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Open AccessArticle10.1017/s0074180900050956

Some remarks on the polarization of 200-Mc/s solar radio emission

M. H. Cohen,A. D. Fokker-1959-01-01-Symposium - International Astronomical Union

TL;DRAbstract

Detecting a weak linearly polarized component in an isolated solar burst is very difficult. It is a unique event and it is not possible to make a series of observations to reduce the error. Interference and reflections confuse the result and it is extremely difficult to determine the equipment parameters precisely, especially those pertaining to the antenna.

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Detecting a weak linearly polarized component in an isolated solar burst is very difficult. It is a unique event and it is not possible to make a series of observations to reduce the error. Interference and reflections confuse the result and it is extremely difficult to determine the equipment parameters precisely, especially those pertaining to the antenna.

Keywords

Solar radioPolarization (electrochemistry)Interference (communication)Event (particle physics)Antenna (radio)PhysicsComponent (thermodynamics)Electromagnetic interference

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