Journal of Non-Crystalline Solids 156-158 (1993) 544-546 North-Holland jouR Na~ or ~ Solid state amorphization of the GaSb high pressure phase O.I. Barkalov, E.G. Ponyatovsky and V.E. Antonov Institute of Solid State Physics, Russian Academy of Science, 142432 Chernogolovka, Moscow region, Russian Federation The process of solid state amorphization of the quenched high pressure GaSb 'white tin'-phase was studied at normal pressure by means of differential scanning calorimetry (DSC) and dilatometry. ...

... Despite the use of counterweights, I have had ongoing problems with preventing unwanted motion in altitude, particularly during star parties when everyone seems to want to lean on the telescope while observing. ... After some difficulties at a windy star party a few years ago at the Boston Museum of Science, I designed a simple and very effective altitude brake and slow motion control which can be assembled very quickly and at minimal cost. ... The other end of the arm attaches to a turnbuckle*. ...

. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Achievments . N.V. Pushkov . 10/04/2016 01:59 MSK . webmaster@izmiran.ru . (C) 2007, IZMIRAN

... 7 2.3 Viewing and modifying registers and memory variables.. ... the output mode to out put access R/W R/W R/W R/W State after reset 0x00000000 0x00000000 0x00000000 Appendix B Table B.1 UART0 Registers The formula for calculating the UART transmission rate The main registers : U0RSR - register the received data; U0THR - data register for transmission; U0IER - Interrupt Enable UART: Bit 0 - 1 - enable interrupt if the received data; Bit 1 - 1 - enable interrupt when buffer under the ...

Next: Mission Operations Data Transfer . ... VLBI Tape Management . VLBI Tapes . ... When: As soon as the correlator is satisfied with the correlator output. back to top . ... What: Each correlator will maintain a data base including the status of all VLBI tapes under its control. ... The correlators will distribute tapes to mission elements based on the Observation Summary File produced by the RSOG ( Observation Summary File ) to ensure each element has enough tapes to support SVLBI observations. ...

. Variable stars - are characterised by the changeable glifter. There are eclipse twin stars and pulsing variable stars (cepheids) with the periodical changing of a glifter, eruptive stars, pulsars and closed twice stars. Back .

... Polish scientists at the Space Research Centre, Polish Academy of Sciences, in Wroclaw, south-west Poland, have constructed an instrument called SphinX (short for Solar PHotometer In X-rays), which is an X-ray spectrophotometer, that will obtain spectra in the energy range 0.5--15 keV in 256 energy channels with frequency of up to 100 times a second. ... SphinX is part of a package of instruments known as TESIS (PI Prof. Sergei Kuzin, Lebedev Institute, Moscow). ... Space Research Centre, . ...

Instruments and Methods 125 Long time tracking of the Sun with RATAN-600 in Radio Schmidt mode V.B. Khaikin, E.K. Ma jorova, I.G. E mov, O.A. Victorov, V.M. Bogod, and S.Kh. ... Cosmic source tracking with unmovable main mirror in a form of cylinder requires a special secondary mirror of double curvature 12 m size or a phased array in the focal plane of an ordinary secondary mirror Ka jdanovskij, 1980. ... Fig. 4 shows the Sun tracking with new drive in speed control mode starting from meridian. ...

... Progress in the development of the 1996 release of the IDL Wavelet Workbench (WWB) is shown. The WWB is now improved in several ways, among them are: (1) a smarter GUI which easily directs the user to the possibilities of the WWB, (2) the inclusion of more wavelets, (3) the enhancement of the input and output modules to provide a better interface to the input and output data and (4) the addition of more analysis methods based on the wavelet transform. ... More analysis routines are now available. ...

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