... 2004: . Creation of a unique set of the spectral and polarization complex of high resolution in the range of 6-18 GHz, consisting of 64 channels with a 1% analysis stripe was concluded. Based on the combination of key parameters - the frequency overlap and resolution, sensitivity and accuracy of polarization measurements, such a complex is the first instrument of its kind in the practice of solar astronomy. ... Archive . ...

Red Hat Advanced Development Labs . ... Table of Contents . I. Overview . ... GTK+ Basics . ... Building a Gnome Application . ... Gnome Application Basics . ... Gnome Application Checklist . ... Advanced GTK+/Gnome Techniques . The GTK+ Object and Type System . GDK Basics . Writing a GtkWidget . ... Writing a GnomeCanvasItem . ... GTK+/Gnome Object Hierarchy . Table of Header Files . ...

A bout ADLab . ... designing of high-sensitivity imaging systems for the 6-m telescope of the Russian AS; . development of new-type image detectors for astronomy in cooperation with other research and industrial institutions. ... analog TV tube systems incorporating image tubes with charge accumulation (SEC vidicon, silicon vidicon, SIT vidicon and others ) and digital processing of videosignal; . ... In 1986 the first CCD system incorporating an array of 512 x 576 pixels was developed in the Lab. ...

... 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 ...