Non-U.S. Radio Astronomy Observatories
Please send corrections or updates to bpa@nas.edu
Argentina--Instituto Argentino de
Radioastronomia
Australia--Molonglo Observatory Synthesis
Telescope
Australian National Radio Astronomy
Observatory, Parkes
Australia Telescope Compact Array,
Narrabri
Australia--Wiruna Telescope Project
Belgium--Humain Radio Astronomical Station
7.5 m
Belgium--Humain Radio Astronomical Station
Interferometer
Brazil--Forteleza Observatory
Brazil--Itapetinga Radio Observatory
Canada--Dominion Radio Astrophysical
Observatory 26 m
Canada--Dominion Radio Astrophysical
Observatory Synthesis Telescope
China--High Time Resolving Solar Radio
Telescope, Nanjing
China--Yunnan Solar Observatory
China--Purple Mountain 0.4 m
China--Purple Mountain 13.7 m
China--Purple Mountain 1.5 m
China--Purple Mountain 2 m
Czech Republic--Ondrejov
Astronomical Observatory 3 m
Czech Republic--Ondrejov
Astronomical Observatory 7.5 m
Czech Republic--Ondrejov
Astronomical Observatory 7.5 m (with spectrograph)
Finland--Metsähovi Radio Research
Station
Finland--European Incoherent Scatter Facility
(EISCAT) Scientific Association (32-m dishes
France--Instituto de Radio Astronomia
Millimetrica (IRAM)
France--Observatoire de l'Université
de Bordeaux, POM 1 Telescope
France--Observatoire de Grenoble,
C.E.R.M.O., POM 2 Telescope
France--Observatoire du Plateau de Bure
France--Station de Radioastronomie de Nancay
(16-element network) Observatoire de Paris-Meudon
France--Station de Radioastronomie de Nancay
(18-element network) Observatoire de Paris-Meudon
France--Station de Radioastronomie de Nancay
(24-paraboloid network) Observatoire de Paris-Meudon
France--Station de Radioastronomie de Nancay
(dual reflecting antenna) Observatoire de Paris-Meudon
France--Station de Radioastronomie de Nancay
(log-periodic antennas) Observatoire de Paris-Meudon
Georgia--Abastumani Astrophysical
Observatory
Germany--Radioobservatorium Effelsberg
Germany--Observatorium für Solare
Radioastronomie
India--Gauribidanur Low-Frequency Array
India--Giant Metrewave Radio Telescope
India--Mauritius Radio Telescope
India--Ooty Radiotelescope and Synthesis
Radiotelescope
Italy--Stazione Radioastronomica di Medicina
(transit instrument)
Italy--Stazione Radioastronomica di Medicina
(32-m telescope)
Italy--Trieste Astronomical Observatory,
Basovizza Solar Radio Telescope
Japan--Hiraiso Solar Terrestrial Research
Center
Japan--Solar-Terrestrial Environment Laboratory
UHF Radio Telescope, Nagoya
Japan--Kashima Space Research Center
Japan--Kisarazu College Observatory
Japan--Nobeyama Radio Observatory (45-m
telescope)
Japan--Nobeyama Radio Observatory (5-element
interferometer)
Japan--Nobeyama Radio Observatory
(16-element interferometer)
Japan--Nobeyama Radio Observatory (8- and
6-m telescopes)
Japan--Nobeyama Radio Observatory
(17-element interferometer)
Japan--Nobeyama Radio Observatory
(3-paraboloid telescope)
Japan--Toyokawa Observatory 0.85 m
Japan--Toyokawa Observatory 1.5 m
Japan--Toyokawa Observatory 2.0 m
Japan--Toyokawa Observatory 3.0 m
Japan--Toyokawa Observatory small array
Japan--Toyokawa Observatory large array
Mexico--Large Millimeter Telescope
Mexico--Tonantzintla Solar Radio
Interferometer
Mexico--UNAM Solar Radio Interferometer
Netherlands--Dwingeloo Radio
Observatory
Netherlands--Westerbork Synthesis
Radio Telescope
Norway--European Incoherent Scatter Facility
(EISCAT) Scientific Association (32-m dishes
Russia--Ratan-600 Special Astrophysical
Observatory
South Africa--Hartebeesthoek Radio
Astronomy Observatory
South Korea--Taeduk Radio Astronomy
Observatory
Spain--Observatorio del Ebro
Spain--Instituto de Radio Astronomia
Millimetrica (IRAM)
Sweden--ESO Submillimeter Telescope
Sweden--Onsala Space Observatory
Sweden--European Incoherent Scatter Facility
(EISCAT) Scientific Association (32-m dishes
Sweden--European Incoherent Scatter Facility
(EISCAT) Svalbard Radar
Sweden--European Incoherent Scatter Facility
(EISCAT) Scientific Association (parabolic cylinders
Switzerland--Bleien Radio Astronomy
Observatory (5-m telescope)
Switzerland--Bleien Radio Astronomy
Observatory (7-m telescope)</
Tasmania--Ceduna Radio Astronomy Observatory
Tasmania--Mount Pleasant Radio
Observatory (14-m telescope)
Tasmania--Mount Pleasant Radio
Observatory (26-m telescope)
UK--Chilbolton Observatory
UK--James Clerk Maxwell Telescope
UK--Nuffield Radio Astronomy Laboratories,
Jodrell Bank (42-ft telescope)
UK--Nuffield Radio Astronomy Laboratories,
Cambridge 32-m paraboloid
UK--Nuffield Radio Astronomy Laboratories,
Darnhall
UK--Nuffield Radio Astronomy Laboratories,
Defford
UK--Nuffield Radio Astronomy Laboratories,
Knockin
UK--Nuffield Radio Astronomy Laboratories,
Lovell telescope
UK--Nuffield Radio Astronomy Laboratories,
Jodrell Bank (Mk II)
UK--Nuffield Radio Astronomy Laboratories,
Pickmere
Ukraine--URAN-1 Interferometer
Ukraine--URAN-3 Interferometer
Ukraine--URAN-4 Interferometer
Ukraine--UTR-2 Array
European Incoherent Scatter Facility (EISCAT)
Scientific Association (32-m dishes)
European Incoherent Scatter Facility (EISCAT)
Svalbard Radar
European Incoherent Scatter Facility (EISCAT)
Scientific Association (parabolic cylinders
Europe--Instituto de Radio Astronomia
Millimetrica (IRAM)
Casilla de Correo No. 5
(1984) Villa Elisa
Prov. de Bs. As., Argentina
Phone: (021) 4-3793 (021) 87-0230
Contact: Fernando R. Colomb
Sponsor: Consejo Nacional de Investigaciones Cientificas y Tecnicas
Reference: Thonnard N., 1980, Carnegie Institution of Washington,
Yearbook 79, 581
Location: Parque Pereyra Iraola
Latitude: -34° 52.1´
Longitude: +58° 08.2´
Telescope: Two steerable paraboloids
Diameter: 30 m
Area: 350 m2
Remarks: Periodic scheduling
Observation Type: HI, recombination lines, OH, continuum
Frequency band(s):
1420 MHz*
1605 MHz*
1612 MHz*
1667 MHz*
1720 MHz*
1415 MHz**
*antenna one
**antenna two (continuum)
Department of
Astrophysics
University of Sydney
NSW 2006, Australia
Contact: A.J. Green
Reference: Mills, B. Y., Proc. Astron. Soc. Aus. 4, 156 (1981)
Location: Hoskinstown, NSW, Australia
Latitude: -35° 22´ 18.97´´
Longitude: 149° 25´ 25.25´´ E
Altitude: 732 m
Telescope: 1570 x 11.6 m E-W cylindrical paraboloid; mechanical
steering ±55° about long axis, electrical phase/delay
±60° about short axis (alt.-az. mount). Earth rotation
aperture synthesis using rotation of fan beams.
Area: 18,040 m2
Coverage: Full synthesis at dec. < -30°, partial synthesis
at -30° to 20° dec.
Remarks: Survey of the southern sky to commence 1997
Observation Type: Continuum; galactic, extragalactic, solar
Frequency band(s):
843 MHz
CSIRO
Australia Telescope National Facility
P.O. Box 276
Parkes, NSW 2870, Australia
Phone: (068) 61 1700
Contact: Dr. R.M. Price
Sponsor: CSIRO (Australian Government)
Location: Parkes, NSW, Australia,
Latitude: 32° 59´ 59.8´´ S
Longitude: 148° 15´ 44.3´´ E
Altitude: 391.8 m
Telescope: Steerable paraboloid
Diameter: 64 m
Area: 3200 m2
Height: 60 m
Coverage: 0°-360° az., 30°-90° el.
Remarks: One of the three sites operated by CSIRO Australia Telescope
National Facility. See entry on the Australia Telescope Compact Array.
Observation Type: Pulsar,
Continuum,
Spectral line
VLBI
Frequency band(s):
418-454 MHz
642-678 MHz
1250-1750 MHz
2200-2500 MHz
4.5-5.0 GHz
5.95-6.25 GHz
6.45-6.75 GHz
8.15-8.65 GHz
12.0-12.4 GHz
12.5-15.5 GHz
21.5-23.5 GHz
CSIRO
Paul Wild Observatory
Locked Bag 194
Narrabri, NSW, 2390, Australia
Phone: +61 67 90 4000
Sponsor: CSIRO
Reference: Journal of Electrical and Electronics Engineering 12 2 (1992)
Location: NSW, Australia
Latitude: -30° 18´ 52.048´´ S
Longitude: 149° 32´ 56.327´´ E
Altitude: 207.780 m
Telescope: Steerable paraboloid, alt.-az. mounted
Diameter: 22 m
Area: 2200 m2
Coverage: 0°-360° az., 12°-90° el.
Remarks: Six 22-m steerable paraboloid telescopes located near
Narrabri, form the Compact Array: five telescopes can be positioned
along a 3-km track, with a sixth at a fixed site 3 km west of the
track. One or more of the antennas of the Compact Array may be linked
to the 22-m paraboloid at Mopra near Coonabara or the Parkes telescope
to form a very long baseline array with a maximum diameter equivalent
to a 320-km dish. This network is linked to other facilities across
Australia and, in 1997 to the VSOP orbital radio telescope.
Observation Type: Earth rotation aperture synthesis and VLBI.
Continuum, spectral line and pulsar gating. Frequency switching, band
switching, and mosaicing.
Frequency band(s):
1250-1760 MHz
2200-2500 MHz
4.4-6.1 GHz
8.0-9.2 GHz
20-25.5 GHz
42-50 GHz
84-98.5 GHz
105-116 GHz
The Astronomical
Society of New South Wales, Inc.
NSW, Australia
Location: Ilford, NSW
Telescope: 5 m
Frequency band(s):
1420 MHz
Remarks: Facility is under development.
Observatoire Royal de
Belgique
B 1180 Brussels, Belgium
Phone: (02) 375 24 84
Contact: Roger Gonze
Sponsor: Ministere de l'Education Nationale
Location: Humain, Belgium
Latitude: 50° 11´ 31´´ N
Longitude: 05° 15´ 19´´ E
Altitude: 293 m
Telescope: Steerable paraboloid
Diameter: 7.5 m
Area: 28 m2
Height: 1 m
Coverage: 0°-360° az., 0°-90° el.
Observation Type: Solar
Frequency band(s):
600 MHz
Observatoire Royal de
Belgique
Avenue Circulaire 3
B 1180 Brussels, Belgium
Phone: (02) 375 24 84
Contact: Roger Gonze
Sponsor: Ministere de l'Education Nationale
Location: Humain, Belgium
Latitude: 50° 11´ 31´´ N
Longitude: 05° 15´ 19´´ E
Altitude: 293 m
Telescope: 48-antenna equatorial-mount interferometer (E-W, N-S)
Diameter: 4 m
Area: 48 x 7 m2
Height: 1 m
Coverage: 50°-310° az., 0°-65° el.
Observation Type: Solar
Frequency band(s):
408 MHz
ROEN-INPE/CRAAE
Rua Jose Hipolito S/N, Bairro Tupuiu
61760-000 Eusebio
CE, Brazil
Contact: P. Kaufmann
Sponsor: Same as operator
Reference:LBI Technology, Proc. URSI/IAU Kyoto Symposium (1994)
Location: Eusebio, near Fortaleza, CE
Latitude: 3° 52´ 39´´ S
Longitude: 38° 25´ 31.84´´ W
Altitude: 26.62 m
Observation Type: Dedicated to geodetic VLBI, within an agreement with
NGS/NOAA (USA)
Frequency band(s):
2.6 GHz
8.8 GHz
Centro de Radio
Astronomia e Aplicacoes Espacias (CRAAE)
(USP, INPE, Mackenzie, UNICAMP)
CRAAE/EPUSP/PTR
SP, Brazil
Contact: P. Kaufmann
Sponsor: Same as operator
Reference: Solar Physics 78, 389 (1982)
Sky and Telescope 45, 144 (1973)
IEEE Trans. Ant. Prop. AP-26, 854 (1978)
Location: Atibaia, SP
Latitude: 23° 11´ 5.077´´ S
Longitude: 46° 33´ 28.428´´ W
Altitude: 805 m
Telescope: Steerable paraboloid, radome-enclosed, cassegrain, el.-az.
mount
Diameter: 13.7 m
Area: 73.7 m2 at 0.50 eff. (44 GHz)
36.8 m2 at 0.25 eff. (94 GHz)
Height: 27-m radome
Coverage: 0°-360° az., 2°-90° el.
Remarks: Scheduling established by program committee. Time available
for both Brazilian and international parties.
Observation Type: Solar, galactic, extragalactic, continuum and line
works, and VLBI astrophysics and geodetics, at 48 GHz multiple-beam
solar observations only (cooperation with Bern University,
Switzerland). Frequency band(s):
10.7 GHz - 22 GHz
30 GHz
44 GHz
48 GHz
94 GHz
National Research
Council of Canada
Herzberg Institute of Astrophysics
P.O. Box 248
Penticton, B.C., V2A 6K3, Canada
Sponsor: Canadian Federal Government
Reference: Astron. J. 93, 747 (1987)
Location: Penticton, B.C., Canada
Latitude: 49° 19´ 12´´ N
Longitude: 119° 37´ 12´´ W
Altitude: 545 m
Telescope: Fully steerable paraboloid
Diameter: 26 m
Area: 290 m2 at 0.55 eff.
Height: 28 m
Coverage: 0°-360° az., 0°-90° el.
Observation Type: Spectroscopy of HI and OH, 1.6-GHz VLBI
Frequency band(s):
1500 MHz (includes 1420 MHz, 1610 MHz, 1660 MHz, 1665 MHz)
National Research
Council of Canada
Herzberg Institute of Astrophysics
P.O. Box 248
Penticton, B.C., V2A 6K3, Canada
Sponsor: Canadian Federal Government
Reference: Proc. IEEE 61, 1270 (1973)
Radio Sci. 20, 1118 (1985)
Location: Penticton, B.C., Canada
Latitude: 49° 19´ 12´´ N
Longitude: 119° 37´ 12´´ W
Altitude: 545 m
Telescope: Earth-rotation synthesis, seven steerable paraboloids
Diameter: 8.5 m
Area: 64 m2 at 0.55 eff. (individual antenna)
Height: 11 m
Coverage: 0°-360° az., 0°-90° el.
Remarks: Operated as a national facility
Observation Type: Continuum and HI spectroscopy
Frequency band(s):The DRAO Synthesis Telescope is a wide-field
telescope that operates simultaneously in continuum bands at 408 MHz
(74 cm) and at 1420 MHz (21 cm) and in 256 channels on the spectral
line of atomic hydrogen at 21 cm.
Nanjing University
Astronomy Department
Nanjing 210093, Jiangsu Province, China
37651-2882
Contact: Zhi-Hai Qin
Sponsor: Chinese National Science Foundation
Location: Nanjing, Jiangsu Province
Latitude: 32° 03´ 26´´ N
Longitude: 118° 46´ 07´´ E
Altitude: 120 m
Telescope: Steerable paraboloid
Diameter: 2 m
Height: 2.5 m
Coverage: 0°-360° az., 15°-90° el.
Remarks: Periodic scheduling
Observation Type: Solar
Frequency band(s):9.375 GHz
Academia Sinica
P.O. Box 110
Kunming, China 72946
Contact: Yang Rongbang and Ji Shuchen
Reference: PYO 3, 64 (1979); Scientia Sinica 11, 1196 (1986 A)
Location: Phoenix Hill, Kunming
Latitude: 25° 02´ N
Longitude: 102° 47´ E
Altitude: 2014 m
Telescope: Steerable paraboloid
Diameter: 2.5, 3.0, 3.2, and 10 m
Area: 3, 4, 5, and 47 m2 (all at 0.60 eff.), respectively
Height: 6, 6, 8, and 14 m
Coverage: ±110° az., 10°-90° el.
Remarks: Daily
Observation Type: Solar
Frequency band(s):
2902 MHz
1420 MHz
3653 MHz
1426 MHz and 230-300 MHz
Purple Mountain
Observatory
Nanjing, Jiangsu Province, China 33738
Contact: Wu Hong-So
Sponsor: The Chinese Academy of Sciences
Location: Nanjing, Jiangsu Province
Latitude: 32° 04´ N
Longitude: 118° 49´ 12´´ E
Altitude: 267 m
Telescope: Steerable paraboloid
Diameter: 0.4 m
Area: 0.075 m2 at 0.60 eff.
Height: 0.1 m
Coverage: 0°-360° az., 15°-90° el.
Observation Type: Solar radio emission (total intensity)
Frequency band(s):
3500 MHz
Purple Mountain
Observatory
Nanjing, Jiangsu Province, China 33738
Contact: Fu Han
Sponsor: The Chinese Academy of Sciences
Location: Delingha, Qing-Hai Province
Latitude: 37° 22´ N
Longitude: 97° 44´ E
Altitude: 3200 m
Telescope: Steerable paraboloid
Diameter: 13.7 m
Coverage: 0°-720°, 10°-85°
Observation Type: Continuum and spectral line
Frequency band(s):
85-115 GHz
Purple Mountain
Observatory
Nanjing, Jiangsu Province, China 33738
Contact: Wu Hong-so
Sponsor: The Chinese Academy of Sciences
Location: Nanjing, Jiangsu Province
Latitude: 32° 04´ N
Longitude: 118° 49´ 12´´ E
Altitude: 267 m
Telescope: Steerable paraboloid
Diameter: 1.5 m
Area: 1.06 m2 at 0.60 eff.
Height: 0.5 m
Coverage: 0°-360° az., 15°-90° el.
Observation Type: Solar radio emission (total intensity)
Frequency band(s):
2700 MHz and 9375 MHz
Purple Mountain
Observatory
Nanjing, Jiangsu Province, China 33738
Contact: Wu Hong-so
Sponsor: The Chinese Academy of Sciences
Location: Nanjing, Jiangsu Province
Latitude: 32° 04´ N
Longitude: 118° 49´ 12´´ E
Altitude: 267 m
Telescope: Steerable paraboloid
Diameter: 2 m
Area: 1.88 m2 at 0.60 eff.
Height: 0.5 m
Coverage: 0°-360° az., 15°-90° el.
Observation Type: Solar radio emission (total intensity)
Frequency band(s):
5000 MHz
Astronomical Institute
of the Czech Republic Academy of Sciences
251 65 Ondrejov, Czech Republic
Contact: A. Tlamicha
Sponsor: Czech Republic Academy of Sciences
Reference: Astron. Astrophys. Suppl.
Ser. 44, 165 (1981)
Location: Ondrejov, Czech Republic
Latitude: 49° 54´ 38´´ N
Longitude: 14° 47´ 01´´ E
Altitude: 525 m
Diameter: 3 m
Area: 4.9 m2 at 0.60 eff.
Height: 1 m
Coverage: Equatorial
Remarks: For daily solar observation
Observation Type: Daily
Frequency band(s):
3 GHz
2-4 GHz
Astronomical Institute
of the Czech Republic Academy of Sciences
251 65 Ondrejov, Czech Republic
Sponsor: Czech Republic Academy of Sciences
Reference: Bull. Astron. Inst. Czech. 18, 163 (1974)
Location: Ondrejov, Czech Republic
Latitude: 49° 54´ 38´´ N
Longitude: 14° 47´ 01´´ E
Altitude: 525 m
Telescope: Steerable paraboloid
Diameter: 7.5 m
Area: 54 m2 at 0.50 eff.
Height: 1 m
Coverage: 0°-360° az., 0°-90° el.
Remarks: For solar observation, all frequencies in one paraboloid
Observation Type: Daily
Frequency band(s):
260 MHz
536 MHz
808 MHz
Astronomical Institute
of the Czech Republic Academy of Sciences
251 65 Ondrejov, Czech Republic
Sponsor: Czech Republic Academy of Sciences
Reference: Bull. Astron. Inst. Czech. 18, 163 (1974)
Location: Ondrejov, Czech Republic
Latitude: 49° 54´ 38´´ N
Longitude: 14° 47´ 01´´ E
Altitude: 525 m
Telescope: Steerable paraboloid
Diameter: 7.5 m
Area: 54 m2 at 0.50 eff.
Height: 1 m
Coverage: 0°-360° az., 0°-90° el.
Remarks: Solar radio spectrograph for daily observations
Observation Type: Daily
Frequency band(s):
100-1200 MHz
Helsinki University of
Technology, Radio Laboratory
Otakaari 5 A, 02150 Espoo, Finland
Phone: +358-0-4342248
Contact: Seppo Urpo
Sponsor: Academy of Finland
Reference: Astrophys. J. 308, 78 (1986)
Location: Metsähovi, Kylmälä
Latitude: 60° 13´ 04´´ N
Longitude: 24° 23´ 17´´ E
Altitude: 60 m
Telescope: Steerable dish
Diameter: 13.7 m
Area: 81 m2 at 0.55 eff.
Coverage: 0°-360° az., 0°-90° el.
Remarks: Periodic scheduling
Observation Type: Solar and extragalactic continuum on all three
frequencies, galactic lines on 22.2 and 75-115 GHz.
Frequency band(s):
22.2 GHz
37.6 GHz
75-115 GHz
Observatoire de
l'Université de Bordeaux
I BP 21 33270 Floirac, France
Sponsor: CNRS and Ministere de l'Education Nationale
Reference: Baudry et al., Astron. Astrophys. 104, 101 (1981)
Latitude: +44° 50´ 10´´ N
Longitude: 00h 02min 06.5s W
Altitude: 73 m
Telescope: Steerable paraboloid
Diameter: 2.5 m
Area: 2.5 m2
Coverage: 0°-360° az., 10°-88° el.
Observation Type: Spectral line observations: in our galaxy (dark
clouds, HII regions, large-scale surveys), in the terrestrial
atmosphere (ozonosphere, mesosphere)
Frequency band(s):
100 GHz (75 to 120 GHz)
Observatoire de
Grenoble, C.E.R.M.O.
BP 68, F-38402
Saint Martin d'Heres Cedex, France
Sponsor: Université Grenoble I and CNRS (Insu)
Location: Plateau de Bure, France
Latitude: 5° 54´ 27´´ E
Longitude: 44° 38´ 02´´
Altitude: 2552 m
Telescope: Cassegrain paraboloid
Diameter: 2.5 m
Area: 6.2 m2
Height: 1.5 m
Coverage: -180° to +180°, +10° to 90°
Remarks: 256 channel autocorrelator--600 MHz bandwidth
Observation Type: Mainly CO isotopes
Frequency band(s):
220 GHz
Institut de Radio
Astronomie Millimétrique Voie
10 Domaine Universitaire de Grenoble
38406 St. Martin d'Héres Cedex
France
Phone: (33) 7642 3383
Contact: Robert Lucas Instrument
Scientist
Sponsor: Centre National de la Recherche Scientifique, Paris; Max
Planck Gesellschaft
Reference: Delannoy, J., Weliachew, L., and Downes, D., in
ESO-IRAM-Onsala Workshop on (Sub) Millimeter Astronomy (ESO Proceedings
No. 22) (1985)
Location: Plateau de Bure, France
Latitude: 5° 54´ 26.0´´ E
Longitude: +44° 38´ 01.2´´ N
Altitude: 2552 m
Telescope: 3-element interferometer
Diameter: 3 x 15 m
Area: 530 m2 at >0.68 eff.
Height: 10 m
Coverage: 0°-360° az., 5°-90° el.
Remarks: Under construction, commissioning expected in 1988
Observation Type: Millimeter wavelength spectroscopy, radiometry, and
interferometry
Frequency band(s):
80-115 GHz
230 GHz
Service de
Radioastronomie
5, Place Jules Janssen
92195, Meudon Cedex, France
Contact: J. Pezzani
Sponsor: Centre National de la Recherche Scientifique (CNRS) and the
French Ministry of Education
Location: Nancay, France
Latitude: 47° 23´ N
Longitude: 02° 12´ E
Altitude: 130 m
Telescope: Network of 16 paraboloids distributed over 23 m, east-west
Diameter: 1 m
Area: 12 m2
Coverage: ±1/2 h, -20° ± 50° dec.
Observation Type: Solar
Frequency band(s):
9.400 GHz
Service de
Radioastronomie
5, Place Jules Janssen
92195, Meudon Cedex, France
Contact: J. Pezzani
Sponsor: Centre National de la Recherche Scientifique (CNRS) and the
French Ministry of Education
Reference: The Mark II Nancay Radioheliograph (Single Frequency
Version), Solar Physics 55, 251-261 (1977)
Location: Nancay, France
Latitude: 47° 23´ N
Longitude: 02° 12´ E
Altitude: 130 m
Telescope: Network of 16+2 paraboloids, distributed over 3.2 km, east
to west
Diameter: Sixteen 4-m paraboloids and two 10-m paraboloids
Area: 300 m2
Coverage: ±3 h, -20° ± 50° dec.
Observation Type: Solar and calibration radio sources (Cygnus A,
Cassiopeia, Hydra)
Frequency band(s):
5 simultaneously observed frequencies between 150-450 MHz
Service de
Radioastronomie
5, Place Jules Janssen
92195, Meudon Cedex, France
Contact: J. Pezzani
Sponsor: Centre National de la Recherche Scientifique (CNRS) and the
French Ministry of Education
Reference: The Mark III Nancay Radioheliograph (Single Frequency
Version) Solar Physics 88, 383-390 (1983)
Location: Nancay, France
Latitude: 47° 23´ N
Longitude: 02° 12´ E
Altitude: 130 m
Telescope: Network of 24 paraboloids, distributed over 1.2 km, north to
south
Diameter: Twenty-four 5-m paraboloids
Area: 300 m2
Coverage: ±3 h, -20° to 50° dec.
Observation Type: Solar and calibration radio sources
Frequency band(s):
5 simultaneously observed frequencies between 150 MHz-450 MHz
Service de
Radioastronomie
5, Place Jules Janssen
92195, Meudon Cedex, France
Contact: J. Pezzani
Sponsor: Centre National de la Recherche Scientifique (CNRS) and the
French Ministry of Education
Location: Nancay, France
Latitude: 47° 23´ N
Longitude: 02° 12´ E
Altitude: 130 m
Telescope: Dual reflecting antenna: tiltable flat reflector and
standing spherical reflector
Diameter: 40 x 200 m
Area: 5000 m2 at 1.5 GHz, 1700 m2 at 3.3 GHz
Coverage: ±1/2 h, 0° to 120° el.
Observation Type: Planetary, cometary, galactic, extragalactic;
continuum and spectral lines
Frequency band(s):
1400 MHz
1650 MHz
3300 MHz
Service de
Radioastronomie
5, Place Jules Janssen
92195, Meudon Cedex, France
Contact; J. Pezzani
Sponsor: Centre National de la Recherche Scientifique (CNRS) and the
French Ministry of Education
Reference: Boischot et al., Icarus 43, 399 (1980)
Location: Nancay, France
Latitude: 47° 23´ N
Longitude: 02° 12´ E
Altitude: 130 m
Telescope: 144 (2 x 72) conical log periodic antennas
Diameter: 60 m equivalent parabolic diameter at 40 MHz
Area: 2 x 4000 m2
Coverage: ±4 h, -20° ± 50° dec.
Observation Type: Solar and Jovian bursts
Frequency band(s):
15 MHz < f0 < 80 MHz
383762 Abastumani
Astrophysical Observatory
Mt. Kanobili
Republic of Georgia
Sponsor: Academy of Sciences of the Republic of Georgia
Reference: BAAO N29
Altitude: 1600-1700 m
Telescope: Flat synphase antenna
Diameter: 6.6 m x 3.1 m
Area: 20 m2
Height: 1.5 m
Coverage: 0°-360° az., 11°-90° el.
Remarks: Observations are carried out every day at 0400 h
Observation Type: Solar radio flares
Frequency band(s):
221 MHz
Max-Planck-Institut
für Radioastronomie
Auf dem Hügel 69
D 5300 Bonn 1, FRG
Contact: Dr. B.-H. Grahl
Sponsor: Max-Planck-Gesellschaft zur Förderung der Wissenschaft
Reference: Hachenberg, O., B.H. Grahl, R. Wielebinski, The 100-Meter
Radio Telescope at Effelsberg, IEEE 61, 1288-1295 (1973)
Latitude: 50° 50´ 0.3´´ N
Longitude: 6° 31´ 32.3´´ E
Altitude: 316 m
Telescope: Single dish
Diameter: 100 m
Area: 7854 m2 (geometrical area)
Coverage: 0°-360° az., 7°-90° el.
Observation Type: Types are listed under polarization below.
Frequency band(s):
610 MHz1
1415 MHz2
1666 MHz3
2695 MHz3
3245 MHz1
4.6 GHz4
4.75 GHz3
10.7 GHz5
22 GHz3
48.99 GHz6
Zentralinstitut
für Astrophysik der AdW
Rosa-Luxemburgstrasse 17
Babelsberg, 1590 Germany
Contact: H. Aurass
Sponsor:
Reference: Data routinely published quarterly as microfiches "Solar
Radio Data"
Location: Tremsdorf, 1501 Germany, 13 km SSW of Potsdam
Latitude: 52.28 N
Longitude: 13.13 E
Altitude: 35 m
Telescope: Three paraboloids
Diameter: 1.5, 4, and 10.5 m; and Yagi
Observation Type: Routine patrol of the total flux and polarization
Frequency band(s):
9.500 GHz (1.5 m*)
775 MHz (4 m**)
1470 MHz (4 m*)
2920 MHz (4 m*)
64 MHz (10.5 m**)
113 MHz (10.5 m*)
234 MHz (10.5 m*)
30 MHz (Yagi*)
40 MHz (Yagi*)
*as polarimeter **as radiometer
Raman Research Institute
Bangalore 560080
Indian Institute of Astrophysics, Bangalore-34
Phone: 340123 or 569951
Contact: Ch. V. Sastry
Sponsor: Department of Science and Technology, Government of India
Reference: J. Astrophy. Astr. 4, 47 (1983)
Location: Gauribidanur, Karnataka, India
Latitude: 13° 36´ 12´´ N
Longitude: 77° 27´ 07´´ E
Altitude: 500 m
Telescope: T-shaped array
Diameter: E-W 1.5 km/25 m, S array 0.5 km/15 m, N array 0.34 km/25 m
Area: 25,000 m2
Coverage: Transit only, ±60° el.
Remarks: Telescope is in use continuously, except for maintenance and
repair.
Observation Type: Solar, planetary, galactic, extragalactic, and
spectral line observations Frequency band(s):
34.5 MHz (45 MHz, 55 MHz, 80 MHz, and 150 MHz)
TIFR Center
P.O. Box 1234
Indian Institute of Science Campus
Bangalore 560 012, India
Phone: 343138, 344062, 342816
Contact: Govind Swarup
Sponsor: Tata Institute of Fundamental Research, Bombay, India
Reference: Swarup, G., Kapahi, V. K., and Ananthakrishnan, S., Status
Report, June 1987
Location: Khodad Village, Narayangaon, Junnar Taluk, 410504, Pune
District
Latitude: 19° 5´ 30´´ N
Longitude: 74° 3´ E
Altitude: 650 m
Telescope: 34 parabolic dishes, 16 of which are in a central cluster of
1 km x 1 km; the rest are along 3 arms of a Y with 6 antennas in each
14-km-long arm
Diameter: 45 m
Area: 35,000 m2 at 0.65 eff.
Height: Feed point is 45 m above ground in zenith position
Coverage: 0°-360° az., 10°-90° el.
Remarks: Planned to be completed by 1992
Observation Type: Search for primordial hydrogen, pulsars, IPS, lunar
occultation, galactic and extragalactic, solar, line, VLBI
Frequency band(s):
38 MHz
151 MHz
235 MHz
327 MHz
610 MHz
1420 MHz
Raman Research Institute
C.V. Raman Avenue
Sadashivanagar, Bangalore 560 080
Phone: 91-80-334 0122
Fax: 91-80-334 0492
Contact: uday@rri.ernet.in
Sponsor: The Raman Research Institute, the Indian Institute of
Astrophysics, and the University of Mauritius
Location: Bras d'Eau, Mauritius
Latitude: 20° S
Longitude: 57° E
Telescope: Aperture synthesis instrument. A T array with a 2 km long EW
arm with 1024 helices and 880 m long S arm, to be synthesized using 16
trolleys each.
Coverage: declination coverage -65 ° to -15 °
Remarks: The major objective is a complete continuum image of the
southern sky with sensitivity comparable to the 6C survey.
Frequency band(s):
151.6 MHz
Radio Astronomy Center
Post Box 8, Ootacamund 643 001
Tamil Nadu, India
Phone: (0423) 2651 or 2032
Contact: M.N. Joshi
Sponsor: Tata Institute of Fundamental Research
Reference: Swarup, G., et al., Nature Physical Science 230 185 (1971);
Swarup, G. and Bagri, D. S., Proc. IEEE 61 1285 (1973); Swarup, G., J.
Astrophys. Astr. 5 139 (1984)
Location: Muthorai Village, Ootacamund, India
Latitude: 11° 24´ N
Longitude: 76° 40´ E
Altitude: 2750 m
Telescope: Equatorially-mounted parabolic cylinder, steered
mechanically in E-W and mechanically in N-S
Diameter: ORT: 530 m (N-S) x 30 m (E-W)
OSRT: ORT plus 8 antennas 23 m x 9 m
Area: 7000 m2 at 0.50 eff.
Height: 25 m
Coverage: -4 h to +5 h 30 min, ±40° dec.
Remarks: The ORT is also used as an aperture synthesis array, with
eight smaller telescopes of size 23 m x 9 m distributed in an area of 4
km x 2 km.
Observation Type: Lunar occultation, IPS, spectral line, synthesis
mapping, pulsar search, VLBI, galactic, and extragalactic.
Frequency band(s):
326.5 MHz
Instituto di
Radioastronomia
Via Irnerio 46
40126 Bologna, Italy
taly
taly
taly
Contact: L. Padrielli
Sponsor: Consiglio Nazionale Delle Ricerche
Reference: Nuovo Cimento 23, 208 (1962)
Location: Medicina (Bologna), Italy
Latitude: 44° 31´ 14´´
Longitude: 11° 38´ 43´´
Altitude: 41.31 m
Telescope: Two arms (T-shaped), transit instrument, parabolic cylinder
Diameter: 560 x 35 m E-W, 64 (24 x 8 m) N-S
Coverage: 0°-90° dec. full instrument, -30° to 110° E-W
only
Remarks: Survey, periodic scheduling
Observation Type: Continuum galactic and extragalactic observations
Frequency band(s):
408 MHz
Instituto di
Radioastronomia
Via Irnerio 46
40126 Bologna, Italy
Phone: 51-243144
Contact: L. Padrielli
Sponsor: Consiglio Nazionale Delle Ricerche
Reference: Workshop on European VLBI for Geodesy and Astrometry, in
press
Location: Medicina (Bologna), Italy
Latitude: 44° 31´ 14´´
Longitude: 11° 38´ 43´´
Altitude: 41.31 m
Telescope: Steerable paraboloid
Diameter: 32 m
Area: 402 m2 at 0.50 eff.
Height: 33 m
Coverage: ±270° az., 0.5°-109° el.
Remarks: Periodic scheduling
Observation Type: VLBI for astronomy and geodesy, spectral lines
Frequency band(s):
1400 MHz
1600 MHz
5.0 GHz
10.7 GHz
22.3 GHz
2.2-8.2 GHz
via G.B. Tiepolo 11
I 34131 Trieste, Italy
Phone: (40) 768005
Contact: Paolo Zlobec
Sponsor: Ministry for University and Scientific and Technological
Research (MURST) and Italian Research Council (CNR)
Reference: Solar Phys. 9, 502 (1969)
Bul. Osservazioni Solari, Trieste Astron.
Obs. Suppl. 18 (1970)
Location: Basovizza (Trieste), Italy
Latitude: 45° 38´ 37´´ N
Longitude: 13° 52´ 34´´ E
Altitude: 400 m
Telescope: Single steerable paraboloid
Diameter: 10 m
Area: 70 m2
Height: 16.4 m
Coverage: 0°-360° az., 0°-90° el.
Remarks: Daily observing time: shortest interval 8h - 15h UT in
December and January; longest interval 6h - 18h UT in June and July.
The integration time is programmable.
Observation Type: Solar
Frequency band(s):
237 MHz
327 MHz
408 MHz
610 MHz
1413 MHz
1665 MHz
2695 MHz
Radio Research
Laboratory
Ministry of Posts and Telecommunications
3601 Isozaki
Nakaminto, Ibaraki
311-12 Japan
Contact: Susumu Isozaki
Location: Nakaminato, Ibaraki
Latitude: 36° 21.9´ N
Longitude: 140° 37.5´ E
Altitude: 26 m
Telescope: Four paraboloids
Diameter: 1.1 m
6 m
10 m (two)
Observation Type: Solar radio at 31.65 GHz, solar patrol at other
frequencies
Frequency band(s):
100.5 MHz
201 MHz
501 MHz
9.500 GHz
31.65 GHz
The Research Institute
of Atmospherics
Nagoya University
3-13 Honohara
Toyokawa, 442, Japan
Contact: Masayoshi Kojima
Sponsor: The Ministry of Education, Science and Culture
Reference: Proc. Res. Inst. Atmospherics, Nagoya Univ. 29, 61 (1982)
Location: Fuji Station
Sugadaira Station
Toyokawa Station
Latitude: 35° 26´ (Fuj.)
36° 31´ (Sug.)
34° 50´ (Tok.)
Longitude: 138° 37´ (Fuj.)
138° 19´ (Sug.)
137° 22´ (Tok.)
Altitude: 1000 m
Telescope: Cylindrical parabolic antenna
Diameter: 100 m E-W, 20 m N-S
Area: 1000 m2
Coverage: ±30° from meridian transit, 25° S to
40° N dec.
Remarks: Routine observation and simultaneous observation at three
stations
Observation Type: Continuous
Frequency band(s):
327 MHz
Radio Research
Laboratory
893-1 Hirai Kashima-machi
Ibaraki-ken, 314 Japan
Phone: 0299-82-1211
Contact: Noriyuki Kawagachi
Sponsor: Ministry of Posts and Telecommunications
Location: Kashima, Japan
Latitude: 35° 57´ 14.846´´ N
Longitude: 140° 39´ 45.8344´´ E
Altitude: 78.770 m
Telescope: Steerable parabolic
Diameter: 26.0 m
Area: 531 m2 at 0.53 eff. (X-band)
531 m2 at 0.52 eff. (S-band)
Height: 18.4 m
Coverage: 0°-360° az., 0°-90° el.
Observation Type: Extragalactic and galactic continuum observation,
VLBI scheduling for geodesy
Frequency band(s):
200-2320 MHz
8160-8800 MHz
Kisarazu National
College of Technology
Kisarazu Chiba, 292 Japan
Phone: 0438-(98)-5751
Contact: Shinji Kodaira
Sponsor: Ministry of Education
Reference: Bull. Kisarazu National College of Technology 13 (1980)
Location: Kisarazu chiba, 292 Japan
Latitude: 35° 22´ 51´´ N
Longitude: 139° 57´ 31´´ E
Altitude: 46 m
Telescope: One paraboloid dish
Diameter: 1.5 m
Area: 0.9 m2 at 0.50 eff.
Height: 2.5 m
Coverage: 90°-270° az., 27°-90° el.
Remarks: No fixed scheduling
Observation Type: CO spectral line observation
Frequency band(s):
115.27 GHz
Nobeyama Radio
Observatory
Minamisaku, Nagano 384-13
Japan 02267
Phone: 0267 (98) 2831
Contact: Prof. Masaki Morimoto
Sponsor: Ministry of Education, Science and Culture
Reference: Nobeyama 45-m Telescope, Kaifu, Proceedings of the
International Symposium on Millimeter and Submillimeter Wave Radio
Astronomy, 1985
Latitude: 35° 56´ 29´´ N
Longitude: 138° 28´ 32´´ E
Altitude: 1349 m
Telescope: Paraboloid
Diameter: 45 m
Area: 410 m2 (at 115 GHz) to 950 m2 (at < 50 GHz)
Height: 21 m
Coverage: 0°-360° az., 11°-85° el.
Remarks: International open use; VLBI on all frequencies except 70-90
GHz
Observation Type: (see frequency list) *Galactic and extragalactic
continuum and spectral line observations
**The above plus solar observations
Frequency band(s):
9.8 GHz*
23.0 GHz**
36-49 GHz
(tunable)**
36-49 GHz
(tunable)*
70-90 GHz
(tunable)**
85-115 GHz (tunable)*
Nobeyama Radio
Observatory
Minamisaku, Nagano 384-13
Japan 02267
Phone: 0267 (98) 2831
Contact: Prof. Masaki Morimoto
Sponsor: Ministry of Education, Science and Culture
Reference: M. Ishiguro et al., The Nobeyama Millimeter Wave
Interferometer, Proceedings of the International Symposium on
Millimeter and Submillimeter Wave Radio Astronomy, 1985
Latitude: 35° 56´ 29´´ N
Longitude: 138° 28´ 32´´ E
Altitude: 1349 m
Telescope: Five-element interferometer array, T baseline is 560 m E-W,
520 m N-S
Diameter: 10 m
Area: 39 m2 x 5 at 0.50 eff. (2.6 mm)
Height: 8 m
Coverage: 0°-360° az., 0°-90° el.
Remarks: *SIS mixer, FX correlator
**HEMT amp, FX correlator
Observation Type: Aperture synthesis, continuum and spectral lines
Frequency band(s):
22-24 GHz*
40-50 GHz**
80-120 GHz*
Nobeyama Radio
Observatory
Minamisaku, Nagano 384-13
Japan 02267
Phone: 0267 (98) 2831
Contact: Prof. Hiroshi Nakajima
Sponsor: Ministry of Education, Science and Culture
Reference: Publ. Astron. Soc. Japan 32, 639 (1980)
Latitude: 35° 56´ 19´´ N
Longitude: 138° 28´ 46´´ E
Altitude: 1300 m
Telescope: Sixteen steerable paraboloids (interferometer)
Diameter: 1.2 m
Area: 0.45 m2 for each paraboloid at 0.40 eff.
Height: 2.0 m
Coverage: -50° to +50° az., 20°-80° el.
Remarks: Daily observations
Observation Type: Solar
Frequency band(s):
17 GHz
Minamisaku, Nagano
384-13
Japan 02267
Phone: (0267) 98 2034
Contact: Prof. Hiroshi Nakajima
Sponsor: The Ministry of Education, Science and Culture
Reference: Publ. Astron. Soc. Japan 32, 371 (1980)
Location: Minamisaku-gun, Nagano
Latitude: 35° 56´ 19´´ N
Longitude: 138° 28´ 46´´ E
Altitude: 1300 m
Telescope: Two steerable paraboloids
Diameter: 8 m, 6 m
Area: 15 m2 for 8-m paraboloid, 8.52 m2 for 6-m paraboloid,
0.30 eff.
Height: 5 m, 4 m
Coverage: -60° to +60° az., 0°-120° el.
Remarks: Daily observations
Observation Type: Solar
Frequency band(s):
70-1000 MHz
Nobeyama Solar Radio
Observatory of Tokyo Astronomical Observatory
Minamimaki-mura, Minamisaku-gun, Nagano 384-13 Japan
Sponsor: The Ministry of Education, Science and Culture
Reference: Proc. Astron. Soc. Australia 1, 56 (1967)
Location: Minamisaku-gun, Nagano
Latitude: 35° 56´ 19´´ N
Longitude: 138° 28´ 46´´ E
Altitude: 1300 m
Telescope: Seventeen steerable paraboloids (interferometer)
Diameter: 6 m
Area: 8.5 m2 for each paraboloid, 0.30 eff.
Height: 10 m
Coverage: -60° to +60° az, 0°-120° el.
Remarks: Daily observations
Observation Type: Solar
Frequency band(s):
160.4 MHz
Nobeyama Radio
Observatory
Minamisaku, Nagano 384-13
Japan 02267
Phone: (0267) 98 2034
Contact: Prof. Hiroshi Nakajima
Sponsor: Ministry of Education, Science and Culture
Reference: Publ. Astron. Soc. Japan 37, 163 (1985)
Latitude: 35° 56´ 19´´ N
Longitude: 138° 28´ 46´´ E
Altitude: 1300 m
Telescope: Three paraboloids on the same equatorial mount
Diameter: 0.3 m for one, 0.25 m for the other two
Area: 0.035 m2 for 0.3-m paraboloid, 0.025 m2 for
the other two telescopes
Height: 2 m
Coverage: -60° to +60° az., 20°-80° el.
Remarks: Daily observations
Observation Type: Solar
Frequency:
35 GHz for 0.3-m paraboloid, 80 GHz for the other two telescopes
Research Institute of Atmospherics
Nagoya University
13 Honohara 3-chome
Toyokawa 442, Japan
Sponsor: Ministry of Education, Science and Culture
Reference: Proc. Res. Inst. Atmospherics, Nagoya Univ. 26, 129-132
(1979)
Location: Toyokawa, Japan
Latitude: 34° 50´ 10.87´´ N
Longitude: 137° 22´ 16.84´´ E
Altitude: 18.49 m
Telescope: Single dish
Diameter: 0.85 m
Area: 0.3 m2
Height: 2.5 m
Coverage: Equatorial mounting
Remarks: Patrol observations
Observation Type: Solar
Frequency band(s):
9.411 GHz
Research Institute of Atmospherics
Nagoya University
13 Honohara 3-chome
Toyokawa 442, Japan
Sponsor: Ministry of Education, Science and Culture
Reference: Proc. Res. Inst. Atmospherics, Nagoya Univ. 26, 129-132
(1979)
Location: Toyokawa, Japan
Latitude: 34° 50´ 10.87´´ N
Longitude: 137° 22´ 16.84´´ E
Altitude: 18.49 m
Telescope: single dish
Diameter: 1.5 m
Area: 1.1 m2
Height: 2.5 m
Coverage: Equatorial mounting
Remarks: Patrol observations
Observation Type: Solar
Frequency band(s):
3750 MHz
Research Institute of Atmospherics
Nagoya University
13 Honohara 3-chome
Toyokawa, Japan
Sponsor: Ministry of Education, Science and Culture
Reference: Proc. Res. Inst. Atmospherics, Nagoya Univ. 26, 129-132
(1979)
Location: Toyokawa, Japan
Latitude: 34° 50´ 10.87´´ N
Longitude: 137° 22´ 16.84´´ E
Altitude: 18.49 m
Telescope: Single dish
Diameter: 2.0 m
Area: 1.9 m2
Height: 2.5 m
Coverage: Equatorial mounting
Remarks: Patrol observations
Observation Type: Solar
Frequency band(s):
2060 MHz
Research Institute of Atmospherics
Nagoya University
13 Honohara 3-chome
Toyokawa 442, Japan
Sponsor: Ministry of Education, Science and Culture
Reference: Proc. Res. Inst. Atmospherics, Nagoya Univ. 26, 129-132
(1979)
Location: Toyokawa, Japan
Latitude: 34° 50´ 10.87´´ N
Longitude: 137° 22´ 16.84´´ E
Altitude: 18.49 m
Telescope: Single dish
Diameter: 3.0 m
Area: 4.2 m2
Height: 3 m
Coverage: Equatorial mounting
Remarks: Patrol observations
Observation Type: Solar
Frequency band(s):
1060 MHz
Research Institute of
Atmospherics
Nagoya University
13 Honohara 3-chome
Toyokawa 442, Japan
Sponsor: Ministry of Education, Science and Culture
Reference: Proc. Res. Inst. Atmospherics, Nagoya Univ. 17, 57-74 (1970)
Location: Toyokawa, Japan
Latitude: 34° 50´ 10.87´´ N
Longitude: 137° 22´ 16.84´´ E
Altitude: 18.49 m
Telescope: 32 x 16 tee, 32 x 2 linear
Diameter: 2 m east-west
1.2 m north-south
Height: 2.5 m
Coverage: ±3 h, ±23.5° dec.
Remarks: Routine observations
Observation Type: Solar
Frequency band(s):
9.407 GHz
Research Institute of
Atmospherics
Nagoya University
13 Honohara 3-chome
Toyokawa 442, Japan
Sponsor: Ministry of Education, Science and Culture
Reference: Nishio, M., et al., Proc. Res. Inst. Atmospherics, Nagoya
Univ. 32, 45-60 (1985)
Location: Toyokawa, Japan
Latitude: 34° 50´ 10.87´´ N
Longitude: 137° 22´ 16.84´´ E
Altitude: 18.49 m
Telescope: 32 x 16 tee, 32 x 2 linear, 16 x 2 linear
Diameter: 3 m
Area: 4.2 m2 x square root of (m x n), where m and n denote
array numbers of antennas
Height: 8 m
Coverage: ±3 h, ±23.5° dec.
Remarks: Routine observation
Observation Type: Solar
Frequency band(s):
3748.5 MHz
Mexico
Sponsor: INAOE and the University of Massachusetts via Mexican and U.S.
funding agencies
Contact: in Mexico Alfonso
Serrano, in the US Peter
Schloerb
Latitude: 18° 59.1´ North
Longitude: 97° 18.8´ West
Altitude: 4580 meters above mean sea level
Telescope: Steerable paraboloid, two-element interferometer
Diameter: 50 m
Area: 2000 m2 (approximately)
Height: 60 m to the top edge of the antenna above the ground when
pointing to the horizon
Coverage: above declination -40°
Observation Type: continuum and spectroscopic
Frequency band(s): any between 85 and 350 GHz
Instituto Nacional de Astrofisica Optica y
Electronica (INAOE)
A.P. 51 y 216 Puebla
72000-Puebla, Mexico
Sponsor: CONACYT
Contact: Eduardo Mendoza
Latitude: 19° 01´ 58´´
Longitude: 98° 18´ 50´´
Altitude: 2200 m
Telescope: Steerable paraboloid, two-element interferometer
Diameter: 1 m
Area: 0.8 m2
Height: 1 m
Coverage: 0°-360° az., 10°-90° el.
Observation Type: Solar
Frequency band(s):
9 GHz
Instituto
de Geofisica
Universidad Nacional Autónoma de México (UNAM)
Ciudad Universitaria
Del. Coyoacán México
D.F. 04510 México
Sponsor: UNAM
Contact: Alejandro Lara
Latitude: 19° 20´ 01´´
Longitude: 98° 10´ 54´´
Altitude: 2280 m
Telescope: Two-element interferometer
Diameter: 1.14 m
Area: 1 m2 (each)
Height: 2 m
Coverage: 0°-360° az., 10°-90° el.
Observation Type: Solar
Frequency band(s): 7.5 GHz
NFRA Radio Sterrenwacht
Dwingeloo
P.O. Box 2
7990 AA Dwingeloo, The Netherlands
Phone: 5219-7244
Contact: C. Slottje
Sponsor: Netherlands Organization for Advancement of Pure Research
(Z.W.O.)
Location: Dwingeloo, Netherlands
Latitude: 52° 48´ 47´´ N
Longitude: 6° 23´ 46´´ E
Altitude: 25 m
Telescope: Steerable paraboloid
Diameter: 25 m
Area: 314 m2 at 0.64 eff. (21-cm wavelength)
196 m2 at 0.40 eff. (6-cm wavelength)
Height: 25 m
Coverage: 0°-360° az., 0°-90° el.
Remarks: Used primarily for large-scale surveys
Observation Type: Auto-correlation spectrometry
Frequency band(s):
1400 MHz
1652.5 MHz
4895 MHz
Netherlands Foundation
for Radio Astronomy
N.F.R.A. Post Box 2
7990 AA Dwingeloo, The Netherlands
Contact: Dr. Marla J. Bentum
Sponsor: Netherlands Organization for Scientific Research
Reference: A&A 31, (1974); A&A 98, 251-259 (1981)
Location: Westerbork, the Netherlands
Latitude: 52° 55´ 0.09´´
Longitude: 00h 26´ 25.0s
Altitude: 16 m
Telescope: Array with 14 steerable paraboloids (of which 4 are movable
and 10 are fixed) on an E-W baseline, operating on the principle of
rotational aperture synthesis. Minimum baseline 32 m, maximum 2796 m.
Diameter: 25 m
Area: 491 m2
Height: 20 m
Coverage: ±90° in hour angle, -32°-90° in declination
Remarks: Integration time is 12 h for a complete observation, but other
integration times are used.
Observation Type: Continuum (to 160 MHz) synthesis, spectral line
synthesis, tied-array - VLBI, tied-array - pulsar
Frequency band(s):
310-390 MHz
606-610 MHz
1200-1450 MHz
1590-1750 MHz
2215-2375 MHz
4770-5020 MHz
8150-8650 MHz
250-460 MHz
700-1200 MHz
Zelenchukskaya
Stravropolski kraj
Russia 357 140
Contact: Sergey A. Trushkin
Sponsor: Russian Academy of Sciences
Reference: Isvestija Glav. Astron. Obs. I88 (1972), Sky and Telescope
(1979)
Location: Zelenchukskaya, Russia
Altitude: 1000 m
Telescope: Variable profile antenna, circle of 895 reflector elements
Diameter: 600 m
Area: 1000 m2 (8 cm) for each of 4 sectors
500 m2 (2 cm) for each of 4 sectors
3000 m2 (8 cm) for the whole circle
Height: 7.6 m
Coverage: 0°-360° az., 3°-90° el.
Remarks: All observations are transit, with tracking 2 min. Three
different programs can run simultaneously at three sectors.
Frequency band(s):
1000 MHz
1500 MHz
2500 MHz
3750 MHz
7.600 GHz
9.375 GHz
11.100 GHz
13.000 GHz
15.000 GHz
37.000 GHz
1420 MHz
1670 MHz
4850 MHz
22.200 GHz
960 MHz
2300 MHz
3650 MHz
3900 MHz
7.700 GHz
14.400 GHz
21.800 GHz
3650 MHz
11.500 GHz
3900 MHz
7.700 GHz
14.400 GHz
Hartebeesthoek Radio
Astronomy Observatory
P.O. Box 443
Krugersdorp 1740, South Africa
Sponsor:
Contact: Information at HartRAO
Latitude: 25 53´ 14.4´´
Longitude: +27 41´ 05.2´´
Altitude: 1415.8211415.8211415.8211415.821orially mounted 85 foot
Cassegrain
Diameter: 25.9 m
Area:
Height:
Coverage:
Observation Type:
Frequency band(s):
Korean Astronomy
Observatory
Sponsor: The Korean Ministry of Science and Technology
Location: Daejeon Daeduk, Chungman
Latitude: 36° 23´ 53.2´´
Longitude: 127° 22´ 19´´ E
Altitude: 110 m
Telescope: Steerable paraboloid, single dish
Diameter: 13.7 m
Area: 50.1 m2 at 0.34 eff. (115 GHz)
Height: 1.5 m
Coverage: 0°-720° az., 7°-90° el.
Remarks: Periodic scheduling
Observation Type:
Spectral line and continuum
d coe and coand(s):
80-115 GHz
43520 Roquetas
(Tarragona) Spain
Location: Observatorio Del Ebro-Roquetas
Latitude: 40° 49´ 14´´ N
Longitude: 0 h 1 min 58.5 s E
Altitude: 51 m
Telescope: Parabolic reflector and feed system
Diameter: 3.24 m
Height: 2-m pedestal
Coverage: 0° ± 110° az., 49° ± 23° el.
Observation Type: Solar
Frequency band(s):
1390-1567 MHz
2540-2720 MHz
1830-5030 MHz
Onsala Space Observatory
Chalmers Institute of Technology
S-439 00
Onsala, Sweden
Phone: 0300/62590
Contact: Roy Booth
Sponsor: The Swedish Natural Science Council (NFR) and European
Southern Observatory (ESO)
Reference: The Messenger 48, 2 (1987)
Location: La Silla, Chile
Latitude: -29° 15´ 34´´
Longitude: 70° 44´ 04´´ W
Altitude: 2400 m
Telescope: Three paraboloids
Diameter: 15 m [only one listed]
Area: (1) 117 m2, (2) 90 m2, (3) 70 m2
Height: 10 m
Coverage: 0°-360° az., 2°-90° el.
Remarks: Periodic scheduling
Observation Type: Planetary, galactic, extragalactic; spectral line and
continuum studies
Frequency band(s):
(1) 85-117 GHz
(2) 220-280 GHz
(3) 300-360 GHz
Chalmers University of
Technology
S-439 00
Onsala, Sweden
Phone: 0300/625 90
Contact: Roy Booth
Sponsor: CTH, Swedish Natural Science Research Council
Reference: The International Journal of Aerial and Space Imaging,
Remote Sensing, and Integrated Geographical Systems 1, 27 (1987)
Location: Onsala, Sweden
Latitude: (1) 57° 23´ 46.9´´, (2) 57°
23´ 37.0´´
Longitude: (1) 11° 55´ 39.4´´ E, (2) 11°
58´ 8.5´´ E
Altitude: (1) 25 m, (2) 24 m
Telescope: Telescopes 1 and 2
Diameter: (1) 20 m, (2) 25 m
Area: (1) 80 to 160 m2, (2) 160 to 270 m2
Height: (1) 14 m, (2) 16 m
Coverage: 0°-360° az., 2°-90° el.
Remarks: Periodic scheduling
Observation Type: Planetary, galactic, extragalactic; continuum and
spectral line observations
Frequency band(s):
(1) 116 MHz to 8 GHz
(2) 7 MHz to 1 GHz
Institute of Astronomy
ETH-Zentrum, CH-8092
Zurich, Switzerland
Phone: (1) 256 3813
Contact: Dr. A. Benz
Sponsor: Swiss Federal Institute of Technology (Zurich)
Swiss National Science Foundation
Reference: Tarnstrom G.L., Astr. Mitt. Eidg. Sternwarte Zurich 317
(1973)
Location: Bleien (near Zurich), Switzerland
Latitude: 47° 20´ 26´´ N
Longitude: 8° 06´ 44´´ E
Altitude: 435 m
Telescope: Steerable paraboloid
Diameter: 5 m
Area: 78 m2 at 0.75 eff.
Height: 3 m
Coverage: 0°-360° az., 5°-90° el.
Remarks: Recorded on 35-mm film, continuous operation from sunrise to
sunset, routine program for overview on solar activities and
identification of radio bursts. List of events published in
Solar-Geophysical Data and Quarterly Bulletin of the IAU.
Observation Type: Solar radio bursts
Frequency band(s):
100-1000 MHz (spectrometer)
Institute of Astronomy
ETH-Zentrum, CH-8092
Zurich, Switzerland
Phone: (1) 256 3813
Contact: Dr. A. Benz
Sponsor: Swiss Federal Institute of Technology (Zurich), Swiss National
Science Foundations
Reference: Benz et al., Solar Phys. 133 385 (1991)
Location: Bleien (near Zurich), Switzerland
Latitude: 47° 20´ 26´´ N
Longitude: 8° 06´ 44´´ E
Altitude: 435 m
Telescope: Steerable paraboloid
Diameter: 7 m
Area: 154 m2 at 0.70 eff.
Height: 3 m
Coverage: 0°-360° az., 5°-90° el.
Remarks: Computer-controlled instrument with programmable observing
range and resolution. Remotely operated. Automatic operation using
flare flag or continuous operation.
Observation Type: Solar radio spectrum of flares
Frequency band(s):
100-3000 MHz (spectrometer)
Physics Department
University of Tasmania
GPO Box 252C
Hobart, Tasmania, Australia 7001
Phone: (03) 62 26 2420
Contact: Prof. P.M. McCulloch
Latitude: 31° 52´ S
Longitude: 133° 48´ 35´´ E
Altitude: 100 m
Telescope: Steerable paraboloid
Diameter: 30 m
Area: 390 m2 at 0.55 eff.
Height: 40 m
Coverage: 0°-360° az., 0°-90° el.
Observation Type: VLBI, line ad continuum, galactic, extragalactic
Frequency band(s):
1.6-24 GHz
Physics Department
University of Tasmania
GPO Box 252C
Hobart, Tasmania, Australia 7001
Phone: (03) 62 26 2420
Contact: Prof. P.M. McCulloch
Location: Cambridge, Tasmania, Australia
Latitude: 42° 48´ 18´´ S
Longitude: 147° 26´ 21´´ E
Altitude: 55 m
Telescope: Steerable paraboloid
Diameter: 14 m
Area: 85 m2 at 0.55 eff.
Height: 25 m
Coverage: 0°-360° az., 0°-85° el.
Remarks: Monitoring Vela pulsar
Observation Type: Pulsars (emission properties and timing)
Frequency band(s):
600 MHz, 900 MHz, 1390 MHz
Physics Department
University of Tasmania
GPO Box 252C
Hobart, Tasmania, Australia 7001
Phone: (03) 62 26 2420
Contact: Prof. P.M. McCulloch
Location: Cambridge, Tasmania, Australia
Latitude: 42° 48´ 18´´ S
Longitude: 147° 26´ 21´´ E
Altitude: 52 m
Telescope: Steerable paraboloid (X-Y mount prime focus)
Diameter: 26 m
Area: 292 m2 at 0.55 eff.
Height: 40 m
Coverage: 0°-360° az., 0°-85° el.
Remarks: Periodic scheduling
Observation Type: Galactic and extragalactic; line and continuum, VLBI
Frequency band(s):
From 600 MHz to 12 GHz
Science and Engineering
Research Council
Appleton Laboratory
Ditton Park
Slough, England
Sponsor: U.K. Science and Engineering Research Council
Location: Hants, England
Latitude: 51° 08´ 40.1´´ N
Longitude: 01° 26´ 13.2´´ W
Altitude: 85 m
Telescope: Steerable paraboloid, prime focus
Diameter: 25 m
Height: ~15 m
Coverage: 0°-540° az., 0°-90° el.
Observation Type: Used for tropospheric propagation research program
Frequency band(s):
3-30 GHz
Royal Observatory
SERC
Blackford Hill
Edinburgh EH9 3HJ
United Kingdom
Phone: (0) 31 667 3321
Contact: S. J. Bell Burnell
Sponsor: SERC (U.K.), ZWO (Netherlands), NRC (Canada)
Reference: Proc. ISAP 233-5 (1985);
J. Brit. Interplanetary Soc. 39, 211 (1986)
Location: Mauna Kea, Hawaii
Latitude: 155° 28´ 19.5´´ W
Longitude: 19° 49´ 33´´ N
Altitude: 4000 m
Telescope: Alt.-az. mounted, steerable paraboloid, cassegrain (or
Nasmyth)
Diameter: 15 m
Coverage: 0°-360° az., 5°-89.5° el.
Remarks: ***He-3 cooled Ge bolometer
Observation Type: (see frequency list)
*Molecular line studies
**Molecular line studies
***Continuum observations
Frequency band(s):
218-235 and 256-270 GHz*
320-370 GHz**
150-1000 GHz***
*Instantaneous bandwidth 500 MHz
**Instantaneous bandwidth 500 MHz
***Various bandwidths, 8 filters
Department of Radio
Astronomy
University of Manchester
Manchester, M13 9PL England
Contact: R. J. Cohen
Location: Jodrell Bank, Macclesfield, Cheshire, England
Latitude: 53° 14´ 8.3´´ N
Longitude: 2° 18´ 18.5´´ W
Telescope: 42-ft fully steerable paraboloid, az.-el. mounted
Diameter: 13 m
Area: 85 m2 at 0.65 eff.
Height: 20 m
Coverage: Full sky
Remarks: Continuous operation at 610 MHz; occasional use at 966 or 1420
MHz
Observation Type: Pulsar Timing
Frequency band(s):
610 MHz
966 MHz
1420 MHz
Department of Radio
Astronomy
University of Manchester
Manchester M13 9PL England
Contact: R. J. Cohen
Location: Lords Bridge Observatory, Cambridge, England
Latitude: 52° 09´ 59´´ N
Longitude: 0° 02´ 20´´ E
Altitude: 24 m
Telescope: 32-m shaped paraboloid, az.-el. mounted
Diameter: 32 m
Area: 635 m2 at 0.79 eff.
Coverage: Full sky
Remarks: Instantaneous bandwidths available for MERLIN and VLBI
observations are restricted to 16 MHz.
Observation Type: MERLIN continuum and spectral line synthesis mapping;
VLBI; spectral line
Frequency band(s):
151 MHz
408 MHz
1350-1750 MHz
4600-5100 MHz
21.0-24.0 GHz
Department of Radio
Astronomy
NRAL Jodrell Bank
Macclesfield
Cheshire SK11 9Dl, England
Contact: R. J. Cohen
Location: Darnhall, Cheshire, England
Latitude: 53° 09´ 21.6´´ N
Longitude: 2° 32´ 03.3´´ W
Altitude: 47 m
Telescope: Fully steerable paraboloid, az.-el. mounted
Diameter: 25 m
Area: 320 m2 at 0.65 eff.
Coverage: Full sky
Remarks: Instantaneous bandwidths available for MERLIN observations are
restricted to 16 MHz.
Observation Type: MERLIN continuum and spectral line synthesis mapping;
VLBI; spectral line
Frequency band(s):
151 MHz
408 MHz
1350-1750 MHz
4600-5100 MHz
21.0-24.0 GHz
Department of Radio
Astronomy
NRAL Jodrell Bank
Macclesfield
Cheshire SK11 9Dl, England
Contact: R. J. Cohen
Location: Defford, North Pershore, Worcestershire, England
Latitude: 52° 06´ 00.6´´ N
Longitude: 2° 08´ 35.0´´ W
Telescope: Fully steerable paraboloid, equatorially mounted
Diameter: 25 m
Area: 320 m2 at 0.65 eff.
Coverage: Full sky
Remarks: Instantaneous bandwidths available for MERLIN observations are
restricted to 16 MHz.
Observation Type: MERLIN continuum and spectral line synthesis mapping;
VLBI; spectral line
Frequency band(s):
151 MHz
408 MHz
1350-1750 MHz
4600-5100 MHz
Department of Radio
Astronomy
NRAL Jodrell Bank
Macclesfield
Cheshire SK11 9Dl, England
Contact: R. J. Cohen
Location: Knockin, Shropshire, England
Latitude: 52° 47´ 23.9´´ N
Longitude: 2° 59´ 44.9´´ W
Altitude: 66 m
Telescope: Fully steerable paraboloid, az.-el. mounted
Diameter: 25 m
Area: 320 m2 at 0.65 eff.
Coverage: Full sky
Remarks: Instantaneous bandwidths available for MERLIN observations are
restricted to 16 MHz.
Observation Type: MERLIN continuum and spectral line synthesis mapping;
VLBI; spectral line
Frequency band(s):
151 MHz
408 MHz
1350-1750 MHz
4600-5100 MHz
21.0-24.0 GHz
Department of Radio
Astronomy
University of Manchester
Manchester, M13 9PL England
Contact: R. J. Cohen
Location: Jodrell Bank, Macclesfield, Cheshire, England
Latitude: 53° 14´ 10.5´´ N
Longitude: 2° 18´ 25.8´´ W
Altitude: 78 m
Telescope: Mk IA fully steerable paraboloid, az.-el. mounted
Diameter: 76 m
Area: 2990 m2 0.65 eff.
Height: 91 m
Coverage: Full sky
Observation Type: MERLIN continuum and spectral line synthesis mapping;
VLBI; pulsars; spectral line; continuum
Frequency band(s):
151 MHz
240 MHz
327 MHz
408 MHz
610 MHz
930 MHz
966 MHz
1350-1750 MHz
2300 MHz
2700 MHz
4600-5000 MHz
5.863 GHz
6.0-6.7 GHz
Department of Radio
Astronomy
University of Manchester
Manchester, M13 9PL England
Contact: R. J. Cohen
Location: Jodrell Bank, Macclesfield, Cheshire, England
Latitude: 53° 14´ 1.2´´ N
Longitude: 2° 18´ 8.9´´ W
Telescope: Mk II fully steerable paraboloid, az.-el. mounted
Diameter: 38 x 25.9 m
Area: 500 m2 0.65 eff.
Coverage: Full sky
Observation Type: MERLIN continuum and spectral line synthesis mapping;
VLBI; pulsars; spectral line; continuum
Frequency band(s):
151 MHz
240 MHz
327 MHz
408 MHz
610 MHz
930 MHz
966 MHz
1350-1750 MHz
2300 MHz
2700 MHz
4600-5000 MHz
21.0-24.0 GHz
Department of Radio
Astronomy
University of Manchester
Manchester, M13 9PL England
Sponsor: NRAL Jodrell Bank
Macclesfield
Cheshire SK11 9Dl, England
Contact: R. J. Cohen
Location: Pickmere, Cheshire, England
Latitude: 53° 17´ 18.4´´ N
Longitude: 2° 26´ 38.3´´ W
Altitude: 35 m
Telescope: Fully steerable paraboloid, az.-el. mounted
Diameter: 25 m
Area: 320 m2 at 0.65 eff.
Coverage: Full sky
Remarks: Instantaneous bandwidths available for MERLIN observations are
restricted to 16 MHz.
Observation Type: MERLIN continuum and spectral line synthesis mapping;
VLBI; spectral line
Frequency band(s):
151 MHz
408 MHz
1350-1750 MHz
4600-5100 MHz
21.0-24.0 GHz
Institute of Radio
Astronomy
National Academy of Sciences of Ukraine
4, Krasnoznamennaya ul.
Kharkov, 310002, Ukraine
Contact: L. N. Litvinenko
Sponsor: National Academy of Sciences of Ukraine
Reference: Braude, S. Ya., et al., Astrophys. Space Sci. 54, 3 (1978)
Latitude: 49° 39´
Longitude: -36° 21´
Altitude: 150 m
Telescope: Linear array, crossed dipoles
Observation Type: Interferometer with the UTR-2, base distance of 43 km
Frequency band(s):
10 MHz
12.6 MHz
14.7 MHz
16.7 MHz
20 MHz
25 MHz
Institute of Radio
Astronomy
National Academy of Sciences of Ukraine
4, Krasnoznamennaya ul.
Kharkov, 310002, Ukraine
Contact:
Sponsor: National Academy of Sciences of Ukraine
Reference:
Latitude:
Longitude:
Altitude:
Telescope:
Observation Type:
Frequency band(s):
Institute of Radio
Astronomy
National Academy of Sciences of Ukraine
4, Krasnoznamennaya ul.
Kharkov, 310002, Ukraine
Contact:
Sponsor: National Academy of Sciences of Ukraine
Reference:
Latitude:
Longitude:
Altitude:
Telescope:
Observation Type:
Frequency band(s):
Institute of Radio
Astronomy
National Academy of Sciences of Ukraine
4, Krasnoznamennaya ul.
Kharkov, 310002, Ukraine
Contact: L. N. Litvinenko
Sponsor: National Academy of Sciences of Ukraine
Reference: Braude, S. Ya., et al., Astrophys. Space Sci. 54, (1978)
Latitude: 49° 38´
Longitude: -36° 56´
Altitude: 150 m
Telescope: T-shaped array
Diameter: 1800 x 54 m north-south
900 x 54 m east-west
Area: 14.3 x 103 m2 at 10 MHz
14.2 x 103 m2 at 12.6 MHz
13.1 x 103 m2 at 14.7 MHz
12.3 x 103 m2 at 20 MHz
6.7 x 103 and 9.9 x 103 m2 at 25 MHz
Coverage: ±70° from zenith in both coordinates
Observation Type: (1) Systematic survey of discrete sources in the
northern sky, (2) Search for recombination lines with large quantum
numbers, (3) Pulsars, (4) Supernova remnants, (5) H II regions, (6)
Fine structure of objects by scintillation method, (7) Jupiter, (8)
VLBI, (9) The sun
Frequency band(s):
10.0 MHz
12.6 MHz
14.7 MHz
16.7 MHz
20 MHz
25 MHz
EISCAT Headquarters
P.O. Box 812
S-98128 Kiruna, Sweden
Sponsor: CNRS (Fr.), SA (Fin.), MPG (W. Ger.), NAVF (Nor.), NFR (Sw.),
SERC (U.K.)
Reference: Folkestad et al., Radio Science 18, 867-819 (1983)
Location: Kiruna, Sweden; Tromsö, Norway; and Sodankylä,
Finland
Latitude: 67.87° N (Kir.)
69.57° N (Tro.)
67.36° N (Sod.)
Longitude: 20.44° E (Kir.)
19.23° E (Tro.)
26.63° E (Sod.)
Altitude: 418 m (Kir.)
86 m (Tro.)
198 m (Sod.)
Telescope: 4 parabolic dishes: transmitter-receiver at Tromsö,
receivers at Kiruna and Sodankylä
Diameter: 32 m
Area: 520 m2
Height: 40 m
Coverage: 0°-360° az., 2°-90° el.
Observation Type: Incoherent scatter radar and radio astronomy
Frequency band(s):
933 MHz
>EISCAT Headquarters
P.O. Box 812
S-98128 Kiruna, Sweden
Sponsor: CNRS (Fr.), SA (Fin.), MPG (W. Ger.), NAVF (Nor.), NFR (Sw.),
SERC (U.K.)
Reference: Folkestad et al., Radio Science 18, 867-819 (1983)
Location: Longyearbyen, Svalbard
Observation Type: Incoherent scatter radar and radio astronomy
Frequency band(s):
933 MHz
EISCAT Headquarters
P.O. Box 812
S-98128 Kiruna, Sweden
Sponsor: CNRS (Fr.), SA (Fin.), MPG (W. Ger.), NAVF (Nor.), NFR (Sw.),
SERC (U.K.)
Reference: Folkestad et al., Radio Science 18, 867-819 (1983)
Location: Kiruna, Sweden
Latitude: 67.87° N
Longitude: 20.44° E
Altitude: 418 m
Telescope: 4 parabolic cylinders
Diameter: 40 x 120 m
Area: 3250 m2
Height: 40 m
Coverage: 0°-360° az., 60-150° el.
Observation Type: Incoherent scatter radar and radio astronomy
Frequency band(s):
224 MHz
300, rue de la Piscine,
Domaine Universitaire
38406 St. Martin d'Heres, Cedex, France
Facility address is:
Avenida Divina Pastora 7
Nucleo Central
18012 Granada, Spain
Phone: (33) 76 42 33 83
Contact: D. Downes
Sponsor: Centre National de la Recherche Scientifique, Paris, and Max
Planck Gesellschaft, Munich, and Instituto Geografico Nacional, Madrid
Reference: Baars, J. W. M., Hooghoudt, B. G., Mezger, P. G., de Jonge,
M. J., Astron. Astrophys. 175, 319 (1987)
Location: Pico Veleta, Spain
Latitude: +37° 04´ 05.6´´ N
Longitude: 3° 23´ 58.1´´ W
Altitude: 2870 m
Telescope: Steerable paraboloid
Diameter: 30 m
Area: 707 m2 at 0.50 eff.
Height: 15 m
Coverage: 0°-360° az., 5°-90° el.
Remarks: Biannual scheduling; deadlines of February 7, September 7
Observation Type: Millimeter wavelength spectroscopy and photometry
Frequency band(s):
74-115 GHz
130-170 GHz
203-270 GHz
250 GHz
320-360 GHz