... 2002: . According to the RATAN-600 observations of the Sun in the microwave range, we isolated a class of flare-productive active regions, characterized by abrupt reversals of circular polarization in frequency and time in the interval from several hours to three days. This indicates the existence of a long preparatory phase in the preflare solar radiation. ... Archive . ... Last update: 17/02/2011 ...
Our publications in 2000 year Kniazev, A. Y.; Pustilnik, S. A.; Masegosa, J.; Marquez, I.; Ugryumov, A. V.; Martin, J.-M.; Izotov, Y. I.; Engels, D.; Brosch, N.; Hopp, U.; Merlino, S.; Lipovetsky, V. A. Astronomy and Astrophysics, v.357, p.101-110 (05/2000) . Compressed postscript version of the paper (170Kb) . ... 07/2000) . ... Kniazev, A. Yu.; ... Kniazev A.Y. Compressed postscript version of the 1st lecture (100Kb) . Kniazev A.Y. Compressed postscript version of the 2nd lecture (350Kb) . ...
... In LABORATORY OF RADIO ASTROPHYSICS OF SPECIAL ASTROPHYSICAL OBSERVATORY OF RAS . ... History . ... Current problems of the group research interests: . study for cosmic microwave background, . study of radio galaxies (identification, evolution, statistical investigation of population), . investigation of the RATAN-600 antenna, . observations in the survey mode with RATAN-600 and their analysis, . creation of the software for data analysis. vo @ sao.ru ( Oleg Verkhodanov ) ...
... Corresponding gates in each row are connected in parallel at both edges of the array. ... Other gates. ... otherwise indicated, 45 kpixels/sec and standard voltages using a dual slope CDS circuit (8 µs integration time) Minimum Format Pixel Size Imaging Area Dark current (MPP), 20° C equivalent Readout noise Front Back Full Well signal Output gain CTE per pixel Typical 512 x 512 pixels 24 µm x 24 µm 12.3 mm x 12.3 mm 50 pa/cm2 5 electrons 7 electrons 350,000 electrons 1.5 µV/ electron 0 ...