Results 31 to 40 of about 7,486 (141)
Supernova Remnants with Fermi Large Area Telescope
The Large Area Telescope (LAT), on-board the Fermi satellite, proved to be, after 8 years of data taking, an excellent instrument to detect and observe Supernova Remnants (SNRs) in a range of energies running from few hundred MeV up to few hundred GeV ...
Caragiulo M., Di Venere L.
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Modelling and design of a coupled system of multiple hydraulic systems and large structures
Control of large structures often involves the use of hydraulic equipment due to the large power requirements. In this study, a large telescope is taken as an example of a large structure.
Tomoya HATTORI+2 more
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Since volcanic activity was first discovered on Io from Voyager images in 1979, changes on Io's surface have been monitored from both spacecraft and ground‐based telescopes.
Al Conrad+20 more
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On-orbit assembling space telescope (OAST) is one of the most feasible methods to implement a large-scale space telescope. Unlike a monolithic space telescope (such as Hubble Space Telescope, HST) or a deployable space telescope (such as James Webb Space
Ye Kuang+4 more
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Extremely Large Telescopes [PDF]
Extremely large telescopes are being planned to address a number of the most profound questions in astronomy today. From the detection and study of extra-solar planets to the study of the first galaxies these optical and infrared telescopes are designed to provide powerful new probes in the field.
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Active Surface Compensation for Large Radio Telescope Antennas
With the development of radio telescope antennas with large apertures, high gain, and wide frequency bands, compensation methods, such as mechanical or electronic compensation, are obviously essential to ensure the electrical performance of antennas that
Congsi Wang+8 more
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The Cherenkov Telescope Array Large Size Telescope
4 pages, 5 figures, In Proceedings of the 33rd International Cosmic Ray Conference (ICRC2013), Rio de Janeiro (Brazil).
Ambrosi, G.+131 more
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Chromospheric K CaII telescope of Baikal Astrophysical Observatory. New light
In recent years, most results of CaII studies of the solar chromosphere in H and K lines have been based on observations with narrow passband filters.
Lopteva L.S.+6 more
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Interferometry with Large Telescopes [PDF]
1. Introduction. A popular - often textbook supported- view is that the diffraction limit of large telescopes is out of reach from ground-based observatories.We summarize on Fig.1 the scope of angular resolving power, in the range lOOnm to 10. nm, as it appears today.A quick look reveals, expressed in absolute angular terms, a number of stimulating ...
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Bernhard Schmidt and the Schmidt Telescope for Mapping the Sky
Bernhard Voldemar Schmidt (1879-1935) was born in Estonia. He ran an optical workshop in Mittweida, Saxonia, between 1901 and 1927. Astronomers appreciated the quality of his telescopes.
Wolfschmidt G.
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