AmateurRadio.com

HAKUNA MATATA

It may not have been the YASME but the recent voyage of the HAKUNA MATATA had all of the radio fun that one might ask for during the mid-summer doldrums! (more later for those too young to recall the YASME)



Crewed by Mark (VA7MM) and YL May (VA7MAY), Toby (VE7CNF) and XYL Nancy, the 31' Benateu recently completed a 14-day circumnavigation of Georgia Strait's Gulf Islands. This is a yearly adventure that has been successfully completed for the past few summers and looks as though it may now be an annual tradition.

Normally, the crew kept up regular radio contact on HF as well as on VHF when possible but this year saw a major departure.

In previous summers, near the end of the voyage, the crew has always visited us here on Mayne Island for an afternoon of vittles and libation before heading for home. There is always a good amount of time spent recalling the past-year's radio activities, winter projects and reminiscence of the 'good old days'. Last year, just as the party was ending, I jokingly suggested that 'next year', it would be cool to work them from the boat on 630m.

Although there was no immediate commitment, I knew that the seed had been planted, and with three of the four crew being engineers, I suspected it might be hard for them to resist, and ... just before departure, the local bunch of 630m ops were put on alert to be watching for CF7MM/mm on 475 kHz CW as they would be attempting to work us from three different overnight anchorages during their summer voyage!

Evidently Toby had been working quietly during the winter to make this become a reality. Here are some pictures of the system along with Toby's (the system's builder) comments.

Variometer and matching transformer

I have attached photos of the CF7MM/MM 630m setup on Hakuna Matata. The lower black toolbox holds a variometer with selectable taps and a matching toroidal autotransformer with selectable taps. At the base of the antenna is another series loading coil.

Wire vertical and loading coil

The antenna wire is 14 ga 38 ft long with plastic Unadilla "END-sulators" at each end. Ground was the boats's cast steel keel and a couple of 30 ft wires near the gunnels. The rig is an IC-746 with my power-mixer transverter. Transmit power was about 20W TPO.

Toby (VE7CNF) working the pileups!

Tuning and matching was done with a resistive voltage divider setup, signal generator, and portable oscilloscope. Once the matching was figured out, I could re-tune the variometer to give a dip on the transverter's RF voltmeter and check that we had the same RF voltage as with a dummy load connected.

Tuneup

The antenna equivalent circuit is approximately 100 pF in series with 27 ohms. Coil losses were 23 ohms for about 50 ohms total load resistance, so the matching autotransformer was not used. The base loading coil is approximately 170 uH and the variometer is 950 uH, for 1120 uH total inductance.

The route, heading north from Vancouver

We tried disconnecting the gunnel ground wires and leaving only the keel, and found that the antenna capacitance and resistance did not change. When we disconnected the keel and left only the gunnel wires, the antenna capacitance dropped to about 87pF and antenna resistance dropped by a few ohms. It appears that the keel provided most of our ground coupling to sea water and it would have been a sufficient ground on its own.

More details of Toby's 630m transverter as well as a practical 630m antenna tune-up procedure can be found on his website here.

All-in-all, I think the 630m operation was a great success and very likely the first-ever 630m marine mobile operation on that band, as I don't recall this happening anywhere else over the years. It was also a great way to pay homage to the band's original maritime heritage where its quality groundwave and skywave capabilities were used to advantage for so many decades safeguarding mariners worldwide.



Maritime mobile operation on the amateur bands has some great history behind it, including the yacht YASME. In the mid-50's, Danny Weil was the first ever amateur to undertake DX'pedition style operations via sailboat, as he visited numerous rare islands in the Caribbean and South Pacific.

Danny on the YASME - courtesy: www.gm3itn.co.uk

Original YASME QSL -  courtesy: http://hamgallery.com/

His exploits were regularly published in CQ magazine at the time and always made for exciting reading as Danny would eventually wreck three YASMES over the years! His adventures laid the groundwork for future island-hopping DX operations such as those undertaken by Gus Browning (W4BPD), Don Miller (W9WNV) and all that followed ... I'm sure they would all have enjoyed working the HAKUNA MATATA as well!

HAKUNA MATATA

It may not have been the YASME but the recent voyage of the HAKUNA MATATA had all of the radio fun that one might ask for during the mid-summer doldrums! (more later for those too young to recall the YASME)



Crewed by Mark (VA7MM) and YL May (VE7MAY), Toby (VE7CNF) and XYL Nancy, the 31' Benateu recently completed a 14-day circumnavigation of Georgia Strait's Gulf Islands. This is a yearly adventure that has been successfully completed for the past few summers and looks as though it may now be an annual tradition.

Normally, the crew kept up regular radio contact on HF as well as on VHF when possible but this year saw a major departure.

In previous summers, near the end of the voyage, the crew has always visited us here on Mayne Island for an afternoon of vittles and libation before heading for home. There is always a good amount of time spent recalling the past-year's radio activities, winter projects and reminiscence of the 'good old days'. Last year, just as the party was ending, I jokingly suggested that 'next year', it would be cool to work them from the boat on 630m.

Although there was no immediate commitment, I knew that the seed had been planted, and with three of the four crew being engineers, I suspected it might be hard for them to resist, and ... just before departure, the local bunch of 630m ops were put on alert to be watching for CF7MM/mm on 475 kHz CW as they would be attempting to work us from three different overnight anchorages during their summer voyage!

Evidently Toby had been working quietly during the winter to make this become a reality. Here are some pictures of the system along with Toby's (the system's builder) comments.

Variometer and matching transformer

I have attached photos of the CF7MM/MM 630m setup on Hakuna Matata. The lower black toolbox holds a variometer with selectable taps and a matching toroidal autotransformer with selectable taps. At the base of the antenna is another series loading coil.

Wire vertical and loading coil

The antenna wire is 14 ga 38 ft long with plastic Unadilla "END-sulators" at each end. Ground was the boats's cast steel keel and a couple of 30 ft wires near the gunnels. The rig is an IC-746 with my power-mixer transverter. Transmit power was about 20W TPO.

Toby (VE7CNF) working the pileups!

Tuning and matching was done with a resistive voltage divider setup, signal generator, and portable oscilloscope. Once the matching was figured out, I could re-tune the variometer to give a dip on the transverter's RF voltmeter and check that we had the same RF voltage as with a dummy load connected.

Tuneup

The antenna equivalent circuit is approximately 100 pF in series with 27 ohms. Coil losses were 23 ohms for about 50 ohms total load resistance, so the matching autotransformer was not used. The base loading coil is approximately 170 uH and the variometer is 950 uH, for 1120 uH total inductance.

The route, heading north from Vancouver

We tried disconnecting the gunnel ground wires and leaving only the keel, and found that the antenna capacitance and resistance did not change. When we disconnected the keel and left only the gunnel wires, the antenna capacitance dropped to about 87pF and antenna resistance dropped by a few ohms. It appears that the keel provided most of our ground coupling to sea water and it would have been a sufficient ground on its own.

More details of Toby's 630m transverter as well as a practical 630m antenna tune-up procedure can be found on his website here.

All-in-all, I think the 630m operation was a great success and very likely the first-ever 630m marine mobile operation on that band, as I don't recall this happening anywhere else over the years. It was also a great way to pay homage to the band's original maritime heritage where its quality groundwave and skywave capabilities were used to advantage for so many decades safeguarding mariners worldwide.



Maritime mobile operation on the amateur bands has some great history behind it, including the yacht YASME. In the mid-50's, Danny Weil was the first ever amateur to undertake DX'pedition style operations via sailboat, as he visited numerous rare islands in the Caribbean and South Pacific.

Danny on the YASME - courtesy: www.gm3itn.co.uk

Original YASME QSL -  courtesy: http://hamgallery.com/

His exploits were regularly published in CQ magazine at the time and always made for exciting reading as Danny would eventually wreck three YASMES over the years! His adventures laid the groundwork for future island-hopping DX operations such as those undertaken by Gus Browning (W4BPD), Don Miller (W9WNV) and all that followed ... I'm sure they would all have enjoyed working the HAKUNA MATATA as well!

YBV - 370kHz  (VE3GOP)

This coming weekend will see another CLE challenge. This time the hunting grounds will be:  370.0 - 384.9 kHz.







For those unfamiliar with this monthly activity, a 'CLE' is a 'Co-ordinated Listening Event', as NDB DXers around the world focus their listening time on one small slice of the NDB spectrum.

A nice challenge in this one is to hear the Berens River (Manitoba)  NDB, 'YBV', on 370 kHz. 'YBV' is a 25-watter and is well heard, having been logged from coast-to-coast as well as in Europe. Look for 'YBV's CW identifier, repeated every 10.4 seconds, on 370.373 kHz with your receiver in the CW mode.

YBV's 25W TX Rack (VE3GOP)

Summertime CLEs can often be challenging, not because of poor propagation but more likely, summer lightning storms ... hopefully it will be quiet for your location.

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' in Fargo transmits on 365 kHz and its upper sideband CW identifier is tuned at 366.025 kHz while its lower sideband CW ident can be tuned at 363.946 kHz. Its USB tone is actually 1025 Hz while its LSB tone is 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 organizer Brian Keyte, G3SIA, comes the usual 'heads-up':


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. As well, you can follow the results of other CLE participants from night to night as propagation is always an active topic of discussion.

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 ... 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.

Good hunting!

YBV - 370kHz  (VE3GOP)

This coming weekend will see another CLE challenge. This time the hunting grounds will be:  370.0 - 384.9 kHz.







For those unfamiliar with this monthly activity, a 'CLE' is a 'Co-ordinated Listening Event', as NDB DXers around the world focus their listening time on one small slice of the NDB spectrum.

A nice challenge in this one is to hear the Berens River (Manitoba)  NDB, 'YBV', on 370 kHz. 'YBV' is a 25-watter and is well heard, having been logged from coast-to-coast as well as in Europe. Look for 'YBV's CW identifier, repeated every 10.4 seconds, on 370.373 kHz with your receiver in the CW mode.

YBV's 25W TX Rack (VE3GOP)

Summertime CLEs can often be challenging, not because of poor propagation but more likely, summer lightning storms ... hopefully it will be quiet for your location.

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' in Fargo transmits on 365 kHz and its upper sideband CW identifier is tuned at 366.025 kHz while its lower sideband CW ident can be tuned at 363.946 kHz. Its USB tone is actually 1025 Hz while its LSB tone is 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 organizer Brian Keyte, G3SIA, comes the usual 'heads-up':


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. As well, you can follow the results of other CLE participants from night to night as propagation is always an active topic of discussion.

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 ... 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.

Good hunting!

Participants in the central states seemed to enjoy much greater groundwave coverage than here on the west coast. It seems that the rugged Coastal ranges and the Rockies do have a pronounced effect on daylight propagation when skywave is not involved. Beacon ERP cannot be ignored as well as location and ground system efficiency ... some definitely get out much better than others even though output powers may be the same.

Anthony Casorso, ADØVC, listening near Denver, Colorado with an Elad SDR and a 17' Low Noise Vertical (LNV), managed several +500 mile catches but all N-S or to the east.

Bill Riches, WA2DVU, in Cape May, NJ, found SJ-212 in Saint John, New Brunswick, 635 miles to the north with his Perseus and Wellbrook loop.

Dave Tomasko, K9QU, in Galena, Illinois, caught OKS-233 in Oshkosh, NE at 625 miles and FOR-236 in Forsyth, Montana, at a whopping 845 miles with his R-75 and Wellbrook ALA100 loop. 

These were heard here at 11 a.m. local time using my Perseus SDR and inverted-L tuned to 300kHz:

24 18:00 200.0  YJ   Victoria - Sidney Island, BC, CAN
24 18:00 203.0  YBL  Campbell River, BC, CAN
24 18:00 214.0  LU   'Cultus' Abbotsford, BC, CAN
24 18:00 216.0  GRF  GRAYE - Fort Lewis, WA, USA
24 18:00 223.0  YKA  Kamloops, BC, CAN
24 18:00 227.0  CG   Castlegar, BC, CAN
24 18:00 236.0  YZA  Ashcroft, BC, CAN
24 18:00 240.0  BVS  Skagit/Bay View - Burlington, WA, USA
24 18:00 242.0  ZT   Port Hardy, BC, CAN
24 18:00 248.0  ZZP  Dead Tree - Queen Charlotte Is, BC, CAN
24 18:00 251.0  YCD  Nanaimo, BC, CAN
24 18:00 257.0  LW   Kelowna - Wood Lake, BC, CAN
24 18:00 266.0  VR   Vancouver - Lulu Island, BC, CAN
24 18:00 269.0  YK   'Brilliant' Castlegar, BC, CAN
24 18:00 272.0  XS   Prince George, BC, CAN
24 18:00 284.0  FHR  Friday Harbor Apt, WA, USA
24 18:00 290.0  YYF  Penticton, BC, CAN
24 18:00 293.0  MB   Mill Bay - Sidney, BC, CAN
24 18:00 312.0  UNT  Naramata, BC, CAN
24 18:00 325.0  YJQ  Bella Bella (Campbell Island), BC, CAN
24 18:00 326.0  DC   Princeton Municipal Apt, BC, CAN
24 18:00 328.0  LAC  'Lacomas' Fort Lewis, WA, USA
24 18:00 332.0  WC   White Rock (Abbotsford), BC, CAN
24 18:00 338.0  K    Ediz Hook - Port Angeles, WA, USA
24 18:00 344.0  XX   Abbotsford, BC, CAN
24 18:00 348.0  MNC  'Mason Co' Shelton, WA, USA
24 18:00 350.0  NY   Enderby, BC, CAN
24 18:00 353.0  RNT  Renton Municipal Apt, WA, USA
24 18:00 356.0  ON   'Okanagan' Penticton, BC, CAN
24 18:00 359.0  YQZ  Quesnel, BC, CAN
24 18:00 359.0  YAZ  Tofino - Vancouver Island, BC, CAN
24 18:00 362.0  BF   'Nolla' Seattle, WA, USA
24 18:00 368.0  ZP   Sandspit - Moresby Island, BC, CAN
24 18:00 371.0  YK   'Donny' Yakima, WA, USA
24 18:00 374.0  EX   Rutland (Kelowna), BC, CAN
24 18:00 378.0  AP   Active Pass (Mayne Island), BC, CAN
24 18:00 382.0  YPW  Powell River, BC, CAN
24 18:00 382.0  AW   WATON - Marysville, WA, USA
24 18:00 385.0  WL   Williams Lake, BC, CAN
24 18:00 389.0  YWB  Kelowna, BC, CAN
24 18:00 400.0  QQ   Comox, BC, CAN
24 18:00 408.0  MW   PELLY - Moses Lake, WA, USA
24 18:00 414.0  YZK  Harper Ranch, BC, CAN
24 18:00 515.0  CL   ELWHA - Cresent Beach, WA, USA

Participants in the central states seemed to enjoy much greater groundwave coverage than here on the west coast. It seems that the rugged Coastal ranges and the Rockies do have a pronounced effect on daylight propagation when skywave is not involved. Beacon ERP cannot be ignored as well as location and ground system efficiency ... some definitely get out much better than others even though output powers may be the same.

Anthony Casorso, ADØVC, listening near Denver, Colorado with an Elad SDR and a 17' Low Noise Vertical (LNV), managed several +500 mile catches but all N-S or to the east.

Bill Riches, WA2DVU, in Cape May, NJ, found SJ-212 in Saint John, New Brunswick, 635 miles to the north with his Perseus and Wellbrook loop.

Dave Tomasko, K9QU, in Galena, Illinois, caught OKS-233 in Oshkosh, NE at 625 miles and FOR-236 in Forsyth, Montana, at a whopping 845 miles with his R-75 and Wellbrook ALA100 loop. 

These were heard here at 11 a.m. local time using my Perseus SDR and inverted-L tuned to 300kHz:

24 18:00 200.0  YJ   Victoria - Sidney Island, BC, CAN
24 18:00 203.0  YBL  Campbell River, BC, CAN
24 18:00 214.0  LU   'Cultus' Abbotsford, BC, CAN
24 18:00 216.0  GRF  GRAYE - Fort Lewis, WA, USA
24 18:00 223.0  YKA  Kamloops, BC, CAN
24 18:00 227.0  CG   Castlegar, BC, CAN
24 18:00 236.0  YZA  Ashcroft, BC, CAN
24 18:00 240.0  BVS  Skagit/Bay View - Burlington, WA, USA
24 18:00 242.0  ZT   Port Hardy, BC, CAN
24 18:00 248.0  ZZP  Dead Tree - Queen Charlotte Is, BC, CAN
24 18:00 251.0  YCD  Nanaimo, BC, CAN
24 18:00 257.0  LW   Kelowna - Wood Lake, BC, CAN
24 18:00 266.0  VR   Vancouver - Lulu Island, BC, CAN
24 18:00 269.0  YK   'Brilliant' Castlegar, BC, CAN
24 18:00 272.0  XS   Prince George, BC, CAN
24 18:00 284.0  FHR  Friday Harbor Apt, WA, USA
24 18:00 290.0  YYF  Penticton, BC, CAN
24 18:00 293.0  MB   Mill Bay - Sidney, BC, CAN
24 18:00 312.0  UNT  Naramata, BC, CAN
24 18:00 325.0  YJQ  Bella Bella (Campbell Island), BC, CAN
24 18:00 326.0  DC   Princeton Municipal Apt, BC, CAN
24 18:00 328.0  LAC  'Lacomas' Fort Lewis, WA, USA
24 18:00 332.0  WC   White Rock (Abbotsford), BC, CAN
24 18:00 338.0  K    Ediz Hook - Port Angeles, WA, USA
24 18:00 344.0  XX   Abbotsford, BC, CAN
24 18:00 348.0  MNC  'Mason Co' Shelton, WA, USA
24 18:00 350.0  NY   Enderby, BC, CAN
24 18:00 353.0  RNT  Renton Municipal Apt, WA, USA
24 18:00 356.0  ON   'Okanagan' Penticton, BC, CAN
24 18:00 359.0  YQZ  Quesnel, BC, CAN
24 18:00 359.0  YAZ  Tofino - Vancouver Island, BC, CAN
24 18:00 362.0  BF   'Nolla' Seattle, WA, USA
24 18:00 368.0  ZP   Sandspit - Moresby Island, BC, CAN
24 18:00 371.0  YK   'Donny' Yakima, WA, USA
24 18:00 374.0  EX   Rutland (Kelowna), BC, CAN
24 18:00 378.0  AP   Active Pass (Mayne Island), BC, CAN
24 18:00 382.0  YPW  Powell River, BC, CAN
24 18:00 382.0  AW   WATON - Marysville, WA, USA
24 18:00 385.0  WL   Williams Lake, BC, CAN
24 18:00 389.0  YWB  Kelowna, BC, CAN
24 18:00 400.0  QQ   Comox, BC, CAN
24 18:00 408.0  MW   PELLY - Moses Lake, WA, USA
24 18:00 414.0  YZK  Harper Ranch, BC, CAN
24 18:00 515.0  CL   ELWHA - Cresent Beach, WA, USA

AP-378 Mayne Island, BC

It's hard to believe but this coming weekend will see another CLE challenge!





No need however, to stay up until the wee hours for this one, as CLE220 is a mid-day affair ... just log what you are able to hear during the day from your location. The entire band is fair-game as well, from 190 - 1740kHz.

Everyone is encouraged to send their logs (see below) so the RNA / REU NDB databases can be kept as up-to-date as possible.

I know that I won't have any trouble hearing AP-378 shown above since it's only about 3/4 mile from my antenna! I'm always curious just how far it can be heard during the day and would encourage listeners on the west coast to have a good listen for it and please let me know if you can hear it.

For those unfamiliar with this monthly activity, a 'CLE' is a 'Co-ordinated Listening Event', as NDB DXers around the world focus their listening time  usually on one small slice of the NDB spectrum.

When tuning for NDBs, put your receiver in the CW mode and listen for the NDB's CW identifier, repeated every few seconds. With your receiver in the CW mode, listen for U.S. NDB identifiers approximately 1 kHz higher or lower than the published transmitted frequency since these beacons are tone-modulated with a 1020 Hz tone approximately.
For example, 'AA' near Fargo, ND, transmits on 365 kHz and its upper sideband CW identifier is tuned at 366.025 kHz while its lower sideband CW ident can be tuned at 363.946 kHz. Its USB tone is actually 1025 Hz while its LSB tone is 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 organizer Brian Keyte, G3SIA, comes the usual 'heads-up':


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. It's also a good place to submit your CLE log! 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.

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 ... 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.

Good hunting!