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2004 ASTRONOMY & ASTROPHYSICS - Indian Academy of Sciences

2004 ASTRONOMY & ASTROPHYSICS - Indian Academy of Sciences

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CHAPTER 5<br />

• Participation in the next generation<br />

international projects<br />

The next generation radio telescopes will be so<br />

large, and therefore so expensive, that they will<br />

almost certainly be built by an international<br />

collaboration. The planning for the large Low<br />

Frequency Array (LOFAR) and the Square<br />

Kilometre Array Interferometer (SKAI) bears<br />

testimony to this.<br />

The <strong>Indian</strong> radio astronomy community has<br />

received considerable international recognition<br />

for its past effort, culminating in the building <strong>of</strong><br />

the GMRT. In order to retain this position <strong>of</strong><br />

eminence, we must participate in the big<br />

international projects. India is already<br />

represented on the ISSC (International Square<br />

Kilometre Array Steering Committee). A<br />

conscious decision should soon be made<br />

to identify areas where we could develop<br />

the necessary expertise to be able to<br />

contribute something concrete to such<br />

projects, and thereby become partners.<br />

An artist’s impression <strong>of</strong> a 500 metre aperture spherical<br />

telescope (FAST) proposed to be built in southwest<br />

China. This is being projected as a prototype for the<br />

SKA by the Chinese <strong>Academy</strong> <strong>of</strong> <strong>Sciences</strong>.<br />

The Large Adaptive Reflector ( LAR ) is the Canadian<br />

concept for a large steerable telescope. It will<br />

consist <strong>of</strong> a long focal length, large diameter<br />

parabolic reflector, composed <strong>of</strong> actuated reflector<br />

panels controlled by a computer. The second<br />

component is a focal package at a height <strong>of</strong> 500<br />

metres, on a large helium balloon platform.<br />

The picture shows an artist’s impression <strong>of</strong> one SKA<br />

station composed <strong>of</strong> 400 Luneburg Lens antennas,<br />

each 5 metre in diameter. It will form many<br />

simultaneous, widely spaced, beams on the sky.<br />

More than 100 such stations will be required for the<br />

SKA. This is one <strong>of</strong> the several concepts being<br />

investigated by CSIRO, Australia.<br />

One <strong>of</strong> the options for a SKA is to use phased arrays<br />

with over 50 million receiving elements with a<br />

mixed RF/digital adaptive beam former.<br />

The Thousand Element Array ( THEA ) is one <strong>of</strong> the<br />

demonstrator systems built by ASTRON in the<br />

Netherlands. The image shows four THEA tiles, each<br />

consisting <strong>of</strong> 64 wide-band antennas.<br />

69

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