAN
28 15:00 347 TNC Tin City, ALS
28 13:30 347 DJN Delta Junction, ALS
28 06:00 347 LEN Leeny, ID, USA
28 15:00 347 SBX Shelby, MT, USA
30 08:00 347 YK Yankton, SD, USA
28 09:00 347 PA Prince Albert, SK, CAN
30 08:00 348 MC Mason City, IA, USA
28 07:00 348 MNC Shelton, WA, USA

More Low Noise Vertical (LNV) Construction

New LNV At WG2XKA

The low-noise vertical discussed here previously, has recently been implemented by at least three of the 630m experimental stations. John, WG2XKA / WA3ETD, along with Ken, WG2XXM / K5DNL and John, WG2XIQ / KB5NJD, have all constructed versions of this receiving antenna after reading about the details here.






John's antenna, pictured above, is described in more detail here, along with some nice pictures of his matching transformer.

All stations report good results with the antenna so it may be something you might want to consider if your present receiving antenna is a noise-collector.

For those interested in getting started on 630m, John (WG2XIQ), has a ton of inspiring information available on his website here as does John (WG2XKA) on his site here.

Aurora On The Move

A recent posting to the Pacific Northwest VHF Society's reflector brought my attention to an interesting article describing the southward migration of the auroral zone.




According to the research paper published in the Proceedings of the National Academy of Sciences, the earth's magnetic field is gradually growing weaker, thus affecting its interaction with the solar wind.

The paper indicates that our present, abnormally high magnetic field, forces this interaction (auroras) to higher latitudes and as the field strength gradually weakens to more long-term average levels, auroras will be seen further south than we have been used to. The field has already weakened by about 10% over the past two hundred years and will continue to do so. Apparently it's all related to the regular 'flipping' of our magnetic field, with the most 'recent' flip taking place about 780,000 years ago.

So what does this mean for radio amateurs? Probably not a lot, in the immediate future but the unwanted effects to disturbances in the geomagnetic field will eventually be felt further and further to the south. Radio propagation in southern British Columbia has always been particularly sensitive to even very small disturbances in the field, particularly on the LF and MF bands. I am constantly amazed at how regions only 150 miles to the south or southeast of me are so much less affected than here, in the southern fringes of the auroral zone. VE7's don't claim to be in radio's 'black hole' without good reason.

630m WSPR

courtesy: http://wsprnet.org/

                     
                    Happy Thanksgiving to those of you in the U.S.A.

It seems that the 630m WSPR digital crowd is growing quickly, with more new stations showing up every evening on the web's WSPRnet activity page. Most nights see activity from 80 or more stations, either transmitting or listening in WSPR mode on 630m!

WSPR is the 'Weak Signal Propagation Reporter' beacon-only mode being used by many of the stations presently transmitting on 630m, especially the U.S. experimental stations.

Those with the WSPR software (freeware and easily installed) usually have the program automatically upload their spots (stations being heard) to the WSPRnet page so that the transmitting stations are able to see where their signals are being heard. It also becomes quickly apparent, when examining the various spots, just how good or bad propagation might be at any given time.

WSPR Waterfall Displaying Detected Signals

Since WSPR is a non-QSO mode, the ability to observe propagation conditions, is its major feature. With transmission periods of just under two-minutes, and a very narrow FSK data information stream, WSPR can dig into the noise and copy signals that are often inaudible by ear ... some 15dB or more, past the audible level. Of course, audible signals are also demodulated as well, and will appear on your list of spotted stations, on the WSPRnet data page.

If you choose, you can also see your spotted stations in a Map mode, as shown at the top. This map shows the stations that I was hearing last night on 630m.

Along with the call and grid locator of the station being heard, the WSPR software also indicates several other bits of information, including the signal-to-noise ratio as heard at your location. Shown below is the decoded output from several stations following the two-minute transmission period.

06:58	WH2XXP	0.475662	-13	0	DM33	5	VE7SL	CN88iu	1909
06:58	WG2XXM	0.475709	-6	0	EM15lj	5	VE7SL	CN88iu	2610
06:58	WG2XKA	0.475723	-9	0	FN33lq	1	VE7SL	CN88iu	3833

Note the SNR reports ... usually, signals stronger than around -14dB will be just detectable by ear with anything in the + range being pretty strong.

Shown below are the Tuesday night reports of local station, VE7CNF, and indicates the extensive area over which his WSPR beacon was reported. Toby is running a modest 5W eirp station from a suburban-sized lot. Analyzing the reports, it is apparent that many of these stations rose to audible signal levels at various times throughout the evening and would have probably been workable on normal CW mode ... even from the 'burbs!

courtesy: http://wsprnet.org/

There are probably many of you already listening to WSPR signals on HF and have yet to venture down to 630m to see what can be heard. The improved propagation conditions of late make this an ideal time to have a peek at 630m and see what you can spot.

Your low-band wire antennas can often hear surprisingly well below the broadcast band and you may be surprised at what WSPR can detect. Use the USB mode with your receiver set to 474.200 kHz and, if possible, upload your 630m MF spots to the WSPRnet. You can also follow up-to-the-minute activity on the 2200m/630m ON4KST Chat page which is always interesting.

Hunting For NDBs IN CLE 200

XX - 344 Abbotsford, BC

How time flies ... it's CLE time once again! For you low-frequency buffs, another challenge awaits.

This month's frequency range covers 335.0 - 349.9 kHz.
Conditions have been very good this week ... hopefully this will continue.

A good CLE target this time is 'XX' on 344 kHz near Abbotsford, B.C. It has been heard throughout North America and can be a good prop-indicator for eastern listeners.

From CLE coordinator Brian Keyte (G3SIA), comes the following reminder:

Hi all:

Our 200th Co-ordinated Listening Event is only a few days away.
Just a normal CLE using a busy range of frequencies which usually
attracts a lot of interest.

First-timers' CLE logs will also be very welcome, as always.

Days: Friday 27 November - Monday 30 November
Times: Start and end at midday, your LOCAL time
Range: 335.0 - 349.9 kHz

Please join us wherever you are - just log the NDBs you can identify
having their nominal frequencies in the range (it includes 335 kHz
but not 350 kHz) and any UNIDs that you come across there too.
(A good way for some of us to unwind after Thanksgiving?)

We last concentrated on these frequencies in CLE185 in Aug. 2014.

Please send your CLE log to the List (no attachments and ideally in a
plain text email) with CLE200 at the start of its title. Show on each line:

# The Date (or Day No: 27 to 30)
# The Time in UTC
# kHz - the nominal published frequency, if known.
# The Call Ident.

Please show those main items FIRST. Any other optional details such
as Location and Distance go LATER in the same line.
If you send any interim logs, please also send a 'Final' (complete) one.
And, of course, tell us your own location and brief details of the
equipment that you were using during the Event.

You can find full details about current and past CLEs from the CLE page
http://www.ndblist.info/cle.htm including access to the CLE200 seeklists
for your part of the World prepared from the loggings on Rxx.

Good listening - enjoy the CLE.
Brian
----------------------------------------------------------
From: Brian Keyte G3SIA: <ndbcle'at'gmail.com>

Location: Surrey, SE England (CLE co-ordinator)
----------------------------------------------------------

(If you would like to listen remotely you could use any one remote
receiver such as http://websdr.ewi.utwente.nl:8901/ for your
loggings, stating its location and owner and with their permission
if required. A remote listener may NOT also use another receiver,
local or remote, to make further loggings for the same CLE)"

__._,_.___

These listening events serve several purposes. They:

• determine, worldwide, which beacons are actually in service and on-the-air so the online database can be kept up-to-date

• determine, worldwide, which beacons are out-of-service or have gone silent since the last CLE covering this range

• will indicate the state of propagation conditions at the various participant locations

• will give you an indication of how well your LF/MF receiving system is working

• give participants a fun yet challenging activity to keep their listening skills honed

Final details can be found at the NDB List website, and worldwide results, for every participant, will be posted there a few days after the event. If you are a member of the ndblist Group, results will also be e-mailed and posted there.

The very active Yahoo ndblist Group is a great place to learn more about the 'Art of NDB DXing' or to meet other listeners in your region. There is a lot of good information available there and new members are always very welcome.

If you are contemplating getting started on 630m, listening for NDBs  is an excellent way to test out your receive capabilities as there are several NDBs located near this part of the spectrum.

You need not be an ndblist member to participate in the CLEs and all reports, no matter how small, are of much value to the organizers. 'First-time' logs are always VERY welcome!

Reports may be sent to the ndblist or e-mailed to either myself or CLE co- ordinator, Brian Keyte (G3SIA), whose address appears above.

Please ... do give the CLE a try ... then let us know what NDB's can be heard from your location! Your report can then be added to the worldwide database to help keep it up-to-date.

__._,_.___