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Biennial Report 2003-2004 - Merlin

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22<br />

Most of the engineering work in <strong>2003</strong> and <strong>2004</strong> was<br />

directed towards e-MERLIN developments, which are<br />

reported elsewhere. In addition to this, two major<br />

projects were undertaken (by our own staff) and one<br />

telescope was repainted (by contractors) during the<br />

<strong>2003</strong> and <strong>2004</strong> summer maintenance periods,<br />

together with a number of minor works such as the<br />

refurbishment of equipment cabins.<br />

D<br />

R EPL EPL EPLA EPL CEMENT CEMENT CEMENT OF OF DDEFF<br />

D EFF EFFORD EFF ORD<br />

C<br />

<strong>Biennial</strong> <strong>Report</strong> <strong>2003</strong>-<strong>2004</strong><br />

ORD & & M MMK<br />

M 2<br />

S<br />

T ELESCOPE ELESCOPE CCONTROL<br />

C ONTROL SSYSTEMS<br />

S YSTEMS<br />

Following the successful replacement of the obsolete<br />

control systems on the three E-Systems telescopes<br />

between 1999 and 2002, similar upgrades were<br />

implemented on the Defford and Mk2 telescopes in<br />

<strong>2003</strong> and <strong>2004</strong> respectively. Both of these telescopes<br />

date from the 1960s, and the amount of work<br />

involved in replacing the control systems was<br />

considerably greater than might be imagined, because<br />

it proved necessary to replace almost every cable,<br />

switch, etc. in order to meet current standards and<br />

ensure reliability (Figure 29).<br />

Figure 29: Some of the life expired material removed from the Defford telescope.<br />

P<br />

C O O R R R R O O S S I I O O O N N P R R O O T T E E C C T T I I O O N<br />

N<br />

The Pickmere telescope was painted by contractors<br />

in <strong>2004</strong> using one of the modern paint systems that<br />

have proved effective in doubling the recoating interval<br />

(from 5 to 10 years) at little extra cost. Despite these<br />

improved paint systems, inadequate funding is<br />

threatening the structural integrity of the telescopes<br />

by restricting the frequency of painting to a level<br />

below that regarded as optimum.<br />

MERLIN/VLBI National Facility<br />

ENGINEERING<br />

ENGINEERING<br />

Figure 30: A new e-MERLIN C-band feed fitted on the<br />

Mk2 and Defford antennas.<br />

Figure 31: An L-band feedhorn being installed on a<br />

MERLIN E-Systems telescope.

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