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radio telescopes

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Image
Lunar <span class="search-highlight">radio</span> <span class="search-highlight">telescope</span> fills a lunar crater on the far side.
Published: 01 January 2006
Figure 6.5. Lunar radio telescope fills a lunar crater on the far side.
Series: GSA Field Guide
Published: 01 January 2011
DOI: 10.1130/2011.0022(01)
EISBN: 9780813756226
... large radio telescopes and two laser ranging facilities at the same observatory is exceptional; the large “G” ring laser is a unique instrument. Staff members are available to explain technical and operational details and to answer questions. Last but not least, the observatory is located...
FIGURES
Series: GSA Field Forum Field Trip Guides
Published: 01 January 2005
DOI: 10.1130/2005.IAAEOM.FFG-p27
EISBN: 9780813759371
... predominantly of late Proterozoic and early Paleozoic metasedimentary rocks. Black Mountain, the peak at 11 o'clock, contains a thick sequence of dark brown Campito Formation quartzite, which we will see trapped between plutons in the Sierra Nevada at the next stop. At M104 radio telescopes of the Owens...
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Journal Article
Journal: Economic Geology
Published: 01 May 1980
Economic Geology (1980) 75 (3): 460–465.
... carried out with radio telescopes at the National Radio Astronomy Observatory (NRAO). The 38th parallel lineament, a zone of strike-slip faults and other features, has been proposed by several authors to pass through the Green Bank area and to extend to the Blue Ridge in Virginia. This study, based...
Journal Article
Published: 01 October 1983
Canadian Journal of Earth Sciences (1983) 20 (10): 1586–1597.
...W. F. Teskey; W. Niemeier; M. Sideris; R. G. Lyall Abstract The proposed Canadian Long Baseline Array (CLBA) and the use of several radio telescopes in the CLBA as very long baseline interferometry (VLBI) stations to determine possible movements of tectonic plates are briefly described. The need...
Journal Article
Published: 01 March 2016
South African Journal of Geology (2016) 119 (1): 83–90.
... locations of temperature sensors on the composite structure of the Hartebeesthoek Radio Astronomy Observatory (HartRAO) LLR 1-metre optical telescope. Furthermore, we describe a mathematical model for (i) obtaining thermal measurements from a network of temperature sensors, (ii) interpolating...
FIGURES
Image
(  left  ) Space-facing end of the Long Duration Exposure Facility in orbit...
Published: 01 June 2016
F igure 2 ( left ) Space-facing end of the Long Duration Exposure Facility in orbit. P hoto courtesy of NASA. ( center ) Submillimeter impact crater in an aluminum panel from the Long Duration Exposure Facility. P hoto courtesy of NASA. ( right ) The NAIC Arecibo Observatory, a radio
Image
70-cm wavelength radar image, collected using the Arecibo and Greenbank rad...
Published: 01 January 2006
Figure 2.55. 70-cm wavelength radar image, collected using the Arecibo and Greenbank radio telescopes, of three large lunar craters (Aristoteles, at upper left, is 87 km diameter). The brightness variations reflect differences in decimeter-scale rocks on the surface or suspended within the upper
Journal Article
Published: 01 March 2016
South African Journal of Geology (2016) 119 (1): 109–116.
... radio telescopes, in order to reveal the structure of extremely compact astronomical radio sources. Subsequently, the use of VLBI has seen rapid expansion and has gained widespread recognition ( Clark, 2003 ). The VLBI technique is unique in that it provides milliarcsecond or even sub-milliarcsecond...
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Image
—What astronomers term “Cygnus A” <span class="search-highlight">Radio</span> Source taken with 200-inch <span class="search-highlight">telescop</span>...
Published: 01 July 1957
Fig. 4. —What astronomers term “Cygnus A” Radio Source taken with 200-inch telescope, and interpreted as collision of two galaxies. (Mount Wilson and Palomar Observatories.)
Journal Article
Journal: The Leading Edge
Published: 01 September 2011
The Leading Edge (2011) 30 (9): 996–1003.
... is to implement CS, and matrix incoherence is the main parameter. The “Y”-shaped configuration currently used by the Very Large Array (VLA) interferometer and reflected in the Giant Metrewave Radio Telescope (GMRT) configuration is used as the comparison model, as both are prominent interferometers currently...
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Journal Article
Published: 01 December 2011
South African Journal of Geology (2011) 114 (3-4): 573–576.
...) radio telescope. Figure 4. LLR telescope in temporary structure at HartRAO (Hartbeesthoek) where it is undergoing refurbishment before being moved to Matjiesfontein. The lunar laser ranger weighs approximately 5 tons. The total pressure that the LLR and the foundation will exert...
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Image
(A)  A 3-dimensional model showing a complete view of the 1-m aperture opti...
Published: 01 March 2016
Figure 1. (A) A 3-dimensional model showing a complete view of the 1-m aperture optical telescope at the Hartebeesthoek Radio Astronomy Observatory, and ( B ) cross section and side view of the telescope indicating the material components considered for thermal analysis in this study. The model
Image
—N.G.C. 5128, which object astronomers believe may be two galaxies in colli...
Published: 01 July 1957
Fig. 5. —N.G.C. 5128, which object astronomers believe may be two galaxies in collision and is a probable radio source. (200-inch telescope photograph. Mount Wilson and Palomar Observatories.)
Journal Article
Published: 01 September 2007
South African Journal of Geology (2007) 110 (2-3): 225–234.
.... at McDonald Observatory, USA, and Observatory de la Cote d’ Azur in France). Lunar distance measurements utilise retro-reflector mirrors installed on the Moon by Apollo 11 and 15. Radio telescope antennas will also be installed at the site for Very Long Baseline Interferometry (VLBI) studies to determine...
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Journal Article
Journal: Elements
Published: 01 June 2022
Elements (2022) 18 (3): 145–146.
... (European Space Agency) satellites ISO (Infrared Space Observatory) and HSO (Herschel Space Observatory), as well as numerous observation campaigns with major radio telescopes (e.g., IRAM, ALMA, VLA). In 2006, she was awarded the prize of Femme Scientifique de l Année (Woman Scientist of the Year...
Journal Article
Journal: Elements
Published: 01 February 2009
Elements (2009) 5 (1): 41–46.
... transmitters and receivers at different locations and with long travel times in the solar system to explore away from zero angle, but only slightly. By using Clementine as the transmitter and a radio telescope on the ground as the receiver, mission radar scientists could measure the angular dependence of sense...
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Journal Article
Published: 01 October 2020
American Mineralogist (2020) 105 (10): 1508–1535.
... of these phases is documented primarily by telescopic observations of absorption and emission spectra of interstellar molecules in radio, microwave, or infrared wavelengths. Nebular and circumstellar ice : Evidence from infrared observations and laboratory experiments suggest that cubic H 2 O (“cubic ice...
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Journal Article
Published: 01 December 2022
Jour. Geol. Soc. India (2022) 98 (12): 1765–1767.
... their scientific reach. These include (i) the Large Hadron Collider (LHC) accelerator at the European organization for Nuclear Research (CERN) (ii) the indigenous Indian Neutrino Observatory (INO), (iii) The Laser Interferometer Gravitational-Wave Observatory (LIGO) and (iv) The Square Kilometer Array (SKA) Radio...
FIGURES
Journal Article
Published: 15 January 2020
Seismological Research Letters (2020) 91 (3): 1417–1429.
... was the time of transit of stars, observed through a telescope (a transit telescope or meridian circle) designed to move only in the plane of the meridian. When a star crosses the center of the telescope’s optical axis, the local sidereal time is equal to the right ascension of the star. Stars with the most...
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