The Siberian Solar Radio-Telescope: Parameters and principle of operation, objectives and results of first observations of spatio-temporal properties of development of active regions and flares

1986 ◽  
Vol 119 (1) ◽  
pp. 1-4 ◽  
Author(s):  
G. Ya. Smolkov ◽  
A. A. Pistolkors ◽  
T. A. Treskov ◽  
B. B. Krissinel ◽  
V. A. Putilov ◽  
...  
1994 ◽  
Vol 144 ◽  
pp. 509-512
Author(s):  
G. Ya. Smolkov ◽  
V. P. Nefedyev ◽  
A. M. Uralov ◽  
N. N. Kardapolova

AbstractThis paper has two goals: to report the informative merits of the Siberian solar radio telescope (SSRT) for ground-support of the SOHO or some other space mission, and provide a generalized presentation of one of the original results obtained at SSRT that indicates, we believe, a fundamental property of the emission from solar corona active regions (AR).


Solar Physics ◽  
1992 ◽  
Vol 142 (2) ◽  
pp. 341-358 ◽  
Author(s):  
C. E. Alissandrakis ◽  
B. I. Lubyshev ◽  
G. Ya. Smolkov ◽  
B. B. Krissinel ◽  
T. A. Treskov ◽  
...  

1973 ◽  
Vol 16 (12) ◽  
pp. 1463-1466
Author(s):  
V. S. Dekhtyarev ◽  
G. T. Kas'yanov ◽  
V. V. Kotovich ◽  
A. Ya. Smol'kov ◽  
A. V. Storozhko

1990 ◽  
Vol 311 (5) ◽  
pp. 313-315 ◽  
Author(s):  
G. N. Zubkova ◽  
N. N. Kardapolova ◽  
B. I. Lubyshev ◽  
V. P. Nefedyev ◽  
G. Ya. Smolkov ◽  
...  

1993 ◽  
Vol 141 ◽  
pp. 388-390
Author(s):  
A. A. Golovko

During the period of high solar activity (1988-1990) the Sayan and Baikal Observatories of the ISTP carried out observations of the chromosphere in the H-alpha line, the photosphere and of sunspot magnetic fields; at the Siberian Solar Radio Telescope, solar radio emission observations at 5.2 cm wavelength were made. Using those observations a study is made of the evolution of “centers of magnetic activity” (Bumba, 1986) in nine active regions with different flare productivity, for which the most complete observations were available. In three cases (NOAA Nos. 5229, 5643 and 5669) they were the targets of the cooperative international Max’91 program.


1986 ◽  
Vol 7 ◽  
pp. 755-757
Author(s):  
G. Ya. Smolkov

As is known from eclipse observations, the microwave emission of an active region consists of three main components: floccular, inter-spot (halo) and spot components which differ in intensity, the degree of polarization, and in structure and sizes /1/. A possibility of identifying the finer spatial and temporal structure in the active region (AR) emission has existed since RATAN, the VLA and WSRT became operational. The construction of the SSRT permitted the initiation of a systematic study of spatio-temporal properties of the development of active regions /2, 3/.The majority of the properties in the AR development are reflected in detail and rapidly in the microwave emission characteristics /4, 6/.


1999 ◽  
Vol 42 (6) ◽  
pp. 445-450 ◽  
Author(s):  
S. V. Lesovoy ◽  
A. T. Treskov ◽  
T. A. Treskov

2002 ◽  
Author(s):  
Alexander T. Altyntsev ◽  
Yuri V. Chugui ◽  
Valery P. Kiryanov ◽  
A. K. Potashnikov ◽  
Oleg I. Potaturkin ◽  
...  

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