I got up quite early today and decided to check the beacons on 23 cm. When beaming to LA1UHG, there was a noticeable signal in F1 about 1 kHz above its frequency. It was easy to read it as DB0LB from the back of the dish. But it seemed, there was another faint signal right beside the spacing carrier. With the help of my SDR radio I could set very narrow filters and after a while of listening, I identified it as LA1UHG, JO59FB, 1028 km. Wow!
But the signal faded out more and more and at least it disappeared.
LA1UHG just 140 Hz below the space carrier of DB0LB
Later this morning, the dish still pointing north, I heard Kurt, OE5XBL, chatting in SSB with Rudi, OE5VRL/5, both with very strong signals on 23 cm. Expecting a huge signal, I turned the antenna to Kurt, but there was no significant increase in signal strength. I called in and the three of us were talking about the conditions and to meet for a beer at the GHz convention in Dorsten next February, when Kurt was called by Dave, G4RQI. I had tried with him earlier without any success, and so, to be honest, I was a little annoyed by this. Even, when turning the dish to the UK, I couldn´t copy anything of Dave’s transmissions, while he was working Kurt and Rudi. These were enough indications, that the inversion was at a too high altitude for me, to enter it. So I went for a long walk with my XYL in the nearby vineyards.
The inversion is at an altitude of about 1000 m (Courtesy DWD)
In the evening I performed another beacon check. It was funny to see beacons, the dish was pointing to, as well as others from the back of the dish
Dish pointing southeast: DB0UX, DB0VC, DB0AAT (from left to right)
Turning the dish, confirmed the experience I had in the the morning: Pointing southeast I saw DB0VC, JO54IF, next to DB0AAT, JN67HU. Turning the dish towards Kiel in the north, the signal of DB0VC increased just a little. Maybe, it has been reflected by a mountain range about 50 km southeast of me.
Dish pointing north: DB0UX, DB0XY, DB0VC, OZ7IGY (from left to right)
By performing my daily beacon check, I noticed a weak keyed carrier in between the spacing of the F1 signal of DB0UX on 2320.900 MHz. I assumed to see F6DWG/B, which I monitored around the .900 before. But it didn´t take long to find out, that the real signal (mark) was the lower carrier and after a while I learned, it was F5ZNI using reverse F1 keying. Later in the evening the signal increased due to good tropo conditions, as can be seen in the pictures. F5ZNI is the 34th beacon I received in the 13 cm (S) Band
F5ZNI and DB0UX in PowerSDR
I am always happy about new beacons, but this case is an example, why beacon coordination and using standards is most important. First of all, reverse F1 keying is always bad, as you are used to listen to the upper carrier of the signal. In case there is an unkeyed carrier in between the text, you can easily identify the mark, where to listen. But if there is text keyed nearly all the time, as F5ZNI does, it is rather time consuming until the mark is identified.
The DB0UX signal was strong and the frequency is locked to a reference, while F5ZNI is drifting a little. So it was obvious, that there was a second signal in place. If the french beacon would have been locked to 2320.900 MHz too and would use the standard A1 or F1 keying, there would have been no chance for me to monitor or even to take notice of it.
An excerpt from BEACONSPOT.UK shows the situation on 2320.900 MHz:
Beacon
Nominal Frequency
Locator
Last Spotted
Last Frequency
Status
F6DWG
2320.900
JN19BQ
2019-05-31
2320.898
Dead/lost
HG3BUC
2320.900
JN96CC
2019-10-11
2320.897
Operational
OZ5SHF
2320.900
JO45VX
2019-08-24
2320.900
Operational on spot date
DB0MJ
2320.900
JO31UB
2019-12-29
2320.905
Operational
ON0TB
2320.900
JO30BM
2019-09-20
2320.897
Dead/lost
DB0UX
2320.900
JN48FX
2019-12-29
2320.900
Operational on spot date
F1ZCC
2320.900
JN08XS
Uncertain - new spot required
SR1SHS
2320.900
JO73PG
2019-12-30
2320.900
Operational
IQ5FI
2320.903
JN53SR
2019-12-28
2320.901
Operational
F5ZNI
2320.904
JN19BQ
2019-12-30
2320.899
Operational on spot date
Depending on the location and the conditions, there will be more or less interference on 230.900 MHz
As the beacon keeper Thomas, DL4EAU, wrote me, the DB0XY beacons in JO51EU are back on air. The frequencies are 1296.912, 2320.912 and 10368.912 MHz. All are locked to a GPS reference now.
DB0XY on 1296.912 MHz in JN49CV: A weak tropo trace, but many nice reflections on airplanesDB0XY on 2320.912 MHz: No trace via tropo, but many reflections on planes
On the annual service day of the DARC districts Saarland and Rhineland-Palatinate I had the pleasure to hold a lecture about EME basics and how to get into. Afterwards I invited the audience to try a live moon bounce QSO on 432 MHz from the parking lot outside. I had prepared some standard equipment of the kind, many might have in their shacks:
Transceiver Yaesu FT-897
15-Element Yagi (YU7EF )
PA Gemini 70, ca. 200 W
LNA SHF-Elektronik, 0,8 dB NF
EME rig in the boot, Photo by courtesy of Klaus, DF6WN
Unfortunately it was rainy outside, the moon close to the sun and a G2 solar storm in progress. When swithing on the transceiver, I noticed some quite massive local QRM. Nevertheless I contacted Bernd, DL7APV, who had agreed in a sked, by phone, to tell him about the noise and that we were ready to go.
Bernd´s array of 128 x 11 elemnt yagis during a barbeque last June
As the noise level went up and down and Bernd is one of the big guns on 70 cm, we were able to decode most of his transmissions despite all adversities. Finally we completed the QSO. That was a great job, Bernd!
I enjoyed to be in Saarbrücken and would like to say thank you to Eugen, DK8VR and his team for organising DST 2019!
When looking for EA2TZ/B during a beacon check a couple of days ago, I mentioned a signal with strong doppler shift about a khz below. As I like the challenge to identify new beacons, I started monitoring it. It became a kind of a nightmare, trying to to catch the beacons callsign. It seems to be very chatty, transmitting a whole bunch of unuseful text. despite the fact I got a lot of good quality fragments via aircraft scatter, it took me hours to identify it as F1ZBK. At least I am pretty sure it is, as there is a second callsign in the end of the text: F1DND, maybe it´s the keepers call.
The text decoded so far is: —— beacon f1zbk jn38bp nancy … 854 khz … 5 watt … f1dnd … orange KA … ——- Where the “…” represent gaps and KA is the prosign for “Attention” or “New Message” (not to be used at the end of a message, like AR).
There are many beacons running in bad modes like reversed F2A or keying the subcarrier of F2A, but transmitting such a lot of stuff is worse.
As OK0EA was audible this morning on 23 and 13 cm I had a look for other, more distant beacons in OK. After noticing a very short and weak signal on 2320.9085 MHz, I monitored the frequency over a couple of hours and saw many doppler shifted traces, typical for aircraft scatter. Very soon I copied “…9DP…”, when a B777 crossed the path and was sure to see OK0ER in JN99DP in the waterfall diagram. At least 4 Airbuses A380 crossed the path one after the other, giving nice reflections.
OK0ER transmits 1.5 W into a slot antenna in 675 m asl. The distance is 722 km.
Großes Finale im Weltraum-Projekt zum Ende des Kindergartenjahres!
Seit dem Auftakt mit einer Mondbeobachtung an der Paul-Baumann-Sternwarte der Astronomischen Arbeitsgemeinschaft Mainz e.V. im April konnten die Kinder viele Eindrücke vom Weltraum und dem Leben der Astronauten auf der Internationalen Raumstation sammeln. Sie absolvierten ein Raumfahrer-Training und stellten selber Astronauten-Nahrung her. Es wurde der Flug von Alexander Gerst zur ISS verfolgt und eigene Brausepulver-Raketen gestartet. Warum Funkverbindungen hinter den Horizont schwierig sind, konnte mit Walkie-Talkies selbst ausprobiert werden. Und nicht zuletzt war dann Astro-Alex selbst live per Amateurfunk von der Raumstation zu hören, als er Fragen von Schülern von Schulen in Leverkusen und Herrenberg beantwortete.
Bild: Alexander fliegt zum Mond (Ben Brinkhus)
Da der Mond ein erklärtes Ziel von Alexander Gerst ist, haben die Kinder dann Bilder gestaltet, die ihn auf dem Weg zum Mond zeigen. In Interviews erzählt er gern von seinem Opa, der als Radioamateur Funksignale am Mond reflektieren lassen konnte, was den jungen Alexander seinerzeit immens beindruckt hat. Deshalb wurde eins der Bilder ausgewählt und zusammen mit einem Foto von ihm, seinem Missions-Logo und dem Logo der Kindertagesstätte St. Laurentius ging es auf die Reise nach Italien zu Nando Pellegrini, der als Funkamateur unter dem Rufzeichen I1NDP eine große Sendestation betreibt. Mit seinem Parabolspiegel, der einen Durchmesser von 10 m hat, sendete er die Bilder im 23 cm Amateurfunk-Band im sogenannten Slow-Scan-Television-Verfahren, ähnlich einem FAX, in Richtung Mond. An der Oberfläche unseres Trabanten wurde die Funksignale reflektiert und trafen zweieinhalb Sekunden später mit Lichtgeschwindigkeit wieder auf der Erde ein.
Bild: Radioteleskop in Dwingeloo
Hier hatte sich das historische Radioteleskop in Dwingeloo in den Niederlanden bereitgehalten, um die Bilder nach ihrer Reise über fast 800.000 km wieder aufzufangen.Betrieben wird die denkmalgeschützte Einrichtung in der Provinz Drenthe im Nordosten der Niederlande von der CAMRAS Stiftung, in der eine große Zahl von Funkamateuren mitarbeitet. Hier, an der erst vor fünf Jahren aufwändig restaurierten Parabolantenne von 25 m Durchmesser, haben die italienische Künstlerin Daniela de Paulis und der niederländische Funkamateur Jan van Muijlwijk, Rufzeichen PA3FXB, im Jahr 2009 das „Visual Moonbounce“ genannte Verfahren entwickelt, bei dem sie im Rahmen von Kunst-Projekten und Astronomie-Events der „Astronomers without Borders“ mit Hilfe geeigneter Gegenstationen in Italien, Brasilien, Großbritannien und der Schweiz Bilder am Mond reflektiert lassen.
Dank guter persönlicher Kontakte konnten die beteiligten Funkamateure dafür gewonnen werden, die Bilder der Ebersheimer Weltraumkinder im Rahmen einer öffentlichen Veranstaltung in Dwingeloo zum Mond zu schicken, um den dortigen Besuchern „Visual Moonbounce” eindrucksvoll zu demonstrieren.
Bild: Alexander Gerst (ESA)
So kam es, dass nicht die ESA, sondern die Weltraumkinder der Kindertagesstätte St. Laurentius in Mainz-Ebersheim Alexander Gerst zum Mond geschickt haben.Wir danken Daniela de Paulis, Jan van Muijlwijk, Nando Pellegrini sowie dem Team CAMRAS für die Unterstützung unseres Weltraum-Projekts! Das Bild vom Flug zum Mond hat das Weltraumkind Ben Brinkhus gestaltet.
Ansprechpartner für das Weltraum-Projekt: Regina Imse,
Kath. Kindertagesstätte St. Laurentius, Großgewann 2,
55129 Mainz-Ebersheim
Bildnachweis:
Zeichnung „Alexander fliegt zum Mond“: Ben Brinkhus
Alexander Gerst, Horizons-Logo: ESA
Radioteleskop Dwingeloo: Andreas Imse
Logo der Kindertagestätte St. Laurentius, Mainz-Ebersheim
Reflektierte Bilder: Nando Pellegrini und Team CAMRAS
After I noticed some spots for SR1KOL in JO74SE on 1296.960 MHz, I monitored the frequency using WSJT-X Wide Graph. About 400 Hz below the nominal frequency traces of a F1 signal can be seen, when airplanes cross the path to the beacon. The signal is not audible, but I am pretty sure, it is SR1KOL.
Traces of SR1KOL in JO74SE, “1000” = 1296.960 MHz. The strong signal at the very left is a birdie.
Some information can be found on the website of Polski Klub UKF: It is located on a high rise building in Kołobrzeg, 40 m above ground. The power is 3 W into a slot antenna. Beacon keeper is Andrzej, SQ1GU.
The video shows an A380 crossing the path between DJ5AR and SR1KOL. At minute 2:00 the plane crosses the first time and at minute 4:00 after a turn it crosses a second time. Mind the traces at 580 Hz in the waterfall diagram. The 1000 Hz mark corresponds to 1296.960 MHz.
Irek, SP5MX, who was involved in building the beacon and who repaired it recently, told me, the beacons reference is an OCXO withtout any GPS-lock. So possibly the beacon may transmit 400 Hz lower than defined.
At least in the morning of July 31st audible reflections could be heard via an Airbus A330. This time the 1000 Hz mark correspondents to 1296.9596 MHz.
After 10 seconds the noise becomes a kind of ‘musical’. Another 10 seconds later experienced ears can hear the tone.
When switching to 13 cm after monitoring GB3MHZ on 23 cm, I heard typical PI4 sound followed by a callsign in CW. So I learned, former GB3MHS changed the callsign to GB3MHZ and is transmitting in PI4 now.
The french beacon F5ZBM is on air again. I found it accidentally, when looking for other french beacons. It is at a new location in JN18MN near Paris transmitting on 1,296.8475 MHz. Nice to monitor it in Mainz via aircraft scatter over a distance of 406 km!
The keying is in F1 with a very narrow spacing. Power is 10 W ERP into a slot antenna, as can be seeen at BEACONSPOT.eu
