Search results
Results From The WOW.Com Content Network
RADIO ASTRONOMY: 25 550–25 650 RADIO ASTRONOMY: 37.5–38.25 MHz FIXED MOBILE Radio astronomy: 322–328.6 FIXED MOBILE RADIO ASTRONOMY: 406.1–410 FIXED MOBILE except aeronautical mobile RADIO ASTRONOMY: 1 400–1 427 EARTH EXPLORATION-SATELLITE (passive) RADIO ASTRONOMY SPACE RESEARCH (passive) 1 610.6–1 613.8
An astronomical radio object is classified as a ROCOS if it possesses (a) an optical image with stellar appearance, which is identified with a radio source, and (b) no emission or absorption features in its optical spectrum, except for those due to galactic interstellar medium, with a signal-to-noise ratio at the level of those observable for quasar candidates. [1]
Operated by the National Centre for Radio Astrophysics. [14] Ooty Radio Telescope (ORT) Ooty, Tamil Nadu, India 326.5 MHz The radio telescope is a 530-metre (1,740 ft) long and 30-metre (98 ft) tall cylindrical parabolic antenna. It operates at a frequency of 326.5 MHz with a maximum bandwidth of 15 MHz at the front end. Gauribidanur Radio ...
العربية; Azərbaycanca; বাংলা; Беларуская; Беларуская (тарашкевіца) Български; Català; Čeština
The Observatory has been used for studying various aspects of the Sun, galaxies and pulsars. A few observations with the array have been the first two-dimensional images of radio emission from slowly varying discrete sources in the outer solar corona, an all-sky survey of radio sources at 34.5 MHz in the declination range -30° S to 60° N, and a low frequency carbon recombination lines in ...
Observation of the Sun at radio wavelengths, in particular of the solar corona, has been a long-standing focus of the RATAN-600's scientific programme. It has also contributed to radio observation for the SETI project. The RATAN-600 has not been dogged by the technical problems of the neighbouring BTA-6.
The National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research (NCRA-TIFR) is a institute for radio astronomy in India. Research activities at NCRA-TIFR are centered on low frequency radio astronomy, with research in a wide range of areas, including solar physics, pulsars, active galactic nuclei, the interstellar medium, supernova remnants, the Galactic Center, nearby ...
العربية; বাংলা; Беларуская; Български; Català; Čeština; Ελληνικά; Español; Esperanto; Euskara; فارسی; Français