INTERNATIONAL ISO WD STANDARD Working draft ______________________________________________________________ Space environment (natural and artificial) Earth's ionosphere and plasmasphere. ... In the present International Standard the appendixes A and B are of informative nature only. ISO WD CONTENTS 1. ... Information presented in the each table about mean values of Ne, Te and Nu includes: - information line (first); - mean values of one of parameters for conditions given in the information line. ...

... Clear conditions, temperature ~16F, network to sundog. 16 mm f/1.4 lens 1 second exposure times 32 16-bit frames captured with frames buffered on the camera coadded dark frames in AIJ, divided by 12, subtracted from data stack aligned data stack using apertures coadded data stack of 12 dark-subtracted frames Stars visible to <8 mag The "NSEW" image polaris_sky5_1s_16mm_f1p4_darksub_nsew.png shows the sky as it would appear facing north in the northern hemisphere. ...

The Apache HTTP Server provides a mechanism for storing information in named variables that are called environment variables . ... For additional flexibility, the directives provided by mod_setenvif allow environment variables to be set on a per-request basis, conditional on characteristics of particular requests. ... As discussed above, the environment passed to CGI scripts includes standard meta-information about the request in addition to any variables set within the Apache configuration. ...

... APT Activities and Science Results 3. ... APT Secretary Philip Edwards (ISAS) reviewed the aims of the APT (http://www.vsop.isas.ac.jp/apt/DefinitionAndAims.html). ... The Australia Telescope Compact Array, and Ceduna, Hartebeesthoek, Kashima, Mopra, Parkes, and Shanghai telescopes of the Asia-Pacific Telescope participated in these observations. ... In the absence of Tetsuo Sasao, Philip Edwards briefly described results of the APT 22 GHz observations conducted from October 1st to 5th, 1997. ...

... The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorption lines where discovered in 1802 by the English scientist William Wollaston. ... Some stars as Pollux show a spectrum similar to that of our sun with strong Ca II and Fe II lines, others as Sirius or Vega show strong absorption lines of hydrogen, others, as Mira show very complicated spectra due to molecular absorption lines (see figure 5). ...

... The primary, secondary and tertiary structures of tRNAs and their function at the first stage of protein biosynthesis are discussed. еУОВНЫОњ Ъ МТФУ ЪМУИ кзд (Ъкзд) Л,, Ъ НО~В,Ы УОе , НТФ ВТТЛЛ ,,ВМУ,, Ы~ТЪ,Ыfl , ФВ В,УВ ЛМЩУ П^ЛЛ, ТУВ КВИТfl , ПЪ Л~Мњi кзд , ,ЛВ НУУМУ,, М flБњН ПЛМУНЛТОУЪМњi УТЪЪНУ, ћВОНУ,њi ^ВФВИ. ... ЗЗЦСЦзаЦ ї о,У У, й.й., 1998 () - , , , (). . ... 50- - (). , оДЗйкйЗД й.й. лнкйЦзаЦ нкДзлийкнзхп кзд 71 , , , . ... 3'-, - (CCA-). ... 1998. ... Val + + ATP Val- + AMP + PP, (1) AMP...