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Study of Solar Radiation on an All-Movable Radio Telescope
Journal of Astronomical Telescopes, Instruments, and Systems, 2021To grasp the effect of nonuniform temperature field, the effects of a nonuniform sunshine temperature field on a large, all-movable radio telescope were analyzed in this study. Based on the overall parameters of a radio telescope model, first, several specific steps of the ray-casting algorithm were introduced for calculating sunlight shadows on radio ...
Y. Liu
exaly +3 more sources
Some Results of Solar Radio Emission Observations at the Siberian Solar Radio Telescope
Astronomische Nachrichten, 1990AbstractThis paper gives the main characteristics of the Siberian Solar Radio Telescope as well as some results derived by investigating the s‐component sources and radio bursts on the Sun using the SSRT.
Robert Sych, G Ya Smolkov
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A High-Speed FFT Based on a Six-Step Algorithm: Applied to a Radio Telescope for a Solar Radio Burst
2013 International Conference on Field-Programmable Technology (FPT), 2013A radio telescope analyzes the radio frequency (RF) received from celestial objects. It consists of an antenna, a receiver, and a spectrometer. The spectrometer converts the time domain into the frequency domain with an FFT operation. A solar radio burst observation requires a high-speed FFT. This paper proposes a P parallel N point FFT for fixed point
Kazumasa Iwai +2 more
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Ten-Antenna Prototype of a Radio Heliograph Based on the Siberian Solar Radio Telescope
Geomagnetism and Aeronomy, 2009An upgrade of the Siberian Solar Radio Telescope (SSRT) [Smolkov et al., 1986; Grechnev et al., 2003] to a multiwave radio heliograph has been started. The radio heliograph being created will be designed mainly to measure coronal magnetic fields, to determine the locations of solar-flare energy release, and to investigate coronal mass ejections.
S. V. Lesovoy +5 more
exaly +3 more sources
Astrophysics and Space Science, 2015
Our aim is to prove that long time series of solar observations measured with Metsahovi Radio Observatory’s 1.8-meter solar radio telescope, RT-1.8, at 11.2 GHz are reliable, and that the data can be used for solar cyclicity studies. We give a detailed description of RT-1.8 and its calibration. We compare 14 years of Metsahovi Radio Observatory’s solar
Kallunki, Juha, Uunila, Minttu
semanticscholar +4 more sources
Our aim is to prove that long time series of solar observations measured with Metsahovi Radio Observatory’s 1.8-meter solar radio telescope, RT-1.8, at 11.2 GHz are reliable, and that the data can be used for solar cyclicity studies. We give a detailed description of RT-1.8 and its calibration. We compare 14 years of Metsahovi Radio Observatory’s solar
Kallunki, Juha, Uunila, Minttu
semanticscholar +4 more sources
Astronomy Reports, 2005
The radio brightness distribution at 5.2 cm has been obtained along the entire solar limb down to a level of 0.01 of brightness temperature at the disk center T0c during the solar minimum. The measurements are based on strip scans from the Siberian Solar Radio Telescope.
B. B. Krissinel
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The radio brightness distribution at 5.2 cm has been obtained along the entire solar limb down to a level of 0.01 of brightness temperature at the disk center T0c during the solar minimum. The measurements are based on strip scans from the Siberian Solar Radio Telescope.
B. B. Krissinel
openaire +2 more sources
Prospects for the solar radio telescope
1997The Solar Radio Telescope (SRT) is an instrument concept for a powerful solar-dedicated radio telescope. As presently conceived. it would combine a high-resolution imaging capability (2″ at 20 GHz) with a broadband spectroscopic capability (0.3–26 GHz).
Timothy S. Bastian, Dale E. Gary
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Additive-correlation regime of operation of the siberian solar radio telescope
Radiophysics and Quantum Electronics, 1999We describe a method for obtaining the two-dimensional image due to Earth’s rotation when performing observations using a cross interferometer. This method also allows us to record the one-dimensional distribution of radiobrightness to ensure high time resolution and is based on the serial recording of signals from each of the two linear ...
S. V. Lesovoy +2 more
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