PA7JB, G4RGK, G3LTF, SM0ERR, RW3BP, UA3AHM, SM7FWZ, UA3TCF,
SM5BSZ, DJ8FR, SM2CEW, SM0DFP, SM7GEP, RA3AQ, SM4IVE, SM6PGP, SM5QA, SM7SJR,
SM6CKU, OZ4MM, DL1YMK, YMK/Monica, SM7GVF, ON5TA, PA2DW, SM4FXR, SM6FHZ, ON7UN,
DL6SH, SM4DHN, PA3DZL, OZ6OL, KE9M, HB9BBD.
Pictures by Ingolf Larsson, SM6FHZ
Report compiled by Peter G3LTF.
There were 32 attendees at the 2013 Swedish EME meeting at Orebro
on May25-26 May who enjoyed a fascinating set of presentations about detailed
aspects of EME as well as enjoying the opportunity to meet, greet and discuss
with old friends.
Thanks of everyone go to Lars SM4IVE for organising the event and
to all the presenters and supporters, especially Mart SM0ERR and Leif SM5BSZ who
supplied and manned the measurement suite.
Ingolf SM6FHZ
described a suite of Kumar (VE4MA) feeds with 5 step septum polarisers,
carefully optimised for f/D ratios 0.32 to 0.42 for 23, 6 and 3cm. This is
focussed on optimum amplitude and flat phase across the aperture and low cross
polarisation. The measured performance of return loss (RL) and isolation shows
excellent agreement with the modelling results. The W1GHZ feed efficiency
programme is used for evaluation so direct comparisons can be made with other
work. All dimensions are given for 23, 6 and 3cm. See
http://www.2ingandlin.se/SM6FHZ.htm hopefully, in time, Ingolf
will add 9 and 13cm dimensions. With this suite and the septum fed W2IMU
described by Marc N2UO (see
http://www.ok1dfc.com/EME/emeweb.htm ) we
now have for 23cm a set of optimised feeds covering 0.32 to 0.6 f/D. Ingolf
cautioned against scaling between frequency bands so we probably need some more
work on the septum fed W2IMU for 13-3cm. For those who play with feeds and
dishes Ingolf’s slides 13-16 are of great interest because they show that,
because of the variation of cross polar response with choke position it is
possible to maximise sun noise (randomly polarised) but then find yourself with
sub-optimum coherent signal performance.
Hannes SM6PGP
described the manufacture of the
new design Kumar
feeds for 6 and 3cm using his home workshop and for
those who build feeds I strongly recommend looking at his slides for some useful
tips on manufacture and assembly / alignment. The designs use standard pipe
sizes which is a big advantage. Both Hannes and Ingolf have used these feeds in
their systems with excellent results.
A
novel 5 step septum feed suite_A.pdf
(Link
to Hannes' webpage for updated versions of the document)
Leif SM5BSZ
outlined the several potential error sources when making accurate total power
measurements of moon (or radio star) noise as a means of evaluating system noise
temperature. Very small Y factor ratios are involved. For example because most
LNAs gain values are very sensitive to input source impedance a small change in
feed position relative to the dish surface could induce an error. A more
accurate measurement of moon noise can be made by injecting a small stable
signal into the front of the system and making a SINAD measurement instead using
LINRAD. Leif was also making a set of precision NF measurements using a special
set up described on his webpage
http://www.sm5bsz.com/lir/loss/1296/hp8970a/hp8970a-auto.htm
Mart SM0ERR
described how accurate measurements of very small losses in components like
adaptors and relays can be made. The magnitude S11 of the item to be assessed is
measured using precision open and short circuit terminations at its output
terminals. By taking the average and dividing by 2, the loss can be measured.
This is best done by using an automatic network analyser. (But it can be done
manually). Some actual results were presented. Note that at 23cm with NFs now in
the 0.2dB region these items have even more effect on Tsys. Mart also measured
the Noise Figure of a large number of preamps and the results will be on this
webpage when the document is compiled.
Jurgen DJ8FR
demonstrated the use of a highly portable VNA made by SDR kits
http://www.sdr-kits.net/Webshop/products.php?14&cPath=5
to measure the RL and isolation of a 23cm RA3AQ feed
Sergei RW3BP
described the progress with his 76GHz system, the essentials are a 60W twt (that
requires 31kV), a 2.4m offset dish, and several 4db LNAs. But that is just the
start! Sergei described a long and painstaking process of finding the correct
focal point of the dish; and similar efforts in all other areas of the system.
The reduced radar cross-section of the moon, libration and atmospheric
absorption add extra losses of 25dB in summer, reducing to 19dB in winter
(that’s a Moscow winter) He showed clearly visible echo results using stacked up
echoes on Spectran. This is a unique set up involving serious engineering and
Sergei hopes that someone in NA will soon construct a similar set up for the
first 76GHz EME QSO
eme_on_77ghz.pdf
http://www.youtube.com/watch?v=2En_W2EaJFw
Dmitry RA3AQ
presented the results of modelling using the OM6AA full dish
simulation of some of his feed designs in various dish sizes. With the low sky
temperatures at 23 and 13cm especially, and very low noise figures in the 0.2dB
region there is much to be gained from careful feed and f/D choices. A lot of
very interesting data is available from his presentation and if there is one
clear message it is this. Looking at the W1GHZ curves of dish efficiency versus
f/D ratio, be sure to stay on the lower (smaller f/D) side of the peak.
http://www.vhfdx.ru/faylyi/view-details/radiolyubitelskie-raschetyi/ra3aq-orebro-2013-eme-meeting-pdf
Dick PA2DW
brought us up to date on the PI9CAM Dwingeloo dish project, he showed the
fascinating film that was shown at EME2012 and emphasised the use of the dish
for educational outreach. An enormous amount of repair and restoration work has
been done by volunteers as well as professionals and the hope is that the dish
will be back in operation in November/ December this year. Many hundreds of QSOs
were made on 70 and 23cm before the re-build began, hopefully with the dish
profile improved from the repairs (with new magic mushrooms!) there will
be some more operation on the bands above 23cm.
http://www.camras.nl/
Ingolf SM6FHZ and Hannes, SM6PGP
described a novel 23cm feed for small dishes (1.8 and 2.4m) comprising a patch
housed in a cavity with a beam-forming ring in front. Ingolf modelled this
comprehensively and optimised its performance for two variants one with the ring
covering f/D 0.34 to 0.43 and a second 0.3 to 0.38. Detailed dimensions and
construction details are given on his webpage, quoted earlier. There are two
orthogonal feed points which can be fed with a 90 degree hybrid to produce the
required CP and with SSPAs spatial combining can be utilised, saving a high
power combiner. Hannes has used this on his 1.8m dish to make both CW and JT65
QSOs and has copied LX1DB and OK2DL on ssb.
Circularly polarized patch feed for 1296 MHz_A.pdf
Dominique HB9BBD
showed a fascinating film detailing the obtaining, restoration, installing and
then re-installing (to get an improved window) of his 10m dish. This involved
substantial amounts of steel and concrete and the use of helicopters and large
cranes, definitely not for the faint-hearted! With its hydraulic control system
it is a beautiful piece of engineering. The film was also very entertaining and
the on-air results speak for themselves.
http://hb9bbd.ch/
Michael DL1YMK and Monika
described their 2012 EME dxpedition to Corsica. For the first time they added
6cm operation to the bands worked on the 4m stress dish and also (another first)
used 10GHz with a separate 1.8m solid dish. For details of QSOs made on 70,
23,13,6 and 3cm see
http://www.ok1dfc.com/peditions/ymk2012/dl1ymk2012.htm
9cm is not available in French territories. Michael concludes that the stress
dish is not good enough for 6cm, although he did make 5 contacts, and that a
1.8m dish is too small for 10 GHz CW contacts so his plan is to find a way to
take a 2.4m dish on future expeditions for those two bands. It has to be both
light and transportable in sections. (He is considering offset following
discussions after the presentation!) We could not determine the location of this
years (possible) planned expedition but were told that a complete absence of
small biting insects inside the house is now an essential for the logistics
manager.
Schweden2013.ppsx
(abt 33 Mb to download. You may need Powerpoint viewer to
watch the file, available at the
Microsoft webpage)
Michael DL1YMK
described the design and construction of the two SSPAs that he made for the
Corsica expedition. These used devices from ELISRA TV links combined with ring
hybrids and needed a significant amount of “snow-flaking” to tune then up.
Michael emphasised the need to protect the eyes while doing his as there is a
significant radiation from the strip line discontinuities Useful device numbers
are FLM1112-8F, FLM1112-12F and TIM 1112-8,
Schweden2013_10G.ppsx
(8 Mb file)
SM2CEW moderated the Round-up session
After thanking everyone who had contributed to organisation and
presentation he emphasised three things we needed to do to increase EME
activity. Inspiration, Information and Focus. Inspiration came from the
excellent technical and operating work that we had heard about at this meeting.
Information comes from the distribution of this which will be done by publishing
on the
http://www.moonbouncers.org/ website and by distributing a
summary (this) to the appropriate newsletters and interested groups, and Focus
comes from ensuring that there is a solid presence of CW activity in addition to
digital operation.
DUBUS Contests Joe CT1HZE, who
organises the DUBUS contests asked that there be a discussion on timings, dates
etc. Points made were: Please continue to organise the contests. One suggestion
made was to have one day only per band and a pairing of bands for the weekend
chosen, for example 144 and 432 on Saturday – Sunday. There is of course the
risk of bad weather if we go for only one day per band.
There was also a call for the weekends chosen to be lower loss
(i.e. closer to perigee) but several disagreed citing horizon blockage. (This
will be a problem for at least 3 years until high moon declination and perigee
get back into synch) In order to get dates into diaries and maximise activity
then it’s essential to have the contest dates announced in DUBUS by October at
the latest.
Activity Weekends
Yes, continue, as they are noticeably increasing activity on the
bands above 13cm. We will have to change the date of the 2013 9cm weekend as it
clashes with the 9cm DUBUS contest. We will move it to share the 6cm AW, 3-4th
August.
Circular Polarization on 3cm
With the availability of the 10.368 / 10.450 GHz septum polariser
Kumar feed described by SM6FHZ there was a strong feeling expressed that CP
should become standard there as well as on the lower bands.
Encouraging cross-mode contacts
Suggestions were: replying to JT CQs on 23cm using SSB
and, on 70cm, calling CQ on 432.060 (which has worked) but both require the JT
audio to be switched on! PI9CAM reported considerable interest in CW operation
among young visitors to the big dish, seeing it done on a screen was more
commonplace for them.
Finally a decision was made to hold the Örebro EME meeting every
2nd year, in between the big international EME conferences.
A big thank you to Lars SM4IVE for organizing the meeting
again in 2013, see you all in
France 2014 and back in Örebro in 2015!
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