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Development of an Astrophysical Facility for the Studies of Fast
Variable Processes.
We finalized the development of a facility for observations (including
remote observations) of the star-shaped objects with the temporal
resolution of 1 micro second. The facility is featuring a multimode
panoramic photospectropolarimeter, 1 or 2 coordinate-sensitive quanta
detectors and a four-computer measurement control and registration system.
Observational modes: photometric in the UBVR colour bands, spectral
(50 or 10 nm per pixel), photopolarimetric and spectropolarimetric
in 2 or 4 polarisation planes.
(For contacts: G.M.Beskin)
RATAN-600 Multi-Octave Frequency Range Overlapping Finalized.
We finalized the multi-octave overlapping of the RATAN-600 frequency range
from 0.75 to 18GHz with the frequency resolution of 1% using the parallel
spectrum analysing complex. In combination with large effective area,
the RATAN-600 offers new opportunities of studying the thin structure
of the solar corona radio emission. We have implemented the registration
of the instantaneous spectra throughout the entire frequency range.
Regular observations of the Sun go through an automated reduction and
are available at
http://www.spbf.sao.ru/prognoz/
within 4 minutes from the acquisition time.
(For contacts: V.M.Bogod)
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Archive