Posts Tagged ‘Propagation’

630m VK’s Light-Up North America


It seems that all of my blogspots of late have focused on 630m propagation ... but what has been happening down there recently has been both amazing and somewhat unexpected. With the growing number of active stations listening and transmitting, the band's propagation capabilities and mysteries are quickly revealing themselves.

Last night was a great example but perhaps the WSPRnet prop map illustrates this best.

courtesy: http://wsprnet.org/drupal/wsprnet/map
The amount of North American activity grows each day, especially now that the DX season has arrived. At one point last night, KB5NJD reports over 100 stations either transmitting or reporting via the WSPRnet activity page! With thunderstorm activity gradually shrinking, reception should only get better over the next few months.

Particularly striking was the long haul propagation from VK to North America, with northernmost VK4YB leading the pack. His 90 watt signal made it all the way to VE3IQB, near Ottawa as well as to NO3M, in Pennsylvania! To provide further hope to those that have little room for big receiving antennas, VE3IQB uses a typical small active e-probe antenna, 20' above ground!

courtesy: http://wsprnet.org/drupal/wsprnet/map
This spotlight propagation to the select regions of the east coast is further mystified by the level of geomagnetic activity overnight, with the K index reaching level 5 and higher!

courtesy: http://www.swpc.noaa.gov/
Interestingly, all of this was right over my head, with not a single peep heard here from Roger. Stations across Georgia Strait, VE7BDQ, VE7CNF and VA7MM all reported hearing Roger as well as being heard by him. For the latter two, yesterday and today represent their initial decodes to down under.

I'm theorizing that Roger's signal was arriving today at much lower angles than normal, evidenced by its far-reaching east coast reception and the fact that it couldn't get over my 600' local obstruction to the west. I've always believed that it takes higher angled signal arrival for me to hear Roger and today's events seem to support this.

Exactly what would cause this to be the case, I'll leave to the experts but I imagine that the sudden surge in geomagnetic activity played a significant role in today's very different propagation paths.

Roger was not the only VK lighting-up the map today. A much more detailed account of all the action can be found on the KB5NJD's daily 630m report here ... all very inspirational and hopefully enough to spur even more new activity on the MF band.

Why not give a listen and see what you can hear?

CLE 211 Results




This past weekend's CLE saw noticeably improved conditions compared with the previous event.





With the fall DX season fast-approaching, the combination of diminishing thunderstorm activity and improved propagation provided some interesting catches. Friday night was the best with Saturday having a brief period of favorable prop, while no new stations were heard on Sunday night, the poorest.

It was particularly nice to hear strong signals from the eastern provinces on Friday, highlighted with an excellent signal from 'JT' (390 kHz) in Stephenville, Newfoundland. This long haul east-west propagation can only be found with quite geomagnetic conditions as was the case on Friday.


After examining the geomagnetic 'K' data for Saturday (25th), it's interesting to note that the four catches for that night all coincided exactly with the brief green bar (K= 0-3) centered on the hours around 0900 UTC (circled).

The following NDBs were heard using my Perseus SDR and 'inverted-L' resonated to ~ 300kHz:

               24 06:30 385.0 WL Williams Lake, BC, CAN
               24 13:00 385.0 OCC Yakutat, ALS
               24 10:00 385.0 MR Pacific Grove, CA, USA
               24 13:00 385.0 EHM Cape Newenham, ALS
               24 08:30 386.0 SYF St. Francis, KS, USA
               24 06:30 386.0 HAU Helena, MT, USA
               24 06:00 386.0 4N Oxford House, MB, CAN
               24 06:30 388.0 MM Fort Mc Murray, AB, CAN
               24 09:30 388.0 JW Pigeon, AB, CAN
               24 06:30 388.0 GLY Clinton, MO, USA
               24 06:30 389.0 YWB Kelowna, BC, CAN
               24 08:00 389.0 TW Twin Falls, ID, USA
               25 08:30 389.0 EN Kenosha, WI, USA
               24 06:00 389.0 CSB Cambridge, NE,USA
               24 06:30 390.0 JT Stephenville, NL, CAN
               24 06:00 390.0 HBT Sand Point, ALS
               24 06:00 390.0 AES Northway, ALS
               24 06:30 391.0 TK Telkwa, BC, CAN
               24 13:00 391.0 EEF Sisters Island, ALS
               24 06:00 391.0 DDP Dorado, PTR
               24 06:30 391.0 4W Kelsey, MB, CAN
               24 08:30 392.0 ZFN Tulita, NT, CAN
               24 06:00 392.0 PNA Wenz, WY, USA
               24 06:30 392.0 ML Charlevoix, QC, CAN
               25 08:30 392.0 FMZ Fairmont, NE, USA
               25 08:30 392.0 BAJ Sterling, CO, USA
               24 06:00 392.0 AGZ Wagner, SD, USA
               25 09:30 393.0 TOG Togiak, ALS
               24 08:30 393.0 2M Opapimiskan Lake,ON, CAN
               24 13:00 394.0 RWO Kodiak, ALS
               24 08:30 394.0 DQ Dawson Creek, BC, CAN
               24 08:30 395.0 YL Lynn Lake, MB, CAN
               24 06:00 395.0 ULS Ulysses, KS, USA
               24 08:30 395.0 L7 Estevan, SK, CAN
               24 08:30 396.0 YPH Inukjuak, QC, CAN
               24 13:00 396.0 CMJ Ketchikan, ALS
               24 08:30 397.0 ZSS Saskatoon, SK, CAN
               24 08:00 397.0 SB San Bernardino, CA, USA
               24 08:00 397.0 CIR Cairo, IL, USA
               24 08:30 398.0 YOD Cold Lake, AB, CAN
               24 08:30 398.0 3D Cumberland House, SK, CAN
               24 08:30 399.0 ZHD Dryden, ON, CAN
               24 13:00 399.0 SRI St George, ALS

The results from all participants can be found at the NDB List website, or if you are a member of the ndblist Group, results have also been 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 helpful information available there and new members are always very welcome. As well, you can follow and chat with other NDB chasers regarding antennas, techniques, unidentified signals and  nightly propagation.

630m And Recent Geomagnetic Activity




High levels of geomagnetic activity have usually, but not always, been the kiss-off-death for LF/MF propagation.

These past few months have seen fairly regular field disturbances, often pushing the K index to a level '5' or higher. However, while usually attenuating the east-west and northerly polar paths, the Trans-Pacific path often seems to benefit from these events ... particularly last night.


Perhaps it is related to the equinox's normal preference for this path or maybe the goop the sun is sending us at this point in the cycle is different or not as energetic as it is at mid-cycle. Nevertheless it's really encouraging to see that not all disturbances are detrimental to LF propagation.

For a daily summary of all overnight activity and much more, see KB5NJD's '630m Daily Reports'.

The WSPRnet map reproduced below shows the extent of reception during my own overnight WSPR 630m beaconing session. Missing are many of the normal spots from the eastern provinces and east coast states, indicating the attenuation on this path. Everything else seems enhanced.

courtesy: WSPRnet

The path to down under, in-spite of my obstruction in that direction, perked-up as well, with VK4YB decoded here 19 times as well as VK3ELV's 150W and inverted-L near Wangaratta, Victoria.


               13:56      VK4YB      0.4756      -28   QG62ku   11820      
               13:50      VK4YB      0.4756      -28   QG62ku   11820      
               13:44      VK4YB      0.4756      -24   QG62ku   11820      
               13:40      VK4YB      0.4756      -24   QG62ku   11820    
               13:30      VK4YB      0.4756      -27   QG62ku   11820      
               13:24      VK4YB      0.4756      -20   QG62ku   11820      
               13:18      VK4YB      0.4756      -24   QG62ku   11820    
               13:12      VK4YB      0.4756      -22   QG62ku   11820    
               12:42      VK4YB      0.4756      -26   QG62ku   11820    
               12:14      VK4YB      0.4756      -20   QG62ku   11820    
               12:02      VK4YB      0.4756      -23   QG62ku   11820    
               11:58      VK4YB      0.4756      -25   QG62ku   11820    
               11:52      VK4YB      0.4756      -25   QG62ku   11820    
               11:40      VK4YB      0.4756      -29   QG62ku   11820      
               11:32      VK4YB      0.4756      -26   QG62ku   11820    
               11:24      VK4YB      0.4756      -25   QG62ku   11820    
               11:12      VK4YB      0.4756      -22   QG62ku   11820    
               10:56      VK4YB      0.4756      -26   QG62ku   11820    
               10:54      VK4YB      0.4756      -25   QG62ku   11820



Merv, WH2XCR in Hawaii, was spotted here 56 times, with numerous transmissions at 'easy CW' levels. He even spotted me twice, with his 80m dipole, presently laying on the ground!

It was also encouraging to see 21 spots from Eden, ZF1EJ in the Cayman Islands, with several at CW levels.

The following stations all uploaded spots of my overnight WSPR signals, as nightly activity continues to grow with the DX season now at the doorstep. Given equal ERP, most of these stations would be workable on either CW or on JT9.

              WH2XGP      DN07dg      319      122
               WG2XSV      CN85sr      353      169
               WI2XJQ        CN87ts      138      150
               NO1D         DM34tn      1825      147
               N3IZN/RX  DM13ji      1796      161
               WW6D      CM88pl      1155      177
               VE7CNF      CN89ng      55      33
               VA7MM      CN89og      59      38
               WE2XPQ      BP51ip      2151      321
               W5EMC      EM10cl      2963      124
               K5ACL      EM10bd      2987      125
               WG2XXM    EM15lj      2610      115
               ZF1EJ/1       EK99ig      4977      116
               KE7LGT      DN26xm      739      107
               W3PM       EM64or      3365      104
               ZF1EJ        EK99ig      4977      116
               VE7KPB      DN29cm      550      79
               KU7Z        DN41af      1227      129
               WH2XCR      BL11je      4295      236
               KB0BRY      EN17nc      1966      86
               WD2XSH/20 CN83      598      178
               WG2XIQ      EM12      2841      120
               WE4X      EM65ut      3326      102
               VE7BDQ      CN89la      26      44
               KB7W      CN93jx      565      163
               W6LEO      DN17oq      498      103
               WH2XAR      DM33vp      1924      147


As interest in 630m continues to expand, many U.S. amateurs are already building their stations so they will be ready to go when the word finally comes. I suspect that 630m may soon sound like a small slice of 40m on a busy night ... will you be ready?

Magicband Morphs

I have been having fun on 6m every summer since the late 60's. Without doubt, this summer's Sporadic-E (Es) season is the worst one I have experienced in terms of domestic (North America) openings. This summer was almost a carbon-copy of last year's summer Es season. As I mentioned in an earlier blog, unless this is some form of short term or cyclical anomaly, the fundamental nature of Sporadic-E openings appears to be undergoing some type of change. Missing-in-action were the numerous day-long intense openings to California as well as the grand openings to the eastern states (FN grids) and Canada ... all guaranteed openings every summer. These openings would often last well into the late night hours and even overnight, picking up the next day where they left off. This is the second summer in a row where no Es MUF's into the 2m band were experienced, with this year having seen nothing even as high as the 88-108MHz FM band. Maybe I missed them if they occurred, but I don't think so. In terms of non-domestic openings, the band continues to evolve, as it seems that a higher percentage of hours with very long skip continues to rise. As poor as this year has been domestically, CW contacts were completed with Germany, Ireland, England, Japan, France, Canary Islands, Balearic Island, Venezuela, Cuba, Puerto Rico, and the Cayman Islands. A short and exceptionally rare opening to Africa, allowed an 'almost QSO' with CN8KD in Morocco, as he had one letter of my call incorrect when he quickly faded away ... pretty exciting even for a 'busted' QSO on 6m, in the middle of summer. Whether this very long propagation is just multi-hop traditional Es or something entirely different is still up for debate, as often there are no indicators (beacons or other mid-point signals) indicating that the band is even open. Many, including myself, believe this is some form of chordal hop or interlayer ducting, involving the E-layer alone or perhaps even the bottom of the F layer. Signals strengths can reach 599 levels and almost without fail, have extremely small footprints, with stations just a few miles away hearing nothing at all.
Chordal Hop courtesy: http://g4fkh.co.uk/projects/lp-experiment/
Inter Layer Ducting courtesy: http://g4fkh.co.uk/projects/lp-experiment/
When these openings occur between western North America and Europe, they can be very exciting, as the footprint on the European end often sprays around like a stray garden hose, popping up in a different country with each passing minute. Openings are often fast and furious and always heart-pounding! Perhaps there is still some magic yet to occur but the 'normal' season (or what used to be normal) is drawing to a close as August nears. The fat-lady is warming up her voice behind the curtain and will soon be singing once again. But something else is changing on 6m besides the propagation and that is the huge growth of the JT65 weak signal digital mode. As the season draws slowly down, I still see long-time dedicated CW operators going up the band to dip their toes for the first time on this alternate mode. I have used it fairly often to work stations when the CW / SSB end of the band appears to be dead. The maps shown below, grabbed just four days ago, illustrate what I have been seeing. The amount of JT65 activity is striking, compared to the traditional CW/SSB modes, both shown for the same one hour period. I could assume that the several extra db of weak-signal sensitivity is the reason for the disparity seen from one mode to the other but there may be other factors coming into play.
courtesy: http://www.dxmaps.com/
courtesy: https://pskreporter.info/pskmap.html
Once the band really opens however, the weak-signal sensitivity of JT65 soon looses its previous advantage and the JT65 segment of the band can get pretty clobbered, with numerous signals on top of each other, all competing for their ~200Hz slice of the spectrum. As well, a JT65 QSO is slow ... a minimum of four minutes. Taking four minutes to exchange calls, reports and 'rogers' on a wide open band with strong signals, makes little sense. Perhaps the majority of 6m JT65 operators are new amateurs with a codeless licence or are operating in antenna-restricted communities. Whatever the reason, the numbers are growing and traditional operating patterns are changing. Who knows what next summer will bring!

April’s Single-Yagi EME

With several QSL's from last month's EME action now arriving, April's 'best days' have just concluded. For me, operating with no antenna elevation, 'best days' mean those with northern-most lunar declinations (these put the moon rising clearly and almost directly out in front of the house, not in the neighbour's trees); not having the moon near the sun and also, having the moon closer to perigee (closest approach to earth) rather than apogee (furthest from earth). With just a single 9 element yagi, every db is precious.

A website that helps determine when these good days occur, is the Making More Miles On VHF eme page. A graphical display of several important elements will easily determine which days might be best to operate ...

courtesy: http://www.mmmonvhf.de/eme.php
... but I have also found success on days that don't look particularly great, with the moon approaching apogee and it's subsequent higher db path loss. As with most radio propagation, there is also some magic involved and, just like on any band, some days are simply 'better' and for no obvious reason.

This month saw six EME contacts, some with stations worked previously, in 2007, and not 'new uniques', while three were new, bringing my uniques total to 73, with this small, horizon-gain assisted system.

G4SXW John 4 x 16el array #71 ... answered my CQ
KB8RQ Gary 24 X 13el array!! worked with moon at 1 deg high
UX5UL Oleg 4 x 16el array #72
UT6UG Val 4 x 32el array #73 Val and Oleg both live in Kyiv, Ukraine
RK3FG Anatoly 4 X 15el array
K9MRI Joe 8 X 28el array - Indiana



G4SWX  4 x 16 el EME Array
KB8RQ 24 x 13 el EME Array

As summer approaches, it will be interesting to see how favorable the above mentioned variables will come into play as many of the best northerly declination days will also closely follow the sun and its increased background skynoise ... not so much a problem for me but for those bigger stations trying to hear a very weak signal in a noisier sky.

Thirty Minutes of Dazzle: The Sun in UHD 4K by SDO (NASA)

Take a front-seat view of the Sun in this 30-minute ultra-high definition movie in which NASA SDO gives us a stunning look at our nearest star.

This movie provides a 30-minute window to the Sun as seen by NASA’s Solar Dynamics Observatory (SDO), which measures the irradiance of the Sun that produces the ionosphere. SDO also measures the sources of that radiation and how they evolve.

SDO’s Atmospheric Imaging Assembly (AIA) captures a shot of the sun every 12 seconds in 10 different wavelengths. The images shown here are based on a wavelength of 171 angstroms, which is in the extreme ultraviolet range and shows solar material at around 600,000 Kelvin (about 1 million degrees F.) In this wavelength it is easy to see the sun’s 25-day rotation.

The distance between the SDO spacecraft and the sun varies over time. The image is, however, remarkably consistent and stable despite the fact that SDO orbits Earth at 6,876 mph and the Earth orbits the sun at 67,062 miles per hour.

Scientists study these images to better understand the complex electromagnetic system causing the constant movement on the sun, which can ultimately have an effect closer to Earth, too: Flares and another type of solar explosion called coronal mass ejections can sometimes disrupt technology in space. Moreover, studying our closest star is one way of learning about other stars in the galaxy. NASA’s Goddard Space Flight Center in Greenbelt, Maryland. built, operates, and manages the SDO spacecraft for NASA’s Science Mission Directorate in Washington, D.C.

Charged particles are created in our atmosphere by the intense X-rays produced by a solar flare. The solar wind, a continuous stream of plasma (charged particles), leaves the Sun and fills the solar system with charged particles and magnetic field. There are times when the Sun also releases billions of tons of plasma in what are called coronal mass ejections. When these enormous clouds of material or bright flashes of X-rays hit the Earth they change the upper atmosphere. It is changes like these that make space weather interesting.

Sit back and enjoy this half-hour 4k video of our Star!  Then, share.  🙂

73 dit dit

 

Never heard Heard

I saw on Facebook this morning, that many were thanking the VK0EK expedition for the ATNO and were thanking them, in general, for a wonderful DXpedition. I would suspect they have gone QRT.

And I would guess I'm in the minority as I'm not in any of their logs.  In fact, I never even heard them decently well enough to work them.  There were a couple of times that I could tell they were on a given frequency, but they never loud enough that I would be able to hear my own call come back to me, on the off-chance that they would have heard me.  It didn't seem right to just add to the QRM.

Am I disappointed?  You're darn tootin' I am!  Working VK0EK would have been an ATNO for me and I sure as heck would love to have them in my DXCC tally.  But I'm not depressed about it.

It all goes back to that post a few weeks ago about balance.  Yes, I do not have Heard Island as an entity worked. However, the sun is still shining, the birds are still chirping, our solar system is still plowing its way throughout the galaxy.  I still have to go to work tomorrow and earn a living.

And while I didn't work them, and life goes on, I still applaud their effort.  It's not easy to go to a remote island near Antarctica, and brave the elements and hardships to provide the rest of us Amateur Radio ops with a bunch of excitement and fun.

Thank you Team VK0EK - even though I'm not in your log - thank you for a job very well done, indeed!

72 de Larry W2LJ
QRP - When you care to send the very least!

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