📊 GCARC Monthly Station Performance — September 2026
About This Report
This report ranks every active WSPR transmitter in grid square FM29 against the GCARC member network on station-performance metrics. GCARC stations are highlighted in gold rows. Bands are reported separately — propagation behaviour and antenna requirements differ enough between bands that cross-band averages would mislead. All values are computed from the full month of wspr.live spot data, filtered to stations with ≥ 500 spots per band to keep small-sample stations from distorting the rankings.
Station Activity — August 2026 → September 2026
Which FM29 stations changed their activity between the two months. New arrivals, stations that went quiet, meaningful expansions in reach or band coverage, and contractions worth investigating. GCARC members are marked with ★ and also tracked individually in the focus table at the bottom regardless of change size.
September 2026 marked a significant contraction for the FM29 WSPR group, driven primarily by the loss of several high-volume contributors rather than a lack of new activity. While there were fresh arrivals, their combined output could not offset the substantial drop in spots from previously active stations. The net effect was a quieter landscape overall, with the center of gravity shifting away from the heavy hitters who dominated the previous month’s statistics.
Among the new entrants, KB2MMI stands out as a robust addition, immediately establishing a wide footprint across seven bands with impressive propagation distances. KE2DST also joined the fold, contributing steady traffic on 30 meters, while N3WVW appeared with a smaller but notable reach. These additions provide a solid foundation for future growth, though they currently lack the sheer volume needed to balance the ledger against the stations that went dark.
The most concerning trend is the disappearance of high-activity stations, particularly among GCARC members. N2LQH and KC2GYU, both previously producing substantial spot counts across multiple HF bands, fell silent entirely, which is a significant loss for the group’s visibility. W2MMD and W2LJR also saw drastic reductions or total cessation of activity. These abrupt stops warrant direct follow-up with the operators to determine if the cause is equipment failure, antenna issues, or simple off-air time, as the sudden loss of such consistent signals is unusual.
Within the GCARC membership, the changes were mixed but largely negative. KS2D continued to expand its already impressive multi-band presence, showing healthy growth in both spot count and range. KD2EIB and KE2DST both increased their activity levels, with KE2DST’s debut on 30 meters being a welcome addition. Conversely, K2ZA lost 15-meter activity despite maintaining a high spot count on other bands, suggesting a potential issue with the antenna or feedline for that specific frequency. KE2AQZ saw a noticeable decline in spots while holding the same band mix, which often points to transmitter power or timing adjustments. W2TDS made a new appearance with limited activity, while W2MMD, N2LQH, KC2GYU, and W2LJR experienced severe drop-offs or complete silence, highlighting a need for maintenance checks across several member stations.
Outside the club, KD3ANN and VE3VRO both experienced roughly halving of their spot volumes without losing any bands, indicating a possible reduction in power or receiver sensitivity rather than a configuration change. Meanwhile, K4CHE nearly ceased reporting after a strong August, a pattern that mirrors the technical or operational interruptions seen in some local members. These external examples serve as a reminder that even established, high-output stations can experience rapid fluctuations due to environmental or hardware factors.
New this month
| Callsign | Spots | Bands | P90 (mi) |
|---|---|---|---|
| KB2MMI | 54,871 | 80m, 40m, 30m, 20m, 17m, 15m, 12m | 4,041 |
| KE2DST ★ | 1,311 | 30m | 736 |
| N3WVW | 543 | — | 4,716 |
Dropped out
| Callsign | Prior spots | Current spots | Prior bands |
|---|---|---|---|
| W2MMD ★ | 180,260 | 18,160 | 40m, 30m, 20m, 15m |
| AC3AU | 140,690 | 0 | 20m, 17m |
| N2LQH ★ | 49,015 | 0 | 80m, 40m, 20m, 17m, 15m, 10m |
| KC2GYU ★ | 38,656 | 0 | 80m, 40m, 30m, 20m, 17m, 15m, 12m |
| K4CHE | 26,804 | 5 | 40m |
| W2LJR ★ | 4,872 | 0 | 20m |
| KR4OGH | 4,250 | 0 | 20m |
| AE3J | 1,150 | 0 | 20m |
| KE2BUO | 778 | 0 | 20m |
| N5SLN | 582 | 0 | 20m |
Expanded activity (more spots or added a band)
| Callsign | Prior → current spots | Change | Added bands |
|---|---|---|---|
| KD2EIB ★ | 913 → 2,166 | +137% | — |
Contracted activity (fewer spots or lost a band)
| Callsign | Prior → current spots | Change | Lost bands |
|---|---|---|---|
| KE2AQZ ★ | 29,246 → 13,538 | -54% | — |
| KD3ANN | 138,283 → 70,614 | -49% | — |
| VE3VRO | 105,095 → 56,382 | -46% | — |
| K2ZA ★ | 180,819 → 164,468 | -9% | 15m |
GCARC member focus (all members, any activity either month)
| Callsign | Prior → current spots | Change | Bands prior → current | Max DX (mi) prior → current |
|---|---|---|---|---|
| KS2D | 183,886 → 236,168 | +28% | 80m,40m,30m,20m,17m,15m,12m,10m → 80m,40m,30m,20m,17m,15m,12m,10m | 11,664 → 11,797 |
| K2ZA | 180,819 → 164,468 | -9% | 40m,30m,20m,15m → 40m,30m,20m | 11,768 → 11,768 |
| W2MMD | 180,260 → 18,160 | -90% | 40m,30m,20m,15m → 40m,30m,20m,15m | 11,756 → 10,579 |
| WB2MNF | 79,353 → 63,744 | -20% | 30m → 30m | 10,542 → 10,542 |
| N2LQH | 49,015 → 0 | — | 80m,40m,20m,17m,15m,10m → — | 11,776 → 0 |
| KC2GYU | 38,656 → 0 | — | 80m,40m,30m,20m,17m,15m,12m → — | 11,664 → 0 |
| KE2AQZ | 29,246 → 13,538 | -54% | 40m → 40m | 11,636 → 4,325 |
| W2LJR | 4,872 → 0 | — | 20m → — | 10,588 → 0 |
| KD2EIB | 913 → 2,166 | +137% | 40m → 40m | 801 → 624 |
| KE2DST | 0 → 1,311 | (new) | — → 30m | 0 → 3,514 |
| W2TDS | 0 → 60 | (new) | — → — | 0 → 2,216 |
40m
| Rank | Call | Spots | Uniq RX | P90 (mi) | Mi/W | Cont. | Dir cov | Days on air | Spots/day | EU % | DX % | Best DX |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | K2ZA | 64,070 | 945 | 3,866 | 275 | 6 of 6 | 14/16 | 28/30 | 2,288 | 38% | 22% | VK6KLI |
| 2 | W4EO | 163,527 | 915 | 2,551 | 12,359 | 6 of 6 | 14/16 | 30/30 | 5,450 | 25% | 10% | VK6KLI |
| 3 | KD3ANN | 33,089 | 900 | 3,996 | 365 | 6 of 6 | 14/16 | 16/30 | 2,068 | 37% | 27% | VK6KLI |
| 4 | WA3DNM | 40,730 | 875 | 4,042 | 431 | 6 of 6 | 14/16 | 28/30 | 1,454 | 42% | 37% | VK6KLI |
| 5 | KS2D | 81,310 | 622 | 2,241 | 4,313 | 5 of 6 | 14/16 | 27/30 | 3,011 | 15% | 3% | VK6PVL |
| 6 | WF1L/B | 31,176 | 557 | 3,600 | 5,506 | 5 of 6 | 13/16 | 30/30 | 1,039 | 25% | 13% | VK5HW |
| 7 | AC2WB | 3,488 | 556 | 4,009 | 424 | 6 of 6 | 14/16 | 3/30 | 1,162 | 41% | 38% | VK6KLI |
| 8 | KB2MMI | 19,910 | 518 | 3,796 | 6,238 | 4 of 6 | 14/16 | 6/30 | 3,318 | 34% | 18% | VK5HW |
| 9 | W2MMD | 11,443 | 296 | 904 | 2,261 | 4 of 6 | 14/16 | 19/30 | 602 | 10% | 1% | PP5ZX |
| 10 | KE2AQZ | 13,538 | 180 | 624 | 3,194 | 3 of 6 | 12/16 | 3/30 | 4,512 | 5% | 0% | OE3GBB |
| 11 | KD2NRJ | 7,810 | 143 | 502 | 2,920 | 2 of 6 | 12/16 | 9/30 | 867 | 0% | 0% | EA8BFK |
| 12 | KD2EIB | 2,163 | 39 | 309 | 2,517 | 1 of 6 | 9/16 | 29/30 | 74 | 0% | 0% | KX4AZ/T |
K2ZA’s superior performance stems from a pronounced eastbound advantage, as the receivers it uniquely reached are heavily concentrated in Europe and at long distances, suggesting a low-angle takeoff optimized for transatlantic paths. In contrast, W4EO’s unique captures cluster tightly to the west and at much shorter ranges, indicating a pattern that favors regional North American contacts over the long-haul DX paths that K2ZA dominated. This directional disparity explains why W4EO generated far more total spots despite similar maximum range, as its energy was directed toward a denser, closer population of stations rather than the sparse European band. KS2D delivered the best efficiency per watt of the group, achieving strong results with modest power, while W2MMD’s limited European reach and lower spot volume suggest a less optimized or lower-height antenna system. KE2AQZ showed promise with high spot density but was limited by very few days on air, whereas KD2EIB’s tight regional footprint and lack of DX highlights the constraints of a low-gain, likely vertically polarized or low-height installation. To improve overall DX capability, the group should prioritize raising antenna heights to lower the takeoff angle, which would help stations like W2MMD and KD2EIB break through local noise floors and access the European path that K2ZA exploited so effectively.
30m
| Rank | Call | Spots | Uniq RX | P90 (mi) | Mi/W | Cont. | Dir cov | Days on air | Spots/day | EU % | DX % | Best DX |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | K2ZA | 66,947 | 700 | 4,035 | 480 | 6 of 6 | 14/16 | 28/30 | 2,390 | 41% | 40% | VK6KLI |
| 2 | WA3DNM | 58,478 | 662 | 4,042 | 434 | 6 of 6 | 14/16 | 28/30 | 2,088 | 37% | 31% | VK6KLI |
| 3 | KS2D | 37,956 | 401 | 2,693 | 7,698 | 5 of 6 | 13/16 | 27/30 | 1,405 | 23% | 10% | VK6PVL |
| 4 | WF1L/B | 21,301 | 362 | 3,848 | 9,685 | 6 of 6 | 13/16 | 30/30 | 710 | 29% | 22% | VK6PVL |
| 5 | AC2WB | 1,734 | 323 | 3,993 | 451 | 6 of 6 | 13/16 | 3/30 | 578 | 40% | 37% | VK6PVL |
| 6 | W4EO | 35,391 | 319 | 2,536 | 13,869 | 5 of 6 | 12/16 | 30/30 | 1,179 | 18% | 7% | VK6PVL |
| 7 | WB2MNF | 63,737 | 292 | 2,739 | 10,371 | 4 of 6 | 11/16 | 30/30 | 2,124 | 26% | 9% | VK5ARG |
| 8 | KB2MMI | 5,887 | 232 | 3,762 | 7,580 | 4 of 6 | 11/16 | 6/30 | 981 | 30% | 20% | VK5ARG |
| 9 | 107ADO | 520 | 97 | 8,339 | 1,451 | 1 of 6 | 10/16 | 11/30 | 47 | 0% | 76% | VE6JY |
| 10 | W2MMD | 1,866 | 91 | 1,933 | 4,572 | 4 of 6 | 9/16 | 19/30 | 98 | 23% | 8% | VK5ARG |
| 11 | KE2DST | 1,311 | 42 | 736 | 5,741 | 2 of 6 | 8/16 | 4/30 | 327 | 0% | 1% | EA8BFK |
K2ZA’s superior DX performance stems from a distinctly stronger eastbound radiation pattern, as evidenced by its unique reception of significantly more European stations compared to WA3DNM. While both stations achieved similar maximum distances, WA3DNM’s exclusive contacts skewed heavily westward and northward at shorter ranges, suggesting its antenna pattern favors local or regional paths over the low-angle takeoff required for transatlantic work. This directional divergence allows K2ZA to capitalize on the high European activity fraction, whereas WA3DNM’s west-leaning nulls limit its long-haul efficiency despite comparable power levels. KS2D demonstrates exceptional efficiency per watt, likely benefiting from a highly optimized feedline or low-loss antenna system, though its lower overall DX ratio indicates a pattern less suited for distant continents. WB2MNF consistently held the highest spots-per-day among the lower-power operators, reflecting strong reliability and a robust local signal despite modest output. W2MMD struggled with limited on-air time and a tight regional footprint, resulting in minimal DX success and low overall visibility. KE2DST’s near-total lack of European reach and extremely limited activity window confirm a highly localized performance profile with little impact on the wider network. To improve overall group efficacy, operators should consider raising antenna heights slightly to lower takeoff angles, specifically targeting the European path where K2ZA’s pattern advantage is most pronounced.
20m
| Rank | Call | Spots | Uniq RX | P90 (mi) | Mi/W | Cont. | Dir cov | Days on air | Spots/day | EU % | DX % | Best DX |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | W4EO | 83,740 | 1,012 | 3,948 | 22,922 | 6 of 6 | 15/16 | 30/30 | 2,791 | 29% | 19% | VK6QS |
| 2 | VE3VRO | 56,379 | 982 | 2,572 | 76,766 | 6 of 6 | 14/16 | 30/30 | 1,879 | 49% | 7% | ZL2AIU |
| 3 | WA3DNM | 31,856 | 940 | 4,042 | 486 | 6 of 6 | 15/16 | 28/30 | 1,137 | 37% | 31% | VK6QS |
| 4 | K2ZA | 33,397 | 909 | 3,982 | 432 | 6 of 6 | 15/16 | 28/30 | 1,192 | 35% | 25% | VK6QS |
| 5 | KD3ANN | 20,138 | 896 | 4,069 | 494 | 6 of 6 | 16/16 | 16/30 | 1,258 | 41% | 35% | VK6QS |
| 6 | KS2D | 26,830 | 537 | 2,574 | 8,661 | 5 of 6 | 15/16 | 27/30 | 993 | 20% | 9% | VK6QS |
| 7 | AC2WB | 2,198 | 457 | 3,997 | 473 | 6 of 6 | 15/16 | 3/30 | 732 | 36% | 29% | VK6QS |
| 8 | WF1L/B | 12,546 | 448 | 3,563 | 8,773 | 4 of 6 | 13/16 | 30/30 | 418 | 25% | 14% | VK6QS |
| 9 | KB2MMI | 9,527 | 446 | 3,711 | 10,152 | 5 of 6 | 14/16 | 6/30 | 1,587 | 26% | 17% | VK6QS |
| 10 | W2MMD | 3,628 | 217 | 2,416 | 7,421 | 5 of 6 | 14/16 | 19/30 | 190 | 10% | 6% | VK5EI |
W4EO’s superior total spot count despite significantly lower transmit power highlights a fundamental efficiency advantage, likely stemming from a higher elevation or more optimized antenna system that favors low-angle radiation. The receiver set-difference reveals that W4EO uniquely reached a volume of nearby North American stations to the west, suggesting a pattern optimized for strong local and regional signals, whereas K2ZA’s unique hits were dominated by distant European receivers to the east. This indicates K2ZA’s antenna is likely tuned for a higher takeoff angle or possesses a deeper null toward the west, allowing it to punch through to long-haul EU paths that W4EO missed, even though W4EO compensated for this with sheer volume and broader directional consistency.
Within the wider GCARC group, KS2D demonstrates exceptional efficiency per watt, achieving a high miles-per-watt ratio and solid DX percentage despite operating at modest power levels, which suggests a well-tuned antenna system with minimal losses. W2MMD’s lower unique receiver count and limited European reach point to either a less effective antenna pattern or a constrained operating window, resulting in a tighter regional footprint compared to the group leaders. To improve overall performance, the group should consider experimenting with antenna height adjustments to optimize the takeoff angle for long-distance paths, as the data suggests that vertical polarization efficiency and elevation play a critical role in distinguishing between local dominance and true DX capability.
15m
| Rank | Call | Spots | Uniq RX | P90 (mi) | Mi/W | Cont. | Dir cov | Days on air | Spots/day | EU % | DX % | Best DX |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | KD3ANN | 7,678 | 460 | 4,159 | 577 | 6 of 6 | 14/16 | 16/30 | 479 | 50% | 52% | VK5HW |
| 2 | WA3DNM | 9,679 | 399 | 4,107 | 560 | 6 of 6 | 13/16 | 28/30 | 345 | 49% | 53% | VK6KLI |
| 3 | KS2D | 9,452 | 222 | 3,970 | 12,656 | 4 of 6 | 9/16 | 27/30 | 350 | 41% | 31% | PP5ZX |
| 4 | WF1L/B | 4,783 | 169 | 3,985 | 12,803 | 5 of 6 | 8/16 | 30/30 | 159 | 40% | 33% | VK7JJ |
| 5 | KB2MMI | 2,911 | 152 | 3,948 | 11,772 | 5 of 6 | 8/16 | 6/30 | 485 | 40% | 30% | VK5ARG |
| 6 | W4EO | 8,140 | 143 | 3,514 | 21,897 | 6 of 6 | 7/16 | 30/30 | 271 | 30% | 13% | VK5ARG |
| 7 | W2MMD | 1,222 | 86 | 4,037 | 12,575 | 4 of 6 | 7/16 | 19/30 | 64 | 38% | 30% | PP5ZX |
KD3ANN’s unique receiver set is heavily weighted toward Europe and distant eastern paths, suggesting a high-performance, low-angle antenna optimized for long-distance ionospheric propagation that successfully exploited the 15m band’s global opening potential. In contrast, KS2D’s exclusive contacts were predominantly nearby North American stations, indicating a pattern with significant takeoff angle or a local noise floor that favored regional NVIS or medium-distance hops while limiting its ability to compete with KD3ANN on deep DX paths. Although KD3ANN missed some local coverage that KS2D captured, the sheer volume and geographic spread of KD3ANN’s unique eastern reaches highlight a clear efficiency advantage in long-range signal projection despite KS2D’s longer operational uptime. W2MMD delivered a tight regional footprint with limited European reach, consistent with a lower-height antenna or suboptimal ground system that restricted its effective radiated power despite matching KS2D’s power levels. To improve overall group performance, stations should experiment with raising dipole heights or improving counterpoise systems to lower the takeoff angle, aiming to convert more of their near-field spots into the deep European and Pacific DX paths that define top-tier 15m performance.
10m
| Rank | Call | Spots | Uniq RX | P90 (mi) | Mi/W | Cont. | Dir cov | Days on air | Spots/day | EU % | DX % | Best DX |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | WA3DNM | 899 | 80 | 4,720 | 336 | 5 of 6 | 11/16 | 28/30 | 32 | 2% | 17% | VK2EFM |
| 2 | W4EO | 812 | 64 | 4,680 | 25,687 | 3 of 6 | 7/16 | 30/30 | 27 | 0% | 19% | PP5ZX |
| 3 | KS2D | 663 | 60 | 4,653 | 13,522 | 3 of 6 | 8/16 | 27/30 | 24 | 0% | 26% | PP5ZX |
WA3DNM’s unique reception set is heavily weighted toward distant North American and African targets with broad compass coverage, suggesting a high-efficiency, multi-directional antenna system optimized for low-angle radiation that effectively exploits long-haul paths. In contrast, KS2D’s exclusive contacts are tightly clustered in the western quadrant at shorter median distances, indicating a directional or vertically polarized array with a narrower beamwidth that favors regional propagation over global reach. While WA3DNM achieved significantly higher total spots and wider continental diversity, KS2D’s remarkably high miles-per-watt figure demonstrates superior efficiency per decibel, proving that a well-matched, low-power station can compete on distance metrics even with a more restricted pattern. KS2D stands out as the sole GCARC contributor this month, delivering a solid DX ratio and impressive efficiency despite limited European reach, which aligns with its observed westbound signal concentration. To further enhance KS2D’s global diversity, operators should consider experimenting with a higher antenna installation or a more omnidirectional vertical configuration to capture the eastern and northern paths that WA3DNM consistently accesses.
Receiver Coverage Map
Every receiver that decoded an FM29 transmitter this month, colored by the transmitter that heard it. Click station chips below to toggle ON/OFF; click band buttons to filter. GCARC stations are gold and ON by default; other FM29 stations are off — turn them on to compare coverage patterns.
18,746 unique (receiver, station, band) data points embedded. Click + drag to rotate; scroll to zoom. Each line traces an FM29 → receiver path.
