Author Archive
July’s EME Window
With QSLs still arriving from previous 2m EME action, I was looking extra forward to late July's very short window.
When last month's activity was interrupted by my 140W brick amplifier catching fire, I was anxious to see if my repairs and homebrew RFC would still allow me to play on the moon. With July's best-positioned moonrises being too close to the sun (which was also rising at the same time), I was only able to spend a short time over two days before the moon travelled too far to the south and into my neighbour's trees.
Luckily I was rewarded with what seemed like very good lunar conditions, enabling me to easily work six different stations ... three of them being all-time new ones and boosting my EME initials total to 112.
I2FAK Franco / 16x19 el array
RK3FG Anatoly / 4x15 el array
G4SWX John / 4x16 el array
F4DJK Paul / 4x11 el array / #110
F5AQX Andre / 4x11 el array / #111
DL9DBJ Hartmut / 4x10 el array / #112
In addition, DL1VPL told me that he was able to copy me with his single 12el Yagi during the QSO with I2FAK! Needless to say, a contact between two single Yagi stations would be truly remarkable. I've only been able to copy a single Yagi station once over the years.
I was gratified to see that letting the smoke out of my little amplifier last month apparently caused no permanent damage and the repair seems to be holding up ... but I'll leave the bottom off for now just in case it gets any more crazy ideas.
When last month's activity was interrupted by my 140W brick amplifier catching fire, I was anxious to see if my repairs and homebrew RFC would still allow me to play on the moon. With July's best-positioned moonrises being too close to the sun (which was also rising at the same time), I was only able to spend a short time over two days before the moon travelled too far to the south and into my neighbour's trees.
Luckily I was rewarded with what seemed like very good lunar conditions, enabling me to easily work six different stations ... three of them being all-time new ones and boosting my EME initials total to 112.
I2FAK Franco / 16x19 el array
RK3FG Anatoly / 4x15 el array
G4SWX John / 4x16 el array
F4DJK Paul / 4x11 el array / #110
F5AQX Andre / 4x11 el array / #111
DL9DBJ Hartmut / 4x10 el array / #112
In addition, DL1VPL told me that he was able to copy me with his single 12el Yagi during the QSO with I2FAK! Needless to say, a contact between two single Yagi stations would be truly remarkable. I've only been able to copy a single Yagi station once over the years.
F4DJK's 4x11 el array |
F5AQX's 4x11 el array |
DJ9DBJ's 4x10 el array |
I was gratified to see that letting the smoke out of my little amplifier last month apparently caused no permanent damage and the repair seems to be holding up ... but I'll leave the bottom off for now just in case it gets any more crazy ideas.
July’s EME Window
With QSLs still arriving from previous 2m EME action, I was looking extra forward to late July's very short window.
When last month's activity was interrupted by my 140W brick amplifier catching fire, I was anxious to see if my repairs and homebrew RFC would still allow me to play on the moon. With July's best-positioned moonrises being too close to the sun (which was also rising at the same time), I was only able to spend a short time over two days before the moon travelled too far to the south and into my neighbour's trees.
Luckily I was rewarded with what seemed like very good lunar conditions, enabling me to easily work six different stations ... three of them being all-time new ones and boosting my EME initials total to 112.
I2FAK Franco / 16x19 el array
RK3FG Anatoly / 4x15 el array
G4SWX John / 4x16 el array
F4DJK Paul / 4x11 el array / #110
F5AQX Andre / 4x11 el array / #111
DL9DBJ Hartmut / 4x10 el array / #112
In addition, DL1VPL told me that he was able to copy me with his single 12el Yagi during the QSO with I2FAK! Needless to say, a contact between two single Yagi stations would be truly remarkable. I've only been able to copy a single Yagi station once over the years.
I was gratified to see that letting the smoke out of my little amplifier last month apparently caused no permanent damage and the repair seems to be holding up ... but I'll leave the bottom off for now just in case it gets any more crazy ideas.
When last month's activity was interrupted by my 140W brick amplifier catching fire, I was anxious to see if my repairs and homebrew RFC would still allow me to play on the moon. With July's best-positioned moonrises being too close to the sun (which was also rising at the same time), I was only able to spend a short time over two days before the moon travelled too far to the south and into my neighbour's trees.
Luckily I was rewarded with what seemed like very good lunar conditions, enabling me to easily work six different stations ... three of them being all-time new ones and boosting my EME initials total to 112.
I2FAK Franco / 16x19 el array
RK3FG Anatoly / 4x15 el array
G4SWX John / 4x16 el array
F4DJK Paul / 4x11 el array / #110
F5AQX Andre / 4x11 el array / #111
DL9DBJ Hartmut / 4x10 el array / #112
In addition, DL1VPL told me that he was able to copy me with his single 12el Yagi during the QSO with I2FAK! Needless to say, a contact between two single Yagi stations would be truly remarkable. I've only been able to copy a single Yagi station once over the years.
F4DJK's 4x11 el array |
F5AQX's 4x11 el array |
DJ9DBJ's 4x10 el array |
I was gratified to see that letting the smoke out of my little amplifier last month apparently caused no permanent damage and the repair seems to be holding up ... but I'll leave the bottom off for now just in case it gets any more crazy ideas.
Hunting For NDBs In CLE 221
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) |
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':
Hi all,
Please join us in our 221st coordinated Listening Event which starts
this Friday. All are very welcome.
Please join us in our 221st coordinated Listening Event which starts
this Friday. All are very welcome.
CLEs are not contests - if you enjoy taking part you will be a winner!
54 of us sent logs for CLE204 back in February 2016 when we
listened on these same frequencies.
It will certainly be tougher for most of us at this time of year.
Days: Friday 28 July - Monday 31 July
Times: Start and end at midday, your LOCAL TIME
Range: 370 - 384.9 kHz
Just log all the NDBs that you can identify with their nominal (listed)
frequencies in the range (it includes 370 kHz, but not 385 kHz)
plus any UNIDs that you come across there.
Please send your CLE log to the List in a plain text email if possible
(not in an attachment) with 'CLE221' at the start of its title.
Show on each log line:
# The date (e.g. 2017-07-29, etc., or just 29) and UTC.
(the date changes at 00:00 UTC)
# kHz (the nominal published frequency, if known)
# The Call Ident.
Show those main items FIRST - other optional details such as Location
and Distance go LATER in the same line.
If you send interim logs, please also send a 'Final' (complete) log.
As always, tell us your own location and brief details of the equipment
that you were using during the weekend.
I'll send the usual 'Any More Logs?' email at about 17:00 UTC on
Tuesday - you can check from it that your log has been found OK.
All logs must arrive on the list by 08:00 UTC on Wednesday 2nd
August at the very latest.
Joachim has again offered to make the combined results which he
Range: 370 - 384.9 kHz
Just log all the NDBs that you can identify with their nominal (listed)
frequencies in the range (it includes 370 kHz, but not 385 kHz)
plus any UNIDs that you come across there.
Please send your CLE log to the List in a plain text email if possible
(not in an attachment) with 'CLE221' at the start of its title.
Show on each log line:
# The date (e.g. 2017-07-29, etc., or just 29) and UTC.
(the date changes at 00:00 UTC)
# kHz (the nominal published frequency, if known)
# The Call Ident.
Show those main items FIRST - other optional details such as Location
and Distance go LATER in the same line.
If you send interim logs, please also send a 'Final' (complete) log.
As always, tell us your own location and brief details of the equipment
that you were using during the weekend.
I'll send the usual 'Any More Logs?' email at about 17:00 UTC on
Tuesday - you can check from it that your log has been found OK.
All logs must arrive on the list by 08:00 UTC on Wednesday 2nd
August at the very latest.
Joachim has again offered to make the combined results which he
hopes to complete on that day.
To help your listening, seeklists and maps for your part of the World
To help your listening, seeklists and maps for your part of the World
are available via the CLE page http://www.ndblist.info/cle.htm
Good listening - enjoy the CLE
Brian
----------------------------------------------------------
From: Brian Keyte G3SIA ndbcle'at'gmail.com
Location: Surrey, SE England (CLE coordinator)
----------------------------------------------------------
Good listening - enjoy the CLE
Brian
----------------------------------------------------------
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 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!
Hunting For NDBs In CLE 221
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) |
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':
Hi all,
Please join us in our 221st coordinated Listening Event which starts
this Friday. All are very welcome.
Please join us in our 221st coordinated Listening Event which starts
this Friday. All are very welcome.
CLEs are not contests - if you enjoy taking part you will be a winner!
54 of us sent logs for CLE204 back in February 2016 when we
listened on these same frequencies.
It will certainly be tougher for most of us at this time of year.
Days: Friday 28 July - Monday 31 July
Times: Start and end at midday, your LOCAL TIME
Range: 370 - 384.9 kHz
Just log all the NDBs that you can identify with their nominal (listed)
frequencies in the range (it includes 370 kHz, but not 385 kHz)
plus any UNIDs that you come across there.
Please send your CLE log to the List in a plain text email if possible
(not in an attachment) with 'CLE221' at the start of its title.
Show on each log line:
# The date (e.g. 2017-07-29, etc., or just 29) and UTC.
(the date changes at 00:00 UTC)
# kHz (the nominal published frequency, if known)
# The Call Ident.
Show those main items FIRST - other optional details such as Location
and Distance go LATER in the same line.
If you send interim logs, please also send a 'Final' (complete) log.
As always, tell us your own location and brief details of the equipment
that you were using during the weekend.
I'll send the usual 'Any More Logs?' email at about 17:00 UTC on
Tuesday - you can check from it that your log has been found OK.
All logs must arrive on the list by 08:00 UTC on Wednesday 2nd
August at the very latest.
Joachim has again offered to make the combined results which he
Range: 370 - 384.9 kHz
Just log all the NDBs that you can identify with their nominal (listed)
frequencies in the range (it includes 370 kHz, but not 385 kHz)
plus any UNIDs that you come across there.
Please send your CLE log to the List in a plain text email if possible
(not in an attachment) with 'CLE221' at the start of its title.
Show on each log line:
# The date (e.g. 2017-07-29, etc., or just 29) and UTC.
(the date changes at 00:00 UTC)
# kHz (the nominal published frequency, if known)
# The Call Ident.
Show those main items FIRST - other optional details such as Location
and Distance go LATER in the same line.
If you send interim logs, please also send a 'Final' (complete) log.
As always, tell us your own location and brief details of the equipment
that you were using during the weekend.
I'll send the usual 'Any More Logs?' email at about 17:00 UTC on
Tuesday - you can check from it that your log has been found OK.
All logs must arrive on the list by 08:00 UTC on Wednesday 2nd
August at the very latest.
Joachim has again offered to make the combined results which he
hopes to complete on that day.
To help your listening, seeklists and maps for your part of the World
To help your listening, seeklists and maps for your part of the World
are available via the CLE page http://www.ndblist.info/cle.htm
Good listening - enjoy the CLE
Brian
----------------------------------------------------------
From: Brian Keyte G3SIA ndbcle'at'gmail.com
Location: Surrey, SE England (CLE coordinator)
----------------------------------------------------------
Good listening - enjoy the CLE
Brian
----------------------------------------------------------
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 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!
Canada Post / QSLs / Magicband Transformations
Several weeks ago I mused about my interest in earth-mode VLF experiments, following the inspirational exploits of G3XBM in his earth-mode work a few years ago.
His low powered system utilizing a 5W audio IC and simple circuitry produced surprisingly interesting results over several kilometers.
With possible future experimenting in mind, I found a nice low-powered IC audio amplifier kit from China on e-Bay, capable of producing about 18W at 12V ... more with higher voltage and proper heat-sinking.
Whenever buying from China, I look for a dealer with the highest feedback rating and always compare their complaints versus the number of orders shipped. There always seems to be a few that are 99.9 - 100%, which, for me, has always assured that they are probably not selling junk. Anything lower than 98% can often be a red flag.
The kit was just $1.50 and with free-shipping, what's to lose?
A few weeks after I had placed my order, the nightly TV news had a spot regarding the problem that these "free shipping" packets were creating for Canada Post and their customers. It seems that in the past few months, as more and more "free" shipments were arriving from the far east, Canada Post had not been able to keep up with the processing. The news spot showed row upon row of shipping containers parked at the back of Vancouver International's (YVR) postal processing plant, with all of them filled with thousands of small "free" packets waiting to be processed!
It seems that each packet needs to be scanned by the border security folks (CBSA) for illegal material before it can be processed by Canada Post and the back-up was building at a tremendous rate. There appears to be little if any profit for Canada Post with these smaller untracked packages and they are given the lowest priority-rating possible.
In order to speed up the process, both CBSA and Canada Post facilities would need to expand their operational capabilities at the airport and I suspect there is no serious will to do this until pressured politically by angry customers.
All parcels from China that are mailed to Canada stop at Vancouver's YVR before going further. The mammoth recent increase in online "free-shipping", in spite of the normally estimated 3-4 week delivery time, has proven too attractive for customers and our domestic system has failed to meet the new load demands.
With this new information in mind, my e-Bay purchase would prove to be an interesting test of the system and of the TV news spot's accuracy. Normally, I would have expected my tiny parcel to arrive in about 30 days, but mine would be one that eventually ended up in the airport parking lot.
The kit finally arrived this week, with a delivery time of 89 days! Many online sellers will offer an inexpensive option to pay for faster shipping, something that will still take a couple of weeks but much better than three months. If you are given this inexpensive shipping option I would highly recommend that you choose it, and if not, ask for an alternative to "free shipping". Unless something changes soon, delays will continue to increase.
I also wonder, and perhaps you can comment below, are U.S. customers seeing the same long delays as we here in Canada are experiencing when the "free shipping" option is chosen?
QSLs in my mailbox always excite me ... especially like yesterday's, arriving in a thin light-brown envelope decorated with colorful stamps.
I'm 100% certain this is because of receiving similar-appearing envelopes containing QSL cards during my formative years from age eleven onward and how much enjoyment the cards from shortwave stations all over the world brought me at this young age. For me, there is no replacement for a paper QSL, but sadly, this long-standing tradition is slowly slipping away due to the high cost of mailing even a normal-size envelope.
Earlier this summer I had a nice run of JA's on 6m Es but this time, instead of CW, they were on JT65A. Yesterday's card was for one of the digital contacts.
Signals were weak, at -23 db ... far too weak to be heard on CW but easily readable during the 60 second deep-listen period mandated by the JT65A mode. With so many stations now listening higher in the band for JT-mode signals, there has been very little activity on CW and now, with the introduction of yet another new digital mode, FT8, even the digital activity is split into sections, with neither mode being compatible.
I have held off installing the newer WSJT-X version containing the FT8 fifteen-second transmission mode until all of the bugs are ironed out ... the software will likely be tweaked a few more times yet before it reaches the polished final version we see for JT65 and others.
FT8 has been designed for weaker 6m Es openings that are often too short in duration for the longer time periods needed by JT65's sixty-second sequences. FT8 contacts can be completed quickly, before short-lived signals can drop out, but the shorter sequences come at the cost of reduced sensitivity ... probably a worthwhile tradeoff.
Conventional mode activity on 6m has suffered tremendously with the introduction of these new modes and it seems that if you want to work weak signal DX (and not all do), sadly it may be digital or nothing at all if the trends continue.
If all of the DX moves from CW to digital, for me, much of the magic will disappear as well. Letting the computer do all of the thinking is not nearly as satisfying or enjoyable as using my brain and CW skills to put a new rare one in the log. Six meters continues to evolve and I'm not overly excited by the direction it seems to be going.
Canada Post / QSLs / Magicband Transformations
Several weeks ago I mused about my interest in earth-mode VLF experiments, following the inspirational exploits of G3XBM in his earth-mode work a few years ago.
His low powered system utilizing a 5W audio IC and simple circuitry produced surprisingly interesting results over several kilometers.
With possible future experimenting in mind, I found a nice low-powered IC audio amplifier kit from China on e-Bay, capable of producing about 18W at 12V ... more with higher voltage and proper heat-sinking.
Whenever buying from China, I look for a dealer with the highest feedback rating and always compare their complaints versus the number of orders shipped. There always seems to be a few that are 99.9 - 100%, which, for me, has always assured that they are probably not selling junk. Anything lower than 98% can often be a red flag.
The kit was just $1.50 and with free-shipping, what's to lose?
A few weeks after I had placed my order, the nightly TV news had a spot regarding the problem that these "free shipping" packets were creating for Canada Post and their customers. It seems that in the past few months, as more and more "free" shipments were arriving from the far east, Canada Post had not been able to keep up with the processing. The news spot showed row upon row of shipping containers parked at the back of Vancouver International's (YVR) postal processing plant, with all of them filled with thousands of small "free" packets waiting to be processed!
It seems that each packet needs to be scanned by the border security folks (CBSA) for illegal material before it can be processed by Canada Post and the back-up was building at a tremendous rate. There appears to be little if any profit for Canada Post with these smaller untracked packages and they are given the lowest priority-rating possible.
In order to speed up the process, both CBSA and Canada Post facilities would need to expand their operational capabilities at the airport and I suspect there is no serious will to do this until pressured politically by angry customers.
All parcels from China that are mailed to Canada stop at Vancouver's YVR before going further. The mammoth recent increase in online "free-shipping", in spite of the normally estimated 3-4 week delivery time, has proven too attractive for customers and our domestic system has failed to meet the new load demands.
With this new information in mind, my e-Bay purchase would prove to be an interesting test of the system and of the TV news spot's accuracy. Normally, I would have expected my tiny parcel to arrive in about 30 days, but mine would be one that eventually ended up in the airport parking lot.
The kit finally arrived this week, with a delivery time of 89 days! Many online sellers will offer an inexpensive option to pay for faster shipping, something that will still take a couple of weeks but much better than three months. If you are given this inexpensive shipping option I would highly recommend that you choose it, and if not, ask for an alternative to "free shipping". Unless something changes soon, delays will continue to increase.
I also wonder, and perhaps you can comment below, are U.S. customers seeing the same long delays as we here in Canada are experiencing when the "free shipping" option is chosen?
QSLs in my mailbox always excite me ... especially like yesterday's, arriving in a thin light-brown envelope decorated with colorful stamps.
I'm 100% certain this is because of receiving similar-appearing envelopes containing QSL cards during my formative years from age eleven onward and how much enjoyment the cards from shortwave stations all over the world brought me at this young age. For me, there is no replacement for a paper QSL, but sadly, this long-standing tradition is slowly slipping away due to the high cost of mailing even a normal-size envelope.
Earlier this summer I had a nice run of JA's on 6m Es but this time, instead of CW, they were on JT65A. Yesterday's card was for one of the digital contacts.
Signals were weak, at -23 db ... far too weak to be heard on CW but easily readable during the 60 second deep-listen period mandated by the JT65A mode. With so many stations now listening higher in the band for JT-mode signals, there has been very little activity on CW and now, with the introduction of yet another new digital mode, FT8, even the digital activity is split into sections, with neither mode being compatible.
I have held off installing the newer WSJT-X version containing the FT8 fifteen-second transmission mode until all of the bugs are ironed out ... the software will likely be tweaked a few more times yet before it reaches the polished final version we see for JT65 and others.
FT8 has been designed for weaker 6m Es openings that are often too short in duration for the longer time periods needed by JT65's sixty-second sequences. FT8 contacts can be completed quickly, before short-lived signals can drop out, but the shorter sequences come at the cost of reduced sensitivity ... probably a worthwhile tradeoff.
Conventional mode activity on 6m has suffered tremendously with the introduction of these new modes and it seems that if you want to work weak signal DX (and not all do), sadly it may be digital or nothing at all if the trends continue.
If all of the DX moves from CW to digital, for me, much of the magic will disappear as well. Letting the computer do all of the thinking is not nearly as satisfying or enjoyable as using my brain and CW skills to put a new rare one in the log. Six meters continues to evolve and I'm not overly excited by the direction it seems to be going.
WWV’s New Antenna On 25MHz – QSA?
New Turnstile Antenna / WWV - 25MHz |
Last week's ARRL announcement regarding WWV's new circular polarized Turnstile antenna tests on their 25MHz transmitter quickly garnered my interest.
Their 25MHz signal used to be heard world-wide on F2 until it was dropped in 1977, but somewhat surprisingly, was resurrected in 2014.
I recall hearing its 2nd harmonic on sporadic-E very routinely on 50.000MHz when I first became active on 6m back in the late 60's. Back then it was also not uncommon to hear the 3rd and 4th harmonics of ship CW stations operating on 12 and 16MHz, at the very low end of 6m and just below the band edge on 49MHz.
6m Prop Indicator From The 70's! |
Having not listened for WWV's 25MHz signal for several decades, I set up yesterday to see if it could be heard here in mid-summer. Using my Perseus SDR and my LF/MF inverted-L, self-resonant in the middle of the broadcast-band (gosh knows what the pattern looks like up on 25MHz!), I started monitoring just after lunch. I could detect their carrier which was very weak but steady, probably arriving on ionospheric scatter via the e-layer.
A few hours later I re-checked after hearing a few Colorado signals on 6m Es and sure enough, there they were with a fairly robust signal. It too, was no doubt arriving via sporadic-E as it was again today during another widespread Es opening from the PNW to as far south as Puerto Rico.
Here is a recording of the 25MHz signal made this morning with my Perseus SDR along with a comparison recording of their 20MHz signal, made about 30 seconds later.
There is not a lot of difference between the two and both run similar powers ... 2.5kW on 20MHz and 2kW on 25MHz. The 20MHz system uses a half-wave vertical on a 7.5m tower while the 25MHz outlet uses the crossed-dipole circular polarized Turnstile shown at the top of the blog.
Reception reports of their 25MHz signal are being sought and can be e-mailed to WWV at this address.