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February 2016

71

Regulars

FSK441 MS QSO followed by a SSB QSO

over that distance. I do wonder now if the

burst was from the Leonids shower which

usually has a sharp peak on 17 November.

I noticed several 30 second bursts in the

days following the predicted maximum of

this shower and it could be that the Leonids

were widely dispersed this year as certainly

there was no noticeable peak on the 17th.

The 2m tropo opening was a during the

Marconi CW contest on the morning of 8

November. I could copy CW signals from

all over Germany and the Czech Republic.

Unfortunately I don’t do CW and I had to

use a CW decoder program. As I couldn’t get

the decoder program to TX, no QSOs could

be made. Another opening occurred on 15

November, this time to Spain and EA1 and

EA2 stations were worked. During a contest,

on 1 December the band opened once more.

Stations in the south of France (JN16, 14

and 03) were worked amongst others. The

band was also open to the east with German

stations in locators JO31, JN49 and JN48

together with PA and ON answering my

contest CQ calls. That doesn’t often happen in

the regular 2m UKAC. The Geminids meteor

shower was much better than last year but it

was certainly not one of the best. Between

10 and 15 December, I completed 51, MS

QSOs with the following DXCC: I, DL, HB,

OK, SM, S5, LY, ES ,OH, OE, YL, OZ, YU,

SP, LA and UR. One new locator was worked

during a QSO with OH8K in KP13FA. Only

one of my QSOs was with a station at over

2000km, this was with YL2FZ in KO37QI at

2067km. I tried a number of times near the

peak of the shower to work RU1AA again at

2225km but this time a QSO could not be

completed. I didn’t notice many long bursts

during the shower this year either.”

Station Profile

Peter, G3MLO (JO01) has been QRV on 2m

for a number of years but over the past few

months he has been sending in details of the

home constructed items in his shack and a

excellent 4 Yagi antenna system (

Photo 1

)

to become QRV on moonbounce (EME). In

particular there is a high power MOSFET PA

central to the project.

“I am from an engineering background

and do not have much in the way of test gear

– only the essentials for building antennas

and other equipment. I decided to build a

high power LDMOS 2m amplifier from a

well tried and tested design, albeit with a

slight number of variations to the original by

F1JRD (

DUBUS

4/2010)

[3]

. After reading

all I could find on the subject I decided to

use kits from Jim, W6PQL after reading

the article in

QST

October 2012

[4]

. After

looking at the extensive lists of components

etc I decided to purchase a mixture of kits

and ready built items. The 2m RF deck,

the low pass filter/dual directional detector

board and the amplifier control board were

the assembled items. I suggest you to flow

solder the LDMOS device to the copper

heat spreader, giving much better cooling.

I designed and built the enclosure for the

amplifier and the separate power supply

and, as I have access to metal forming and

cutting equipment, this was easy to achieve.

The enclosures takes the form of trays and

using 4mm rivet nuts to form the cabinets,

the front panel was made to order by a local

engraving company (multilayer plastic). The

amplifier worked perfectly when testing, the

only problem I have encountered was the

failure of one of two 50V 20A switch mode

supplies that were operating in parallel.

Although equipped with the balance circuits

connected, one failed. These were of Chinese

origin. I have replaced these with a single

50V 42A SM supply (Mean Well RSP-2000).

The antenna system was decided as a 4 x

10 element Yagi array using the well known

and respected G4CQM WAXXX10 design.

With information taken from the websites of

Derek, G4CQM and Richard, G6HKS, both

of whom gave outstanding advice and tips in

the antennas construction

[5] [6]

.”

What’s On Your PC Screen?

Stations have been asking me ‘how to

anticipate conditions on VHF/UHF’ so they

can try and prepare or monitor such events.

With all the different PC applications to

monitor conditions, including a SDR system,

its is sometimes difficult to manage all the

windows while trying to search for the DX.

Many stations now use two screens to

expand the windows and reduce clutter and

actually concentrate on the main event – to

work DX. Considering applications like DX

Cluster, ON4KST Chat, JT65 EME Chat plus

solar and tropospheric information, how do

you collate all the information into an easily

manageable package? A one stop website

for all things VHF DX has been developed

over many years by the Make More Miles On

VHF (MMMONVHF) team

[7]

. Some of the

tools available are exceptional, particularly

the tropo propagation forecast map that

has been very accurate over the past few

months. Details of expeditions, meteor

and EME data are updated constantly.

After registering with the system, in the

download section a very handy DX CLIENT

which consolidates applications like DX

Cluster/KST/JT65B EME Chat all in one

window. Numerous configuration settings

allow customisation so you can filter out

unwanted DX spots etc.

Sign Off

Thanks to all contributors this month and

looking forward to good DX in 2016.

Websearch

[1]

www.bavarian-contest-club.de/

[2]

http://physics.princeton.edu/pulsar/k1jt/doc/wsjt/

[3]

www.qsl.net/f1jrd/MRFE6VP61K25H.html

[4]

www.w6pql.com/index.htm

[5]

http://g4cqm.www.idnet.com/

[6]

www.powabeamantennas.co.uk/G6HKS/

[7]

www.mmmonvhf.de/

The high power MOSFET PA central to the design of Peter, G3MLO’s moonbounce station.