OpenBCM V1.08-5-g2f4a (Linux)

Packet Radio Mailbox

IZ3LSV

[San Dona' di P. JN]

 Login: GUEST





  
G4TNU  > NEWS     01.04.12 02:08l 233 Lines 11957 Bytes #999 (0) @ EU
BID : 32952G4TNU
Read: GUEST
Subj: RSGB Main News - 01 Apr 2012
Path: IZ3LSV<I0OJJ<GB7CIP<GB7CIP<GB7CIP
Sent: 120401/0001Z @:GB7CIP.#32.GBR.EU $:32952G4TNU

T:From: G4TNU@GB7CIP.#32.GBR.EU <g4tnu@gb7ipf.ampr.org>
T:Newsgroups: ampr.news.europe
T:Message-Id: <E113623_G4TNU@gb7ipf.ampr.org>

GB2RS Main News for Sunday 1st April 2012

The news headlines:

* Did you know Ken Rowell G5RL?
* TEP observation beacons
* RSGB prepared to defend CW

Following the announcement a few months ago of the legacy from the 
late Ken Rowell, the Legacy Trustees, appointed to consider the way 
in which the bequest might be used, have held their first meeting. 
They are now asking for help from anyone who has any information on 
Ken Rowell, G5RL, his station, or any particular interests he had, 
that would help the Trustees to develop proposals on how his generous 
bequest could best be utilised. They are particularly anxious to 
obtain any photographs, letters or documents that would assist in 
this work. The Trustees are grateful for all the suggestions that 
have already been made regarding this legacy and will keep members 
informed of progress through RadCom. If you can help, please send any 
information to the Secretary to the Trustees, care of RSGB 
Headquarters, or to legacysecretary<at>rsgb.org.uk. 

There are two new beacons on air from Namibia for TEP observations. 
They are active 24 hours a day from JG82IE, callsign V51VHF. Listen 
out for the 35 watt CW signal on 70.005 that uses a DK7ZB beam headed 
North, and the 144.430MHz CW signal into a 10 element DK7ZB beam, 
also heading North.

Some say that CW has been made obsolete by modern digimodes, which 
work well in conditions far too poor for the older mode. Now that 
Morse is no longer used in commercial radio traffic, the RSGB 
confirms that it would fight any moves to prohibit CW on amateur 
bands. The Society recognises that Morse gives much pleasure to 
thousands of operators, and will continue to support its use. 

The Radio Security Service will hold its 16th reunion at Bletchley 
Park on Sunday 22 April in the Mansion Ballroom. Gates open at 10am 
and the meeting starts at 11am. All are welcome. The reunions are 
held to commemorate the 1,500-plus radio amateurs who used their 
special skills in the greatest secrecy in WW2 to monitor the German 
Secret Service, and thus facilitate numerous deceptions contributing 
to military successes, especially on D-Day. There will be a series of 
presentations and there will be the opportunity to visit Hut One to 
view the large collection of communication equipment from the past. 
Booking is not required, but it will be helpful if you can let Stan 
Ames know if you hope to attend. You can contact him by email to 
RSSreunion<at>aol.com. 

Ofcom has announced a GPS jamming exercise between 9 and 20 April 
near RAF Spadeadam in Cumbria. From 7am to 6pm there will be multiple 
jammers based within 5km of N55° 04.000' W002° 34.000', operating 
within the 24MHz band centred around 1575.42MHz. The total power used 
will be up to 10 watts EIRP. It is stressed that, as in previous 
exercises, Safety of Life operations will, at all times, take 
precedence over exercise activities.

The Spring Edition of The 5MHz Newsletter has now been published and 
features information on the recent WRC-12 conference. A subscription 
is not needed and the Newsletter can be freely read or downloaded 
from Google documents at http://tinyurl.com/7ylxz9z. A paper copy can 
be obtained by sending an SASE large enough to take folded A4 to the 
Editor, G4MWO, who is QTHR and on QRZ.com. A chart is also maintained 
of current Worldwide 5MHz Amateur Allocations. This can be found at 
http://tinyurl.com/82rwq2b 

On 24 March, sometime between 0230 and sunrise, in Kenninghall, 
Norfolk, Peter Lock, M0RYB had his red Land Rover Defender 90 X191 
FVC stolen. Inside was an Icom IC-7000, serial number 1002538. The 
crime Number is 12618/12/0. If anyone has any information on the 
whereabouts of the radio, or vehicle, please contact Peter via 
doc.lock<at>tesco.net so that he can pass the information onto the 
police.


And now for the details of rallies and events for the coming week

The Lough Erne Amateur Radio Club Annual Rally will take place today, 
1 April, at The Share Holiday Village, Lisnaskea, Co. Fermanagh 
BT92 0EQ. Doors open at 11.30am. There will be trade stands and a 
Bring & Buy. The RSGB President, Dave Wilson, M0OBW, will also be 
visiting the rally. Details from Iain on 02866 326 693.

Also today, 1 April, the South Gloucestershire Amateur Radio Rally 
will be held in the Scout Activity Centre, Woodhouse Park, 
Almondsbury, Bristol BS32 4LX. Doors open at 10am. There will be 
trade stands and a Bring & Buy. Talk in is on S22. More details from 
Stan Goodwin, G0RYM on 07833 517 370.

From 10 April the Titanic Centenary event will take place from 
Charterhouse, Godalming. GR100MGY will be active for 6 days. There is 
free admission and free car parking on 14 and 15 April, 12 to 4pm. 
Contact G0EFO at michaelgs1<at>talktalk.net.


Now for the news of special events

On 8 April, GB50WVR will be on the air from the Keighley & Worth 
Valley railway, which is celebrating 50 years of the Preservation 
Society. More information, including QSL details, is on qrz.com.

GB100MGY will be on the air from 6 to 26 April from Fort Perch Rock 
Marine Radio Museum, New Brighton, Wirral in commemoration of the 
Titanic. They also have special permission from Ofcom to use this 
callsign on the 501 to 504kHz band. They plan to transmit and receive 
on 502kHz and, for those without a 500kHz band NoV, it will be 
crossband on 3566kHz or 7066kHz as propagation conditions determine. 
More on www.gb100mgy-fortperchrock.co.uk. 

The centenary of the loss of RMS Titanic in 1912 will be commemorated 
with many activities taking place around the world, including a 
number in Godalming, Surrey, the birthplace of Titanic's Marconi 
Radio Officer, Jack Phillips. GR100MGY will be on the air from the 
grounds of Charterhouse school in Godalming. Operated by Wey Valley 
Amateur Radio Group, members of the public are invited to visit on 14 
and 15 April from noon until 4pm. Visitors should come to the school 
on Hurtmore Road, GU7 2DX, during these opening hours and simply 
follow the parking signs.


And now the HF DX news compiled from 425 DX News and other sources

ON4AEO and several other operators from Belgium and South Africa will 
be active as 3DA0FC from Swaziland on 6 to 10 April. They plan to 
operate SSB, RTTY and PSK on 10 to 80m bands. QSL via ON4CJK, direct 
or bureau. 

JA1XGI will be active as A35XG from Tongatapu, Tonga, which is IOTA 
reference OC-049,
on 2 to 9 April. Activity will be on the 10 to 30m bands, especially 
30, 17 and 12 metres using CW, SSB and digital modes. QSL via his 
home callsign, direct or via the bureau.

GM6TW will be operating from the Inner Hebrides, IOTA reference 
EU-008, from 7 to 13 April. The main QTH will be the Isle of Jura, 
but will also be activations from Islay and Colonsay. QSL via M0UTD.

PJ2/PA7JWC and PJ2/PD7DB will be on the air from Curacao, which is 
IOTA reference SA-099, on 2 to 9 April. They will operate SSB, CW, 
RTTY and PSK on the 10 to 80m bands. QSLs via Logbook of The World 
are preferred or via home callsigns, direct and via the bureau. 


Now the contest news

At 90 minutes in duration it may be a short contest, but make no 
mistake, the 1st RoPoCo contest today, 1 April, is quite challenging. 
The maximum permitted power is 100 watts with no QRP or high power 
categories. The basic format is that in your first QSO you send your 
full postcode and for all subsequent QSOs you send the postcode you 
received in your previous QSO. If you receive a postcode that you 
know is erroneous, for example a corrupted version of your own 
postcode, record it as received and give it to your next QSO partner 
as-is. Provided you are not the person to introduce an error, you'll 
get points for the QSO, because it is the accuracy of the exchange 
that is important. This all takes place on the 3.5MHz band from 1900 
to 2030UTC.

Activity on 70MHz continues to grow with the 1st 70MHz contest taking 
place today, 1 April, from 0900 to 1200UTC. Last year 156 stations 
took part from six different call areas. It's a race to accumulate as 
many kilometres worked as possible, with no multipliers. Using all 
modes the exchange is signal report, serial number and locator.

The latest CW leg of the 80m club championships takes place on 2 
April from 100 to 2030UTC. The exchange is signal report and serial 
number.

On 3 April the 144MHz UK Activity contest takes place from 1900 to 
2130UTC. Using all modes on the band the exchange is signal report, 
serial number and locator. 

The first leg of the SP DX Contest takes place on 7 and 8 April from 
1500 to 1500UTC. Using both CW and SSB on the 1.8 to 28m bands, SP 
stations send a signal report plus a single character province code, 
while non-SP stations send a signal report and a serial number. 


And now the solar factual data for the period from Friday the 23rd to 
the 29th of March, compiled by Neil Clarke, G0CAS on Friday the 30th 
of March.

Several small sunspot groups were visible every day. Only one group 
was large, which produced an M class solar flare on the 23rd, 
otherwise solar activity was at low levels every day with just a few 
C class solar flares taking place each day. However, on the 29th a 
large group was approaching the north-east limb and produced numerous 
large C class flares. This is the return of a region that produced 14 
M class and two X class solar flares on its last rotation during the 
first two weeks of March. Solar flux levels increased from 101 units 
on the 25th to 112 by the 29th. The average was 105 units. The 90 day 
solar flux average on the 29th was 119, that's three units down on 
last week. X-ray flux levels varied little day to day and averaged 
B2.5 units. Geomagnetic activity was quiet until a weak coronal hole 
disturbance arrived around midday on the 27th and lasted for 24 
hours. The Ap index on the 27th and the 28th was 15 units. The 
average was Ap 8 units. Solar wind data from the ACE spacecraft saw 
solar wind speeds increase from 330 kilometres per second on the 23rd 
to 510 by the 28th. Particle densities were low every day except for 
an increase to 20 particles per cubic centimetre by the 27th. Bz 
varied between minus 3 and plus 4 nanoTeslas and between minus 12 and 
6 nanoTeslas during the disturbance. MUFs fell below forecast levels 
on several days, this is due to the coronal hole disturbance and 
seasonal decline. A radio aurora event took place from the afternoon 
27th to the early hours of the 28th but contracts appear to have been 
confined to high latitudes.


And finally the solar forecast. This week the active side of the Sun 
is expected to be looking our way. Depending on how active the old 
region 1429 is, which is now back in view, that will determine the 
level of activity for the coming week. Moderate levels are a 
possibility. Solar flux levels should increase and be in the 130s 
later in the week. Geomagnetic activity should be quiet every day. 
However, there is a chance that later in the week activity could 
increase due to the arrival of a coronal mass ejection. MUFs during 
daylight hours at equal latitudes should be about 26MHz for the south 
and 23MHz for the north. Darkness hour lows should be around 10MHz. 
Paths this week to Australia should have a maximum usable frequency 
with a 50 per cent success rate of around 27MHz. The optimum working 
frequency with a 90 per cent success rate will be about 21MHz. The 
best time to try this path will be between 0900 and 1200 hours. 

And that's all for this week from the propagation team. 


And that's the end of the main news for this week prepared by the
Radio Society of Great Britain.  Items for inclusion in subsequent
bulletins can be emailed to  gb2rs<at>rsgb.org.uk to arrive by
10:00 on the Thursday before transmission.


Read previous mail | Read next mail


 08.09.2024 04:24:25lGo back Go up