Results 101 to 110 of about 1,087,488 (286)
Practical Limits in the Sensitivity-Linearity Trade-off for Radio Telescope Front Ends in the HF and VHF-low Bands [PDF]
Radio telescope front ends must have simultaneously low noise and sufficiently-high linearity to accommodate interfering signals. Typically these are opposing design goals. For modern radio telescopes operating in the HF (3-30 MHz) and VHF-low (30-88 MHz)
R. Tillman, S. Ellingson, J. Brendler
semanticscholar +1 more source
A decametric wavelength radio telescope for interplanetary scintillation observations [PDF]
A phased array, electrically steerable radio telescope (with a total collecting area of 18 acres), constructed for the purpose of remotely sensing electron density irregularity structure in the solar wind, is presented.
Cronyn, W. M., Shawhan, S. D.
core +1 more source
Probing ionospheric structures using the LOFAR radio telescope [PDF]
LOFAR is the LOw‐Frequency Radio interferometer ARray located at midlatitude (52°53′N). Here we present results on ionospheric structures derived from 29 LOFAR nighttime observations during the winters of 2012/2013 and 2013/2014.
M. Mevius+30 more
semanticscholar +1 more source
Bin Li, Zhiqiang Shen
semanticscholar +1 more source
Engineering and science highlights of the KAT-7 radio telescope [PDF]
The construction of the KAT-7 array in the Karoo region of the Northern Cape in South Africa was intended primarily as an engineering prototype for technologies and techniques applicable to the MeerKAT telescope.
A. Foley+107 more
semanticscholar +1 more source
In this talk, I will review the current status of the Sardinia Radio Telescope and the near-future technical developments. In particular, I will discuss the new generation receivers and focus on the spectroscopic capabilities of the telescope and on the impact that the SRT could have in the field of star formation .
openaire +2 more sources
For accurate astronomic and geodetic observations based on radio telescopes, the elevation-dependent deformation of the radio telescopes’ main reflectors should be known.
C. Holst+7 more
semanticscholar +1 more source
Sardinia Radio Telescope: General Description, Technical Commissioning and First Light [PDF]
In the period 2012 June–2013 October, the Sardinia Radio Telescope (SRT) went through the technical commissioning phase. The characterization involved three first-light receivers, ranging in frequency between 300MHz and 26GHz, connected to a Total Power ...
Pietro Bolli+37 more
semanticscholar +1 more source
The need for precise radio telescope pointing has driven great attention to investigating the effect of antenna local deformation or irregularity, such as unevenness in the azimuth track.
Ye Yuan, Zhi-Yong Liu, Na Wang
doaj +1 more source