AmateurRadio.com

courtesy: https://sdo.gsfc.nasa.gov/

This past weekend's CLE event was, as is so often the case, perfectly timed with the arrival of poor propagation in most parts of the world. This time around, it was particularly bad.

The 'Co-ordinated Listening Event' might more aptly be called the 'Cursed Listening Event' as once again the same large coronal hole (shown above) that has been present for several solar rotations seems to be more disruptive than ever. The subsequent higher than normal solar wind speeds causing widespread auroral conditions and elevated K indices have pretty much made a mess of MF and HF radio for the past several days.

courtesy: http://www.noaa.gov/

NDB-band recordings made with the Perseus SDR for the three-night event turned up very little activity other than a few strange hot-spots. Both 'OIN' in Kansas and 'CC' in California were strong on all three nights! Nothing from eastern Canada was heard and one of Alaska's strongest signals, 'ELF', was barely detected. Only the following few stations were logged:

23 08:00 341.0    ELF  Cold Bay, ALS
22 06:00 338.0    ZU   Whitecourt, AB, CAN
22 06:00 343.0    YZH  Slave Lake, AB, CAN
22 04:00 344.0    YC   Calgary, AB, CAN
22 12:00 338.0    RYN  Tucson, AZ, USA
22 04:00 344.0    XX   Abbotsford, BC, CAN
22 12:00 335.0    CC   Concord, CA, USA
22 10:00 344.0    FCH  Fresno, CA, USA
22 08:00 341.0    OIN  Oberlin, KS, USA
22 04:00 344.0    BKU  Baker, MT, USA
24 08:00 335.0    BK   Brookings, SD, USA
22 04:00 347.0    PA   Prince Albert, SK, CAN
22 08:00 338.0    K    Port Angeles, WA, USA
22 04:00 348.0    MNC  Shelton, WA, USA
22 05:00 341.0    DB   Burwash, YT, CAN

I suspect the this same coronal hole will be with us for several more rotations ... perhaps it's time fool Ol' Sol and stagger our CLE's 28-day cycle so it doesn't continue go sync-up with poor band conditions but somehow I think that Murphy might not be so easily duped!

'XX-344' - Abbotsford, BC

This coming weekend will see another CLE challenge. This time the hunting grounds will be:  335.0 - 349.9 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 Abbotsford  NDB, 'XX', on 344 kHz. 'XX' is located about 40 miles east of  Vancouver International (YVR) and a few miles SW of the Abbotsford Airport, YVR's alternate for those foggy winter nights. 'XX' is a 500-watter and is well heard, having been logged from the east coast to Hawaii and is a good propagation indicator for listeners in eastern North America. Look for 'XX' on 344.404 kHz with your receiver in the CW mode.

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' in Fargo, MN, 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':

Hello all

Our 218th Co-ordinated Listening Event is less than a week 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 21 April - Monday 24 April
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.

We last concentrated on these frequencies for CLE200 in Nov. 2015
when 55 of us joined in.

73
Brian
----------------------------------------------------------
From: Brian Keyte G3SIA ndbcle'at'gmail.com
Location: Surrey, SE England (CLE coordinator)
----------------------------------------------------------
(Reminder: 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 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. 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!

'XX-344' - Abbotsford, BC

This coming weekend will see another CLE challenge. This time the hunting grounds will be:  335.0 - 349.9 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 Abbotsford  NDB, 'XX', on 344 kHz. 'XX' is located about 40 miles east of  Vancouver International (YVR) and a few miles SW of the Abbotsford Airport, YVR's alternate for those foggy winter nights. 'XX' is a 500-watter and is well heard, having been logged from the east coast to Hawaii and is a good propagation indicator for listeners in eastern North America. Look for 'XX' on 344.404 kHz with your receiver in the CW mode.

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' in Fargo, MN, 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':

Hello all

Our 218th Co-ordinated Listening Event is less than a week 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 21 April - Monday 24 April
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.

We last concentrated on these frequencies for CLE200 in Nov. 2015
when 55 of us joined in.

73
Brian
----------------------------------------------------------
From: Brian Keyte G3SIA ndbcle'at'gmail.com
Location: Surrey, SE England (CLE coordinator)
----------------------------------------------------------
(Reminder: 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 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. 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!

CLE 216 NA Targets!

This coming weekend will see another CLE challenge. This time the hunting grounds will be:  320.0 - 334.9 kHz.






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 White Rock NDB, 'WC', on 332 kHz. The 'WC' NDB is located just a few hundred feet from the Canada - U.S. border, about 25 miles south east of the Vancouver International airport and about 20 miles west of the Abbotsford airport.

The beacon is located on a quiet residential street, nestled between well kept homes and towering fir trees.

'WC - 332' White Rock, BC

Antenna at 'WC - 332'

The antenna is an inverted 'L' end-fed Marconi about 65' in height with a flat top of about 200'. The downlead is barely visible in the above photo as it angles its way back to the transmitter shed. 

Heard regularly in California, 25 watt 'WC' is not as widely reported as is 'XX -344', especially from points east. As the system is similar to what a typical amateur LF installation might be, I would be very interested in any reception reports of 'WC' by DXers to the east. 'WC's upper sideband modulation frequency is ~ 423Hz so look for it on 332.423 kHz with your receiver in the CW mode. 



From CLE organizer Brian Keyte, G3SIA, comes the usual 'heads-up':


(Reminder: 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 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. 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!

CLE 216 NA Targets!

This coming weekend will see another CLE challenge. This time the hunting grounds will be:  320.0 - 334.9 kHz.






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 White Rock NDB, 'WC', on 332 kHz. The 'WC' NDB is located just a few hundred feet from the Canada - U.S. border, about 25 miles south east of the Vancouver International airport and about 20 miles west of the Abbotsford airport.

The beacon is located on a quiet residential street, nestled between well kept homes and towering fir trees.

'WC - 332' White Rock, BC

Antenna at 'WC - 332'

The antenna is an inverted 'L' end-fed Marconi about 65' in height with a flat top of about 200'. The downlead is barely visible in the above photo as it angles its way back to the transmitter shed. 

Heard regularly in California, 25 watt 'WC' is not as widely reported as is 'XX -344', especially from points east. As the system is similar to what a typical amateur LF installation might be, I would be very interested in any reception reports of 'WC' by DXers to the east. 'WC's upper sideband modulation frequency is ~ 423Hz so look for it on 332.423 kHz with your receiver in the CW mode. 



From CLE organizer Brian Keyte, G3SIA, comes the usual 'heads-up':


(Reminder: 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 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. 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!

CLE 216 NA Targets!

This coming weekend will see another CLE challenge. This time the hunting grounds will be:  320.0 - 334.9 kHz.






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 White Rock NDB, 'WC', on 332 kHz. The 'WC' NDB is located just a few hundred feet from the Canada - U.S. border, about 25 miles south east of the Vancouver International airport and about 20 miles west of the Abbotsford airport.

The beacon is located on a quiet residential street, nestled between well kept homes and towering fir trees.

'WC - 332' White Rock, BC

Antenna at 'WC - 332'

The antenna is an inverted 'L' end-fed Marconi about 65' in height with a flat top of about 200'. The downlead is barely visible in the above photo as it angles its way back to the transmitter shed. 

Heard regularly in California, 25 watt 'WC' is not as widely reported as is 'XX -344', especially from points east. As the system is similar to what a typical amateur LF installation might be, I would be very interested in any reception reports of 'WC' by DXers to the east. 'WC's upper sideband modulation frequency is ~ 423Hz so look for it on 332.423 kHz with your receiver in the CW mode. 



From CLE organizer Brian Keyte, G3SIA, comes the usual 'heads-up':


(Reminder: 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 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. 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!

As usual, the wonderful LF and MF conditions experienced during the week went into the dumper as the CLE weekend arrived.




Looking back, most of this can be blamed on our monthly (~28 days) repetitive schedule which nicely matches the rotation of the Sun. It seems that the same large coronal hole stream that whacked us during CLE 212, is the same one that showed up for CLE 213 right on schedule. Perhaps we need to shift our schedule by a week in case it wants to hang around for yet another rotation.

Conditions were not as bleak as I make them sound but they were a far cry from those enjoyed earlier in the week. The skip seemed fairly long on all three nights, but most signals were on the runty side, with only a few making strong appearances here on the left coast.

As shown below, conditions were quite 'flat' for the entire weekend and propagation did not vary much in quality other than favoring slightly different regions each night. Interestingly, 'YLH - 247' in Landsdowne House, Ontario, whose antenna was pictured on my last blog, was not heard at all on both Friday or Saturday but had a booming signal on Sunday night.

         Date 27 27 27 27 27 28 28 28 28 28 28 28 28 29
         UTC 0900 1200 1500 1800 2100 0000 0300 0600
         SFlx 81 81 81 81 83 83 83 83 83 83 83 83 85 85
         A-in 12 12 12 12 10 10 10 10 10 10 10 10 7 8
         K-in 3 3 2 1 2 2 2 2 2 1 2 3 2 3

My usual procedure with the Perseus SDR is to record the CLE segments of the band for two minutes, every hour and every half-hour, from shortly after sunset to local sunrise. It then requires several hours of carefully going through the recordings to see what CLE signals were recorded ... sometimes spending up to an hour on one frequency only, sorting out what was coming through.

I have also found that the classic blue-screen waterfall does not yield the best contrast for finding weak signals ... the 'photo-negative' screen shown above is far superior, with signals in black appearing on a white background.


26 02:00 240.0 BVS Burlington, WA, USA
26 03:00 241.0 YGT Igloolik, NU, CAN
27 03:00 242.0 ZT Port Hardy, BC, CAN
26 03:00 242.0 XC Cranbrook, BC, CAN
27 08:00 242.0 MMI Athens, TN, USA
26 07:30 242.0 EL El Paso, TX, USA
27 06:30 244.0 TH Thompson, MB, CAN
27 06:30 245.0 YZE Gore Bay, ON, CAN
28 15:00 245.0 HNS Haines, ALS
27 06:30 245.0 CRR Circle, MT, USA
27 06:00 245.0 CB Cambridge Bay, NU, CAN
27 09:30 245.0 AVQ Marana, AZ, USA
27 04:00 246.0 ZXJ Fort St. John, BC, CAN
27 09:00 247.0 YLH Lansdowne House, ON, CAN
27 08:00 248.0 ZZP Queen Charlotte Is, BC, CAN
27 08:00 248.0 QL Lethbridge, AB, CAN
27 08:00 248.0 QH Watson Lake, YT, CAN
27 07:30 248.0 PQF Mesquite, TX, USA
27 06:30 248.0 GLA Gulkana, ALS
27 08:00 248.0 FRT Fairmont, SC, USA
27 08:00 250.0 FO Flin Flon Municipal, MB, CAN
27 08:00 250.0 2J Grand Forks, BC, CAN
27 08:00 251.0 YCD Nanaimo, BC, CAN
27 15:00 251.0 OSE Bethel Apt, ALS
28 08:00 251.0 JZY Macomb, IL, USA
27 06:30 251.0 BR Brainerd, MN, USA
27 08:00 251.0 AM Amarillo, TX, USA
27 10:00 253.0 GB Marshall, MN, USA
27 08:00 254.0 ZYC Calgary, AB, CAN
27 08:00 254.0 SM Fort Smith, AB, CAN
27 04:00 254.0 EV Inuvik, NT, CAN
27 04:00 256.0 LSO Kelso, WA, USA
27 14:00 256.0 EB Edmonton, AB, CAN
27 14:00 257.0 XE Saskatoon, SK, CAN
27 05:00 257.0 SQT Melbourne, FL, USA
27 07:00 257.0 SAZ Staples, MN, USA
27 08:30 257.0 PEA Pella, IA, USA
27 07:00 257.0 MB Saginaw, MI, USA
27 14:00 257.0 LW Kelowna, BC, CAN
27 12:00 257.0 HCY Cowley, WY, USA
27 08:00 258.0 ZSJ Sandy Lake, ON, CAN
27 06:30 420.0 V7BE2 XOC, XUU
27 08:00 420.0 PK Olathe, KS, USA
27 08:00 420.0 FQ East Chain, MN, USA
27 04:00 421.0 VLY McKenney, TX, USA
27 08:30 422.0 EA Kearney, NE, USA
27 06:30 424.0 RVJ Reidsville, GA, USA
27 06:00 425.0 PFL Fort Sill, OK, USA
27 06:00 426.0 FTP Fort Payne, AL, USA
27 08:00 426.0 EN Council Bluffs, NE, USA
27 07:30 428.0 POH Pocahontas, IA, USA
27 07:00 432.0 IZN Lincolnton, NC, USA

The logging at 0630Z of 'V7BE2' is a large drill ship, the "Deepwater Thalassa", located near the center of the Gulf of Mexico.