Barn Door Wide! Hunting For NDBs In CLE253

This weekend's upcoming CLE event will be the "Barn Door" listening event.




Participants are required to use receivers without the usual narrow filters. Some of the older tube radios can do this easily as can most homebrew receivers ... especially the regens!

If you've never listened to the NDB band with a wide bandwidth, it is a fascinating experience! If conditions are normal, you can typically hear a half dozen or more signals, all at various pitches, vying for your attention. It's almost as if you have plunked yourself down in the middle of the NDB forest of signals, and they are coming at you from all directions.

Many choose to use one of their homebrew receivers for this event, often as simple as a '1AD' or a '1 Active Device' circuit.

From organizer Brian Keyte:

Hello all

Here comes our sixth 'Barn Door' Coordinated Listening Event.

Between us there will be a great variety of ‘Back to Basics’ receiver

types in use.  Maybe this is an opportunity for you to bring back to life

that old receiver that has been collecting dust for so long!

    Days:      Friday 21 to Monday 24 February 2020

    Times:    Start at Midday on Friday 21st, your LOCAL time
                   End at  Midday on Monday 24th, your LOCAL time

    Frequencies:   Centred on 360 kHz (see below)

    NDBs:     NOT MORE than 100 'normal' NDBs including any UNIDs
                    (That is not intended to be a target to reach)

 

We are all asked to listen with NON-SELECTIVE receivers - i.e. with a WIDE

filter or NO filter.  Your 'barn door' should be open wide so you could hear,

at the same time, any NDBs 2 kHz away on both sides of your receiver

setting -  E.g. NDBs on 348, 349, 350, 351 and 352 kHz with the receiver

set to 350 kHz.

You could listen with:

Whichever you choose, use the same receiver throughout the CLE.

If your choice of receiver includes a waterfall please use only the

audio output for your listening.   You could even cover part of the

screen if there is no other way of stopping or hiding the waterfall.

Unfortunately the use of Pskov – and probably of recordings – is

not appropriate for this CLE.

You choose how wide a RANGE of frequencies you will listen in, CENTRED

ON 360 kHz. You could choose 350-370 kHz , 330-390 kHz, 260-460 kHz, etc.

   (That allows each of us to choose a +/- range with enough NDBs to

    match our equipment's capability.   It will also allow us to compare our

    loggings in the Combined Results, at least around 360 kHz).

Logs should show not more than 100 NDBs please (if more than 100

the harvester program will 'drop' the loggings furthest from 360 kHz).

We’ll summarise everyone's equipment on the first page of the combined

results, so please describe:

The RECEIVER/AERIAL you used and the FILTER(s) selected and,

if homebrew, the number of active devices used, transistor types, etc.

All the usual procedures for making logs apply:

Send your CLE log to NDB List, not in an attachment.

Please show on EVERY LINE of your log:

    # The full date (or Day No.) and UTC (the day changes at 00:00 UTC).

    # kHz - the beacon's nominal published frequency, if known.

    # The Call Ident.

Show those main items FIRST on each line, before other optional details

such as Location, Distance, etc.  Please send your complete log with

CLE253 and FINAL in the Subject line.

Whether you are a first time CLE-er or a regular, always make your log

interesting to everyone by giving your own location and do feel free

to share any comments you have on this unusual event.

Joachim or I will send the usual 'Any More Logs?' email at about 2000 UTC

on Tuesday 25th so that you can check that your log has been found OK.

Make sure your log has arrived on the List at the very latest by 09:00 UTC

on Wednesday 26th February.   

We’ll try to complete making the combined results a day or so later.

However you choose to take part, we hope you will find your 'back to basics'

listening enjoyable and worthwhile.

  Brian

------------------------------------------------------------------

From:   Brian Keyte  G3SIA          ndbcle'at'gmail.com

Location: Surrey, SE England         (CLE coordinator)

-------------------------------------------------------------------

P.S.  NOT FOR YOU?

Listening without narrow filters is not going to revolutionise our hobby!

But there ARE some unexpected benefits and advantages:

1. Hearing several beacons on a few adjacent frequencies at the same time

becomes easier as you get practice at recognising them by listening to their

very different audio tones. At first, when listening to a random frequency

setting, you may hear just one or two beacons.  But after listening for a

little while you realise that there are three - - four, maybe more, all of

them audible without altering any of the receiver controls.

It is a skill that gives satisfaction as you improve.

2. Hearing multiple beacons like that can be useful because, with no extra

tools, you can hear NDBs over a wide frequency range much more quickly than usual, perhaps spotting the arrival of new UNIDs or the return of occasional beacons.  (To protect your hearing, keep your receiver gain controls fairly low, except around very quiet frequencies).

3. With normal listening it is easy to miss any NDBs that have abnormal

carrier frequencies or non-standard offsets.  With 'Barn Door' listening

they won't escape because everything is let through.

4. When using a wide filter, you may be surprised by hearing some

Broadcast Station signals (e.g. harmonics) among the NDBs and you will

be able to identify them.

With a narrow filter, often you may not recognise an AM signal as audio

- it just sounds like nondescript 'hash' affecting a wide range of frequencies

around the central carrier.

Maybe listeners will report some other good things about their barn door

listening during the CLE - and probably some bad things too!

Do join in if you can.

**************************

  
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.


The NDB List 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. 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!