Zobrazeno 1 - 10
of 13
pro vyhledávání: '"S. Kh. Tokhchukova"'
Autor:
V. P. Maksimov, D. V. Prosovetsky, T. I. Kaltman, A. A. Kochanov, S. Kh. Tokhchukova, I. I. Myshyakov
Publikováno v:
Geomagnetism and Aeronomy. 55:1124-1130
Microwave observations of the solar active region NOAA 11734 were done on April 28–May 8, 2013 with SSRT and the RATAN-600 radio telescopes. As a result of observations, two-dimensional distributions of the Stokes parameters I and V were obtained a
Publikováno v:
Astrophysical Bulletin. 69:356-367
We report the spectra of the horizontal size of the beam pattern of the RATAN-600 radio telescope operating in the “Southern Sector with a Flat Reflector” observing mode computed in the geometrical optics approximation with allowance for the beam
Publikováno v:
Geomagnetism and Aeronomy. 53:1021-1024
We present the results of a study of the subsecond pulses (SSPs) registered in the microwaves during the C2.4 solar flare. The event occurred on August 10, 2011, in the 11236 active region near the western limb and reached a maximum at 0935 UT. Subse
Publikováno v:
Astrophysical Bulletin. 67:225-229
New elements of the algorithmic and software bases of the ephemeris support for the RATAN-600 radio telescope observations of distant radio sources and objects of the Solar system are briefly described.
Publikováno v:
Astrophysical Bulletin. 66:488-495
We describe the technique and results of modelling the solar radio emission during the maximum phase of the solar eclipse of March 29, 2006 on the RATAN-600. The aim of modelling is to refine the brightness temperature of the solar corona at the dist
Autor:
S. Kh. Tokhchukova
Publikováno v:
Astrophysical Bulletin. 66:379-388
The development of observational equipment and software for processing and efficient representation of spectral and polarization solar microwave observations on the RATAN-600 contributes to obtaining new information about the parameters of plasma at
Autor:
S. Kh. Tokhchukova, V. M. Bogod
Publikováno v:
Cosmic Research. 44:506-519
Application of the mode of azimuthal observations on RATAN-600 has made it possible to realize multiple daily observations [1]. The results of multiwavelength observations of the Sun in this mode point to the existence of sharp spectral irregularitie
Publikováno v:
Astronomy Letters. 30:715-727
The observations of the solar radio emission on September 11, 2001, with the RATAN-600 radio telescope (southern sector) at four centimeter wavelengths (1.92, 2.24, 2.74, and 3.21 cm) revealed synchronous brightenings in solar radio sources. These we
Publikováno v:
Radiophysics and Quantum Electronics. 47:227-237
This paper is devoted to the development of capabilities of the RATAN-600 radio telescope by putting the regime of multi-azimuth observations at the southern sector with periscope reflector into regular operation. This method makes it possible to stu
Autor:
V. M. Bogod, S. Kh. Tokhchukova
Publikováno v:
Astronomy Letters. 29:263-273
RATAN-600 multiwavelength observations of the Sun reveal sharp spectral inhomogeneities in the polarized radiation from active regions that produce intense flares. These events occur in a wide range of radio fluxes (0.05–10 s.f.u.) in a relatively