MERLIN

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The Multi-Element Radio Linked Interferometer Network (MERLIN) is an Interferometer array of radio telescopes spread across England and the Welsh borders. The array is run from Jodrell Bank Observatory in Cheshire by the University of Manchester on behalf of PPARC as a National Facility.

The array consists of up to seven radio telescopes and includes the Lovell Telescope, Mark II, Cambridge, Defford, Knockin, Darnhall and Pickmere (previously known as Tabley). The longest baseline is therefore 217km and MERLIN can operate at frequencies between 151 MHz and 24 GHz. At a wavelength of 6 cm (5 GHz frequency), MERLIN has a resolution of 40 milliarcseconds which is comparable to that of the HST at optical wavelengths.[citation needed]

Some of the telescopes are occasionally used for EVN and VLBI observations in order to create an interferometer with even larger baselines, providing images with much greater angular resolution.

Contents

[edit] MTLRI

The radio telescope at Knockin
The radio telescope at Knockin
Original MTRLI telescopes
Name Coordinates
(links to map & photo sources)
Lovell Telescope 53°14′10.50″N 02°18′25.74″W / 53.23625, -2.30715 (Lovell Telescope)
Mark II 53°13′51.62″N 02°18′34.16″W / 53.2310056, -2.3094889 (Mark II)
Mark III 53°06′09.16″N 02°31′15.63″W / 53.1025444, -2.5210083 (Mark III)[1]
Defford 52°05′27.61″N 02°08′09.62″W / 52.0910028, -2.1360056 (Defford)
Knockin 52°47′23.9″N 02°59′44.9″W / 52.789972, -2.995806 (Knockin)
Pickmere 53°17′18.4″N 02°26′38.4″W / 53.288444, -2.444 (Pickmere)
Darnhall 53°09′21.6″N 02°32′03.3″W / 53.156, -2.53425 (Darnhall)

In 1973, Henry Palmer made the suggestion of extending the interferometer links already in place at Jodrell Bank at the time, which started the planning of the telescope array.[2][3] Construction started in 1975.[3] The system was originally officially called MTRLI (Multi-Telescope Radio Linked Interferometer), but was commonly referred to by the simpler name of MERLIN. It originally consisted of either the 76m Lovell Telescope or the 25m Mark II, along with the 25m Mark III at Wardle, the 85ft at Defford and a new telescope at Knockin. This new telescope was made by E-Systems and was constructed based on the designed for the telescopes in the Very Large Array, which was being constructed at the same time also by E-Systems.[4][5]

The construction of the new telescope, the installation of microwave communication links and the construction of the correlator were jointly called "Phase 1" of the MERLIN project, the funding for which was approved on 30 May 1975[6]. The construction of the new telescope started on 9 July 1976, and was completed by 8 October 1976. The telescope was first controlled remotely from Jodrell in January 1977.[7] The microwave links were installed in May 1978.[8] The first observations using the system - measurements of 30 distant radio sources - were taken in January and February 1980.[9] The final cost of phase 1 of the system was £2,179,000 (1976).[9]

Two additional telescopes were added in Phase 2 of the project, along with their radio links to Jodrell Bank. While it was originally proposed that one of the telescopes would be sited at Jodrell Bank and the other at Darnhall, the pair were finally sited at Pickmere (also known as Tabley) and Darnhall. The two telescopes were the same as that at Knockin. Construction on both telescopes started on 9 April 1979, and was completed by 31 October 1979. The Pickmere telescope was connected into MTRLI for the first time on 20 July 1980, followed by the Darnhall telescope on 16 December 1980. The second phase was formally completed on the 31 December 1981, and had cost £3,142,210.[10]

The longest baseline of MTRLI was 134km, between Pickmere and Defford.[4] The first map produced by the array was published on 6 November 1980[3]. In the first 2 years of operation (1980-1982), the array was used to observe at frequencies of 408MHz (with a resolving power of 1 arcsecond), 1666MHz (0.25 arcsecond) and 5GHz (0.08 arcsecond).[11]

When the Mark II's surface was replaced in 1987, it could be used along with the three E-systems telescopes on the 22GHz frequency, expanding MTRLI at that frequency.[4]

[edit] MERLIN

Current MERLIN telescopes
Name Coordinates
(links to map & photo sources)
Lovell Telescope 53°14′10.50″N 02°18′25.74″W / 53.23625, -2.30715 (Lovell Telescope)
Mark II 53°13′51.62″N 02°18′34.16″W / 53.2310056, -2.3094889 (Mark II)
Defford 52°05′27.61″N 02°08′09.62″W / 52.0910028, -2.1360056 (Defford)
Knockin 52°47′23.9″N 02°59′44.9″W / 52.789972, -2.995806 (Knockin)
Pickmere 53°17′18.4″N 02°26′38.4″W / 53.288444, -2.444 (Pickmere)
Darnhall 53°09′21.6″N 02°32′03.3″W / 53.156, -2.53425 (Darnhall)
Cambridge 52°10′1.2″N 0°2′13.4″E / 52.167, 0.037056 (Cambridge)

MTRLI was renamed to MERLIN in the early 1990s, and shortly afterwards the addition of the Cambridge antenna in 1991 increased both the sensitivity and angular resolution of the array. The array also had a new correlator and new, cooled receivers, and some of the microwave links between the telescopes were improved so that the array could observe both hands of polarization.[12]

Since 1996, carousels for the different receivers on each of the E-systems telescopes and the Mark II telescope were installed (the Cambridge telescope already had such a system installed), providing frequency agility. In 1997 and 1998, dual-frequency (5 and 22GHz) observations were made with the array for the first time.[12]

There are plans to construct a telescope in Ireland that would be added to the array.[13]

[edit] e-MERLIN

MERLIN currently uses microwave links to send astronomical data back from the remote stations. These links have a limited bandwidth so much of the data is thrown away. In order to increase the sensitivity of the telescope the current links are being replaced by optical fibre links which will carry a bandwidth of 4 GHz, compared to the current limit of 30 MHz, increasing the sensitivity of the array by a factor of around 30. This vast increase in data means that the old correlator will no longer be able to cope, so a new correlator is under construction which will be capable of processing over 200 Gbit/s.[citation needed]

Another major development which is part of the upgrade is frequency flexibility - the ability to alter the observing band of the entire array in a matter of minutes using rotating carousels of receivers. Some telescopes in the array already have this capability, while the rest require the visit of an engineer to change the receiver. When e-MERLIN becomes operational the telescope will be able to switch rapidly between 1.4, 5, 6 and 22 GHz. This is required in order to take advantage of optimum conditions for high frequency observations where atmospheric conditions can severely affect results.[citation needed]

Work started on the e-MERLIN upgrade in May 2004.[14]

On 6 March 2008 The Science and Technology Facilities Council announced that the project was at risk because of a £80m shortfall in its budget. Additionally, an assessment panel had listed the project as a "lower priority" for UK physics and astronomy. A Jodrell Bank spokesman said it opposed any cut backs and would push for eMerlin to keep its funding.[15]

[edit] Scientific results

Among many other things, MERLIN has been used to observe:

  • Radio-loud galaxies, for example Messier 87.[11]
  • Quasars, for example 3C 418.[16]
  • Spectral line observations of Hydroxyl (OH) in interstellar gas clouds.[17]

The telescope can also be used for highly precise astrometry.[18]

In 1998, MERLIN in conjunction with the Hubble Space Telescope discovered the first Einstein ring.[19]

[edit] References

  1. ^ MERLIN user guide - 4.1 Location of Telescopes. Retrieved on 2007-08-04.
  2. ^ Lovell, Jodrell Bank Telescopes, p. 184
    Lovell, Astronomer by Chance, p. 312
  3. ^ a b c Davies et al. (1980)
  4. ^ a b c JBO - MTRLI. Retrieved on 2007-06-10.
  5. ^ Lovell, Jodrell Bank Telescopes, p. 185
  6. ^ Lovell, Jodrell Bank Telescopes, p. 191
  7. ^ Lovell, Jodrell Bank Telescopes, p. 201
  8. ^ Lovell, Jodrell Bank Telescopes, p. 203
  9. ^ a b Lovell, Jodrell Bank Telescopes, p. 204
  10. ^ Lovell, Jodrell Bank Telescopes, Chapter 20 (pp. 208–215)
  11. ^ a b Lovell, Jodrell Bank Telescopes, p. 220
  12. ^ a b JBO - MERLIN. Retrieved on 2007-06-10.
  13. ^ "Irish giant could get new partner", BBC News, 2 October 2000. Retrieved on 2007-04-06. 
    A Radio Telescope for Ireland. Retrieved on 2007-04-06.
  14. ^ Giant UK telescope gets upgrade. BBC News (26 May 2004). Retrieved on 2007-04-05.
  15. ^ [ http://news.bbc.co.uk/1/hi/england/manchester/7281176.stm Jodrell Bank fears funding loss]
  16. ^ Lovell, Jodrell Bank Telescopes, p. 221
  17. ^ Lovell, Jodrell Bank Telescopes, p. 224
  18. ^ Lovell, Jodrell Bank Telescopes, p. 226
  19. ^ A Bull's Eye for MERLIN and the Hubble. Retrieved on 2007-06-10.

[edit] Journals

  • Davies, J. G.; et al. (1980). "The Jodrell Bank radio-linked interferometer network" 288: 64–66. Nature. doi:10.1038/288064a0. 

[edit] Books

[edit] External links