On the 1st of December, we arrived on site around mid-day.
Field conditions were favourable this year, with no mud or heavy
ploughing as encountered on previous expeditions. This allowed for a smooth
installation of the first set of receiving antennas. Deployed were the 300°
North American Beverage, the reversible ARG/JAP Beverage, and the African BOG
(Beverage On Ground).
Other participants deployed the following antennas: Vertical 9 metre
with balun, LA-1 van Dijken loop, 1090Mhz antenna, Active L-Band 1525-1660
antenna, Vertical 7,- m, T2FD or13 MHz and a Sony AN1.
On the following day, the Far East /
Initial monitoring was severely affected by wideband QRM. Extensive
troubleshooting followed: all feedlines and terminations were checked, laptops
and other potential noise sources were powered down, and a systematic RFI hunt
was carried out using a portable receiver both indoors and in the field. Persistent
QRM was present throughout — until the small house was investigated. After
switching off the halogen lighting, the noise floor dropped very dramatically,
resulting in a largely clean MW band.
It was later noted that the Deepelec DP-666 is not suitable for MW-QRM
hunting, as its display generates noise, potentially leading to false
conclusions during RFI investigations.
Consequently, the first night produced little of interest beyond the
usual power stations.
Geomagnetic conditions were poor, and propagation forecasts suggested a
preference for southern paths. African trans-equatorial paths, however,
underperformed — possibly also due to limited monitoring time spend and the
shrinking number of active MW broadcasters in that region. In contrast, the
Argentine Beverage delivered consistently more results.
Unfortunately, for several years now, antenna deployment during the
hunting season has been prohibited on the surrounding fields which results that
the chances to end up in the "Winter Anomaly" is a real bugger, and this
expedition clearly reflected that limitation. Signals frequently hovered just
above the noise floor, with only brief enhancements lasting a minute or so. So
you had to be lucky to be able to grab an ID in these cases. Nevertheless, it
remains remarkable that even weak signals can still exhibit acceptable
intelligibility under favourable noise conditions. Several stations, provided
just sufficient audio for tentative or positive identification.
For the first time, a temporary FMDX.org remote server was brought
online at the site. It utilised an oddly shaped antenna that had originally
been intended as a ground-plane but proved usable as a receive antenna.
Medium-wave propagation showed gradual improvement, particularly on the
Argentine Beverage, where signal levels increased in small but noticeable steps
over the days.
The final day offered improved South American propagation. Signals from
Notable catches with ID included R Atual,
Further First-logged stations were: Radio San Genaro, San Genaro Norte,
On 4 December, a strong candidate signal was detected that could only
correspond to Universo 970,
We were pleased to welcome Stef as part of the team. He provided assistance in a wide range of practical tasks in the field, the kitchen, the stove,etc, and shared valuable knowledge. As a newcomer to the Jaguar SDR user group, he also benefited from extensive exchanges with experienced Jaguar users.
It was equally rewarding to observe Frank’s home-designed and home-built
NAVTEX receiver in operation, demonstrating excellent performance in real-world
conditions.
Leen caught some nice Fax pictures shown below.
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On Friday, KNL-16 officially came to an end. The dismantling process — including the recovery and rolling in of several dozen reels of wire and coaxial cable — proceeded efficiently. All participants returned home safely. Several members left with storage media full of SDR recordings awaiting detailed post-expedition analysis.
While propagation conditions were occasionally uninspiring, the
expedition nevertheless yielded a number of valuable catches. Moreover, it
remains likely that additional weak or unidentified signals are still hidden
within the recordings.
Many thanks to all participants whose efforts contributed to the success
of this MW-DXpedition.






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