Yurovs'kyj Y. Millisecond pulsation of solar radio emission: the physical properties and origin.

Українська версія

Thesis for the degree of Doctor of Science (DSc)

State registration number

0501U000181

Thesis Registration Form

0501U000181.pdf

Applicant for

Specialization

  • 01.03.02 - Астрофізика, радіоастрономія

24-05-2001

Specialized Academic Board

Д 26.208.01

Main Astronomical Observatory

Essay

The radio telescopes for digital registration of millisecond pulsation of radio flux are constructed. The data obtained during 40 years of daily observations of the Sun are published. The new direction of research of the physical properties of corona with use the millisecond radio pulsation have been developed. The parameters of plasma in the radio sources are appreciated. Is shown, that the known and the first time found properties of radio emission can be a consequence of scattering of radio waves by the inhomogeneity of solar corona.

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