Author Archive
Hunting For NDBs In CLE277
February 23rd, 2022 | 
Author:  |
| ZYC-254 kHz Calgary, Alberta (http://www.ve3gop.com) |
Another month has zipped by which means it's time for another CLE weekend!
When tuning for NDBs, put your receiver in the CW mode and listen for the NDB's CW identifier, repeated every few seconds. Listen for U.S. NDB identifiers approximately 1 kHz higher or lower than the published transmitted frequency since these beacons are modulated with a 1020 Hz tone approximately.
For example, 'AA' near Fargo, ND, transmitted on 365 kHz and its upper sideband CW identifier was tuned at 366.025 kHz while its lower sideband CW ident could be tuned at 363.946 kHz. Its USB tone was actually 1025 Hz while its LSB tone was 1054 Hz.
Often, one sideband will be much stronger than the other so if you don't hear the first one, try listening on the other sideband.
Canadian NDBs normally have an USB tone only, usually very close to 400 Hz. They also have a long dash (keydown) following the CW identifier.
All NDBs heard in North America will be listed in the RNA database (updated daily) while those heard in Europe may be found in the REU database. Beacons heard outside of these regions will be found in the RWW database.
From CLE organizers comes the following CLE info:
Hello all,
This coming weekend we have another chance to enjoy a Coordinated Listening
Event.
All CLE logs will be very welcome, short or long.
Days: Friday 25 Feb. - Monday 28 Feb.
Times: Start and end at midday, local time at the receiver.
Listening for Normal NDBs in the ranges:
240.0 - 259.9 kHz plus 420.0 - 439.9 kHz
(BOTH ranges are for ALL listeners)
Please log the NDBs you can identify that are listed in the ranges, plus any
UNIDs that you come across there.
You can find details of the beacons in those ranges, lists and maps, if you
go to http://www.ndblist.info/cle.htm and click on 'CLE SEEKLIST'.
Send your final CLE log to ndblist'at'groups.io with CLE277 and FINAL in
the email Subject.
Please show on EVERY LINE of your log:
# The full Date (or Day no.) e.g. ‘2022-02-25’ (or just ‘25’)
and UTC (the day changes at 00:00 UTC)
# kHz (the beacon's nominal published frequency if you know it)
# The Call Ident.
Other optional details - Location, Distance, etc. - go LATER in the same
line (or in footnotes). Please make your log useful to old and new members
alike by ALWAYS including your own location (and 6-character Locator if you know it) and brief details of the equipment and aerial(s) that you were
using.
We will send an 'Any More Logs?' email at about 20:00 UTC on Tuesday evening so you can check that your log has been found OK.
To be included in the combined results your log must have arrived by 09:00
UTC on Wednesday 2nd March at the very latest.
We hope to complete making the Combined Results within a day or two.
Good listening
Brian and Joachim
---------------------------------------------------------------------
From: Brian Keyte G3SIA ndbcle'at'ndblist.info
Location: Surrey, SE England (CLE coordinator)
---------------------------------------------------------------------
If you are interested in some remote listening - maybe
due to local difficulties - you could use any one remote
receiver for your loggings, stating its location and with
the owner’s permission if required.
( e.g. see kiwisdr.com )
A remote listener may NOT also use another receiver,
local or remote, to make more loggings for the same CLE.
These listening events serve several purposes. They
• 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.
The NDB List Group is a great place to learn more about the 'Art of NDB DXing' or to meet other DXers in your region. There is a lot of good information available there and new members are always very welcome. As well, you can follow the results of other CLE participants from night to night as propagation is always an active topic of discussion.
You need not be an NDB List member to participate in the CLEs and all reports, no matter how small, are of much value to the organizers.
Remember - 'First-time' logs are always VERY welcome!
Reports may be sent to the NDB List Group or e-mailed to CLE co-ordinator, Brian Keyte (G3SIA), whose address appears above. If you are a member of the group, all final results will also be e-mailed and posted there.
Please ... 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.
Have fun and good hunting!
DX Central’s MW Frequency Challenge
If you like DXing the broadcast band, then the weekly ‘DX Central MW Frequency Challenge' may be of interest to you. It’s run and organized by Loyd Van Horn, W4LVH, a dedicated DXer and a big promoter of BCB DXing.
Basically, participants are asked to listen on the chosen frequency for a one week period and report what they have been able to identify. Results of course will be different throughout the continent but if you are near any other listeners, it’s always fun to compare your final results.
The new frequency (or frequencies) are announced Sunday evening around 0100Z on Loyd's regular live-feed Youtube channel as well as on his Twitter feed @dxcentral
Loggings are reported via a fill-in form which is updated weekly.
As well, information on most aspects of AM BCB DXing can be found on Loyd’s website.
Hopefully you can give it a shot during the week and see what you can catch.
This week’s frequency is 1450 kHz.
Hunting For NDBs In CLE 276
 |
| ZQT-263 Thunder Bay, ON (tnx ve3gop.com) |
It's CLE fun time once again. How quickly time zooms by.
When tuning for NDBs, put your receiver in the CW mode and listen for the NDB's CW identifier, repeated every few seconds. Listen for U.S. NDB identifiers approximately 1 kHz higher or lower than the published transmitted frequency since these beacons are modulated with a 1020 Hz tone approximately.
For example, 'AA' near Fargo, ND, transmitted on 365 kHz and its upper sideband CW identifier was tuned at 366.025 kHz while its lower sideband CW ident could be tuned at 363.946 kHz. Its USB tone was actually 1025 Hz while its LSB tone was 1054 Hz.
Often, one sideband will be much stronger than the other so if you don't hear the first one, try listening on the other sideband.
Canadian NDBs normally have an USB tone only, usually very close to 400 Hz. They also have a long dash (keydown) following the CW identifier.
All NDBs heard in North America will be listed in the RNA database (updated daily) while those heard in Europe may be found in the REU database. Beacons heard outside of these regions will be found in the RWW database.
From CLE organizers comes the following CLE info:
Hello all,
Here's your chance to join in this coming weekend's Coordinated Listening
Event which uses some unusual and challenging frequencies.
Any first-time CLE logs will also be very welcome, however modest.
Days: Friday 28 Jan. - Monday 31 Jan.
Times: Start and end at midday, local time at the receiver.
Target: Normal NDBs (not NAVTEX or amateur beacons)
QRG: 260.0 - 269.9 kHz
plus: 440.0 - 1740.0 kHz
Please log the NDBs you can identify that are listed in those ranges, plus
any UNIDs that you come across there.
North America has a modest number of active NDBs in both ranges.
For Europe listeners there are LOTS of targets in the HF range, but they are
mostly well to the east, many of them also competing with strong
Broadcasting Stations. Australia has a few NDBs in both ranges.
You can find all the details of the beacons in these ranges, lists and maps,
if you go to http://www.ndblist.info/cle.htm and click on the 'CLE
SEEKLIST' link.
If you are disappointed by having very few likely targets, maybe you could
listen instead via a remote receiver located nearer to the action? By doing
that many of us could have some very nice surprises, especially listening in
these extreme frequencies. See kiwisdr.com - and please also see the
important footnotes below.
Send your final CLE log to the List, preferably as a plain text email, not
in an attachment, with CLE276 and FINAL at the start of its title.
Please show on EVERY LINE of your log:
# The full Date (or Day no.) e.g. '2022-01-28' (or just '28')
and UTC (the day changes at 00:00 UTC)
# kHz (the beacon's nominal published frequency if you know it)
# The Call Ident.
Other optional details - Location, Distance, etc. - go LATER in the same
line (or in footnotes). If you can give any extra details about new UNIDs,
especially strong ones that may be near to you (maybe their approximate
direction, etc.) it will help us to discover more about them. Please make
your log useful to old and new members alike by ALWAYS including your own location and brief details of the equipment and aerial(s) that you were
using.
We will send an 'Any More Logs?' email at about 20:00 UTC on Tuesday evening so you can check that your log has been found OK.
To be included in the combined results your log must arrive at the very
latest by 09:00 UTC on Wednesday 2 Feb.
We hope to complete making the Combined Results within a day or two.
Good listening
If you are interested in some remote listening - maybe due to local
difficulties - you could use any one remote receiver for your loggings
stating its location and with the owner's permission if required.
A remote listener may NOT also use another receiver, either local
or remote, to make further loggings for the same CLE.
Joachim has put together some very helpful guidance on remote
listening using the Kiwi SDRs, WebSDRs, etc. - he'll be posting it
to NDB List before the start of the CLE.
------------------------------------------------------------------
From: Brian Keyte G3SIA ndbcle'at'gmail.com
Location: Surrey, SE England (CLE coordinator)
------------------------------------------------------------------
These listening events serve several purposes. They
• 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.
The NDB List Group is a great place to learn more about the 'Art of NDB DXing' or to meet other DXers in your region. There is a lot of good information available there and new members are always very welcome. As well, you can follow the results of other CLE participants from night to night as propagation is always an active topic of discussion.
You need not be an NDB List member to participate in the CLEs and all reports, no matter how small, are of much value to the organizers.
Remember - 'First-time' logs are always VERY welcome!
Reports may be sent to the NDB List Group or e-mailed to CLE co-ordinator, Brian Keyte (G3SIA), whose address appears above. If you are a member of the group, all final results will also be e-mailed and posted there.
Please ... 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.
Have fun and good hunting!
January’s Crystal Radio DX Contest
The first time I was involved with a crystal radio DX contest was about 20 years ago when I built a well-performing crystal receiver for the Yahoo Crystal Radio Group's annual DX contest. It was a great learning experience and taught me much about circuit losses and how to overcome them. I originally built several sets but was unable to hear anything other than local stations until I eventually figured things out ... the system was only as good as its weakest link or links!
Fast forward to more recently when I obtained and wrote about the Heathkit CR-1 Crystal Radio, a simple but very well-designed tuner that has become popular with collectors. Using the CR-1 re-kindled my interest in the DX contest activity of years ago and when talking with two other amateurs that had an interest as well (one had also been in the earlier contests sponsored by the Alabama Crystal Radio Group), we decided to bring the contest back once again. The Facebook Crystal Radio DX Contest Group was formed last fall, a set of rules drawn up and the contest date set for the first week of January of this year. This gave interested participants plenty of time to build something they could use in the contest.
I spent all of December designing and constructing a new contest radio, hopefully one with enough selectivity to get around the 15 local flamethrowers (10-50kW S9++ signals) that plague the band for me and eventually drove me from crystal radio activities.
The new radio makes use of several 'traps' to null strong signals ... two are in the antenna line while one is loosely coupled inductively to the detector tank circuit. The two inline trap coils are wound with Litz wire on ferrite toroids (R40C1) while the third is a basket-wound Litz coil (660/46) on a 4" diameter form.
The antenna tuning stage also uses the same ferrite material but in the rod / bar form. I wound a low-end as well as a high-end coil for the tuner using the same high-count Litz as on the big trap coil. The low-end coil is wound on a bundle of three rods while the high-end coil uses a single rod.
 |
| Antenna tuner |
The detector stage uses another Litz coil with this one being solenoid-wound on a 4" diameter form. Both the antenna tuner and the detector use excellent quality hi-Q ceramic insulated air variable capacitors (18-360 pfd). All components that handle RF are insulated from the plywood bases in order to reduce losses. Moving a capacitor from the plywood to the insulated standoffs makes a noticeable difference, something learned the hard way years ago but actually measured while using the new radio.
 |
| Detector stage |
The detector also has provisions for comparing various diodes as not all diodes are created equal ... not even all diodes with the same number! When testing and comparing diodes of the same type such as the popular 1N34 germanium, every once in awhile one of them will turn out to be noticeably more sensitive than the others. In my built-in B-A-C diode test module, the hottest diode is always mounted in middle-position A, making it easy to quickly compare by switching to the left for B or to the right for C. So far the best one I have found is the vintage Russian D18 germanium diode but an old 1N34 removed years ago from a 1950s-era Heathkit has given it a good run for the money! I've still several hundreds of early germanium diodes, pulled from old diode matrix boards years ago, to test against the D18 as well as numerous Schottky diodes.
Also on board the detector module is a Selectivity Enhancement Circuit (SEC) that increases selectivity by unloading some of the diode's effect on the detector coil, similarly to tapping the diode further down the tank coil. It uses a small butterfly capacitor seen to the right of the main tuning capacitor in the photo above. I found it extremely effective when needed and is well worth the addition to a high-performance tuner.
The detector stage is followed by an impedance-matching transformer for the sound-powered headphones. This stage also houses a 50uA meter to measure diode current / signal strength levels.
The meter can be switch-bypassed to prevent needle-bounce on stronger signals. It is particularly helpful when using the traps to null a signal to the minimum level.
The three traps utilized have been very effective in eliminating what I had originally perceived as an impossible DXing situation.
Here are the daytime-power signal strengths of my 15 line-of-site blowtorch stations that, without trapping, very effectively block most sections of the band. Anything over 50uA is ear shattering and problematic, usually requiring the use of all 3 traps:
KVRI 1600 50uA
KRPI 1550 100uA
CJVB 1470 40uA
CFTE 1410 350uA
CHMB 1320 100uA
CJRJ 1200 400uA
CKWX 1130 300uA
CKST 1040 90uA
CKNW 980 150uA
KGMI 790 100uA
CHMJ 730 450uA
CBU 690 650uA
CISL 650 200uA
CJWW 600 100uA
KARI 550 100uA
Overall I was very pleased and surprised at the good performance of the new radio. During the contest period I identified and logged 92 unique stations in 16 states / provinces. More than one station was logged on 9 different frequencies as the propagation varied from night to night.
Highlights of the DX Contest were hearing WHAS in Kentucky (2,007 miles), WJR in Michigan (1,970 miles), KXEL in Iowa (1,556 miles), WCCO in Minnesota (1,423 miles) and CBW-990 in Winnipeg, smack up beside local blowtorch CKNW-980! Additionally, hearing Washington state 250 watter KFLD-870 and 250 watt KWBY-940 in Oregon were great surprises.
I found the use of a spotter radio (Sony ICF-2010) to be very useful in locating signals to target and to zero-beat with an RF signal generator. The generator’s tone-modulated signal can then be tuned in and the xtal radio and antenna / detector stages optimized.
From here, any pest signals are then tuned to and individually nulled using the traps while watching the signal meter. Antenna and detector stages are then re-tweaked before disabling the generator and listening for the desired signal.
Often it is heard immediately following the above tuning procedures but if not, monitoring the frequency for several minutes often allows time for the weak signal to fade up to audible levels.
Comparing programming audio with what is heard on the spotter radio will confirm hearing the correct signal as will comparing audio to the station’s own live-feed on the internet.
Due to the larger and much better antenna (inverted-L 70’ x 100’) on the crystal radio, I would often hear good audible signals on it and not on the spotter (something that I found surprising) so often times it was productive to just tune around the band on the crystal radio, tweaking stages as required.
I’m looking forward to further improvements of the tuner as well as to the next DX Contest whenever that will be scheduled ... hopefully you can join in as well!
FREQ UTC STN LOCATION MI
550 1:04 KARI Blaine, WA 25
560 1:30 KPQ Wenatchee, WA 168
570 3:45 KVI Seattle, WA 107
580 3:42 KIDO Nampa, ID 492
600 1:17 CKSP Vancouver, BC 32
610 4:15 KONA Kennewick, WA 271
620 1:22 KPOJ Portland, OR 241
630 3:40 CHED Edmonton, AB 530
630 21:10 KCIS Edmonds, WA 87
650 1:05 CISL Richmond, BC 24
660 3:30 CFFR Calgary, AB 693
660 21:23 KAPS Mt. Vernon, WA 52
670 3:25 KBOI Boise, ID 807
690 1:06 CBU Vancouver, BC 19
710 3:21 KIRO Seattle, WA 108
730 1:02 CHMJ Vancouver, BC 22
750 3:55 KXTG Portland, OR 243
760 4:01 WJR Detroit, MI 1970
770 3:17 KATL Miles City, MT 831
780 4:00 KKOH Reno, NV 658
790 1:07 KGMI Bellingham, WA 39
810 4:05 KGO San Francisco, CA 786
820 1:59 KGNW Seattle, WA 106
830 2:20 WCCO Minneapolis, MN 1423
840 4:10 CFCW Camrose, AB 530
840 4:00 WHAS Louisville, KY 2007
850 4:20 KOA Denver, CO 1118
850 1:12 KHHO Seattle, WA 121
860 3:48 CBKF Saskatoon, SK 758
860 1:04 KPAM Troutdale, OR 226
870 4:30 KFLD Pasco, WA 266
880 1:17 KIXI Seattle, WA 102
890 4:35 CJDC Dawson Creek, BC 494
900 4:38 CKBI Prince Albert, SK 810
910 4:40 CKDQ Drumheller, AB 468
920 4:42 KXLY Spokane, WA 285
930 1:50 KBAI Bellingham, WA 37
940 4:45 CJGX Yorkton, SK 940
940 0:58 KWBY Woodburn, OR 256
950 4:50 KJR Seattle, WA 106
960 4:52 CFAC Calgary, AB 444
970 4:55 KBUL Billings, MT 722
980 1:08 CKNW New Westminster, BC 32
990 4:58 CBW Winnipeg, MB 1156
1000 3:45 KOMO Seattle, WA 105
1010 4:59 CBR Calgary, AB 453
1020 0:54 KWIQ Moses Lake, WA 216
1030 5:06 KTWO Casper, WY 918
1040 1:09 CKST Vancouver, BC 23
1050 5:10 CJNB N Battleford, SK 707
1060 5:07 CKMX Calgary, AB 441
1070 5:10 cfax Victoria, BC 33
1080 0:33 KFXX Portland, OR 232
1090 1:40 KFNQ Seattle, WA 109
1100 3:55 KFAX San Francisco, CA 779
1110 5:15 KRPA Oak Harbor, WA 48
1120 0:48 KPNW Eugene, OR 340
1130 1:10 CKWX Vancouver, BC 22
1140 5:20 CHRB High River, AB 443
1150 5:50 CKFR Kelowna, BC 185
1160 5:53 KSL Salt Lake Cty, UT 781
1170 1:11 KPUG Bellingham, WA 39
1180 5:09 KOFI Kalispell, MT 416
1190 5:55 KEX Portland, OR 241
1200 1:12 CJRJ Vancouver, BC 23
1260 5:58 CFRN Edmonton, AB 522
1290 6:00 KUMA Pendleton, OR 306
1290 6:00 KGVO Missoula, MT 449
1320 1:13 CHMB Vancouver, BC 23
1360 6:12 KKMO Tacoma, WA 115
1370 4:32 KXTL Butte, MT 535
1380 6:16 KRKO Everett, WA 88
1410 1:14 CFTE Vancouver, BC 22
1460 1:55 KUTI Yakima, WA 207
1470 1:15 CJVB Vancouver, BC 25
1480 1:20 KBMS Vancouver, WA 227
1520 1:05 KKXA Snohomish, WA 88
1520 1:13 KQRR Oregon City, OR 241
1530 4:30 KFBK Sacramento, CA 698
1540 1:50 KXPA Bellvue, WA 102
1540 4:46 KXEL Waterloo, IA 1556
1550 1:16 KRPI Ferndale, WA 31
1560 1:14 KVAN Burbank, WA 272
1580 6:25 KGAL Lebanon, OR 297
1590 1:22 KLFE Seattle, WA 91
1600 1:00 KVRI Blaine, WA 25
1620 1:30 KYIZ Renton, WA 111
1640 6:45 KDZR Lake Oswego, OR 239
1660 0:56 KBRE Merced, CA 812
1680 1:35 KNTS Seattle, WA 91
1690 0:53 KFSG Roseville, CA 705
Hunting NDBs In CLE 275
It's holiday CLE time once again. This one is designed to take your mind from your troubles and enjoy a relaxing 10 day beacon hunt!
For example, 'AA' near Fargo, ND, transmitted on 365 kHz and its upper sideband CW identifier was tuned at 366.025 kHz while its lower sideband CW ident could be tuned at 363.946 kHz. Its USB tone was actually 1025 Hz while its LSB tone was 1054 Hz.
Often, one sideband will be much stronger than the other so if you don't hear the first one, try listening on the other sideband.
Canadian NDBs normally have an USB tone only, usually very close to 400 Hz. They also have a long dash (keydown) following the CW identifier.
All NDBs heard in North America will be listed in the RNA database (updated daily) while those heard in Europe may be found in the REU database. Beacons heard outside of these regions will be found in the RWW database. These databases have recently been re-vamped and are slicker than ever before!
From CLE organizers comes the following CLE info:
Hello all
Here are the final details for our holiday listening event.
Please read this carefully to avoid disappointment!
The task is to build a size 10 pyramid, with a size 10 aerial on top.
We hope you will enjoy trying this challenge, whether you are a beginner or have been an NDB listener for many years, and whether you will have a lot of time, or rather little.
|
|
| Days: Saturday 25 Dec. to Monday 3 Jan.
. / \ Times: Midday - Midday, your LOCAL Time
/ \ Frequencies: 190 - 1740 kHz
/ \ Beacons: Normal NDBs (no UNIDs, DGPS, Navtex or Amateur)
~~~~~~~~~~~~~~
You make your pyramid by logging beacons from 19 different radio countries of your choice as follows:
10 different NDBs from the country at the base of the pyramid
9 NDBs from the next radio country
8 NDBs from the third, etc.
- - - all the way to:
2 NDBs from the ninth country at the top of the pyramid.
Finally, your pyramid needs a vertical antenna on it! That is made by logging 10 extra NDBs, each one from yet another different radio country.
An example of a completed pyramid is given at the end of this email.
You can log the NDBs in any time sequence, of course.
IMPORTANT The countries are the same ones that we always use, defined in our Radio Countries List http://www.ndblist.info/ndbinfo/countrylist.pdf
Each USA State, each Australian State and each Canadian Province is a separate radio country.
* If you can't reach size 10, please still send your log.
E.g. a size 7 would have 7 loggings for the base country, then 6, 5, 4, 3 and 2 loggings from five other different countries and, for the antenna, a single logging from each of 7 yet other different countries.
If you reach size 10, there is no need to stop there - with enough time, you could go on and try to build your pyramid bigger and higher by adding more loggings.
E.g. For a size 12 pyramid you would need to log:
12 NDBs from one country and 11, 10, 9, 8, . to 2 loggings from10 other different countries
12 extra loggings from 12 other different countries to make the antenna.
You can get a lot of help in planning your listening from the Rxx database https://rxx.classaxe.com/rww/signals
The 'Help' option explains how you can make very powerful enquiries in the Database.
LOGS: We suggest that you show your loggings in pyramid order. E.g., if you choose top-to-bottom, show each of the '1' loggings first (forming the aerial), then the '2', then the '3', then '4', '5', etc. with just an extra blank line to separate the loggings from different radio countries. There's no need to add any text to describe the levels in your pyramid because the Harvester Software will work that out automatically.
Please include for every logging:
# the UTC date ( e.g. '2021-12-25', etc. )*
# UTC time (the day changes at 00:00 UTC).
# kHz - the NDB's nominal, published, frequency.
# Call Ident.
Show those main log items FIRST. Other details, such as country, location, etc., go LATER on the same line. Do be careful that each of your NDBs really is associated with the radio country you intended.
*If you have made any loggings in January and also in December (by UTC time) we ask you please NOT to use the simple 'dd' date format (that can make difficulties for the good people who enter logs into the RXX database)
UNIDs, though not suitable for this CLE, could be shown in a SEPARATE section of your log, together with other interesting loggings that didn't fit into your pyramid.
Please post your 'Final' log to the List, preferably as a Plain Text email (not in an attachment) using 'CLE275' and 'FINAL' in its title. We'll send an 'Any More Logs?' email at about 18:00 UTC on TUESDAY 4th Jan. so you can check that your log has been found OK. Do make sure that it has arrived on the List by 09:00 UTC on WEDNESDAY 5th Jan. at the very latest.
We hope to finish making the combined results within two or three days.
The size of our pyramids will depend a lot on where each of us happens to be located. If you are unlucky there, why not try listening via a suitable remote receiver that gives good NDB listening?
You could use any one remote receiver for your loggings, stating its location and owner - with their permission if required.
A remote listener may NOT also use another receiver, whether
Local or remote, to obtain further loggings for a CLE.
As with all our CLEs, this is intended to be an educational and 'fun' event
- it's not a contest!
Enjoy your listening - you may find it quite addictive this time!
The COVID difficulties have made things really hard for most of us, but maybe a bit of pyramid-building will provide a safe and relaxing escape for a while!
Joachim and I hope you have a very Happy Christmas and many good things during 2022.
73
Brian and Joachim
--------------------------------------------------------------------
From: Brian Keyte G3SIA ndbcle'at'ndblist.info
Location: Surrey, SE England (CLE coordinator)
---------------------------------------------------------------------
Here is an imaginary example of a pyramid with its antenna,
maybe for a listener in British Columbia (BC).
Each B is a different Beacon:
B GRL 1 ndb
B PTR 1 ndb
B AZ 1 ndb
B NE 1 ndb
B IA 1 ndb
B NT 1 ndb
B CA 1 ndb
B CO 1 ndb
B NC 1 ndb
B ON 1 ndb
B B HWA 2 ndbs
B B B OR 3 ndbs
B B B B MB 4 ndbs
B B B B B WA 5 ndbs
B B B B B B MT 6 ndbs
B B B B B B B SK 7 ndbs
B B B B B B B B ALS 8 ndbs
B B B B B B B B B BC 9 ndbs
B B B B B B B B B B AB 10 ndbs
These listening events serve several purposes. They
• 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.
The NDB List Group is a great place to learn more about the 'Art of NDB DXing' or to meet other DXers in your region. There is a lot of good information available there and new members are always very welcome. As well, you can follow the results of other CLE participants from night to night as propagation is always an active topic of discussion.
You need not be an NDB List member to participate in the CLEs and all reports, no matter how small, are of much value to the organizers.
Remember - 'First-time' logs are always VERY welcome!
Reports may be sent to the NDB List Group or e-mailed to CLE co-ordinator, Brian Keyte (G3SIA), whose address appears above. If you are a member of the group, all final results will also be e-mailed and posted there.
Please ... 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.
Have fun and good hunting!
Cycle 25 … On The Move?
Anyone looking at the Sun this week has to be impressed with its sudden reawakening over the past few days. From its recent somewhat troubling slumber, with flux numbers in the high 70s, these values have quickly risen to a Cycle 25 high in the 120s as of early Saturday. With at least two more active regions about to rotate into view shortly, it seems as though these numbers might continue to grow.
What is interesting is the suddenness with which these groups formed as this is a keystone marker for the long awaited ‘terminator’ event … the point at which cycle growth starts to increase rapidly. Is this it or will the Sun go back to sleep as it has in the past few excursions into the 90’s?
If this rapid increase does indeed herald the terminator's arrival, it’s a sign that Cycle 25 should be one of above average strength. Wouldn’t that be nice after Cycle 24’s weak showing over the past 11 years.
With the present asymmetry of the Sun's two hemisphere, we are guaranteed a cycle with a double hump in the peak years. The first peak is usually the strongest but not always. Let's see how Cycle 25 plays out in this department.
I’ve yet to do any comparisons with past progress of strong cycles at this same point into their upward climb but let’s cross our fingers and hope the present numbers continue for some time. There will always be drops of course but if recovery is quick, we may still be in for a good ride in Cycle 25.
Hunting For NDBs In CLE 274
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| ZWG - 287kHz Winnipeg courtesy: http://www.ve3gop.com/ |
I know it's hard to believe but it's CLE time once again. How quickly time zooms by.
When tuning for NDBs, put your receiver in the CW mode and listen for the NDB's CW identifier, repeated every few seconds. Listen for U.S. NDB identifiers approximately 1 kHz higher or lower than the published transmitted frequency since these beacons are modulated with a 1020 Hz tone approximately.
For example, 'AA' near Fargo, ND, transmitted on 365 kHz and its upper sideband CW identifier was tuned at 366.025 kHz while its lower sideband CW ident could be tuned at 363.946 kHz. Its USB tone was actually 1025 Hz while its LSB tone was 1054 Hz.
Often, one sideband will be much stronger than the other so if you don't hear the first one, try listening on the other sideband.
Canadian NDBs normally have an USB tone only, usually very close to 400 Hz. They also have a long dash (keydown) following the CW identifier.
All NDBs heard in North America will be listed in the RNA database (updated daily) while those heard in Europe may be found in the REU database. Beacons heard outside of these regions will be found in the RWW database. These databases have recently been re-vamped and are slicker than ever before!
From CLE organizers comes the following CLE info:
Hello all
Here are brief details for our 274th co-ordinated listening event next weekend.
It spans a 50 kHz frequency range - about three times wider than usual.
In that range, the Rxx database is showing about 200 active NDBs located in Europe, 120 in North America, 35 in Oceania. The numbers are approximately doubled if you include DX from other parts of the World that have been heard from each of those three regions.
Days: Friday 26 November – Monday 29 November
Times: Start and end at midday, your LOCAL time
Range: 270.0 - 319.9 kHz (NDB signals only)
Part of the frequency range also has DGPS signals among the NDBs.
We last listened on these frequencies in CLE259 in August 2020.
Any first-time CLE logs will be very welcome, as always.
Send your final log to the List (not in an attachment, please) with 'CLE274’ and ‘FINAL' in its title (important).
Show on each line:
# The Date (e.g. '2021-11-26', etc., or just '26' )
# The Time in UTC (the day changes at 00:00 UTC).
# kHz - the nominal published frequency, if known.
# The Call Ident.
Please show those main items FIRST. Other optional details such as Location and Distance go LATER in the same line.
As always, of course, tell us your own location and give brief details of the equipment that you were using during the Event.
We will send the usual 'Any More Logs?' email at about 19:00 UTC on Tuesday so you can check that your log has been found OK.
Do make sure that your log has arrived on the List by 08:00 UTC on Wednesday 01 December at the very latest.
We hope to complete making the combined results within a day or two.
You can soon find full details about current and past CLEs from the CLE page http://www.ndblist.info/cle.htm It includes access to the CLE274 seeklists for your part of the World, prepared from all the previous loggings in Rxx.
Good listening
- enjoy the CLE.
Brian and Joachim
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From: Brian Keyte G3SIA ndbcle'at'gmail.com
Location: Surrey, SE England (CLE coordinator)
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(If you would like to listen remotely you could use any one remote receiver 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 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.
The NDB List Group is a great place to learn more about the 'Art of NDB DXing' or to meet other DXers in your region. There is a lot of good information available there and new members are always very welcome. As well, you can follow the results of other CLE participants from night to night as propagation is always an active topic of discussion.
You need not be an NDB List member to participate in the CLEs and all reports, no matter how small, are of much value to the organizers.
Remember - 'First-time' logs are always VERY welcome!
Reports may be sent to the NDB List Group or e-mailed to CLE co-ordinator, Brian Keyte (G3SIA), whose address appears above. If you are a member of the group, all final results will also be e-mailed and posted there.
Please ... 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.
Have fun and good hunting!
