Next: *fold* - Make a Up: Timing Analysis Previous: *ftpplot* - Distribution of . Search for periodicity using the timesorted output file . ... To search for a period p seconds in an observation of length t seconds, sorting into n bins, the period interval, , should be . ... The parameter get_gintvs=yes requires that an exposure be calculated for each interval, important if the period is comparable to the duration of gaps and good-data intervals. input file: rp90_sect2_sti.qp . ...

XmCCD Copyright 2007-2012 John Kielkopf ======================================= Development Log =============== March 9, 2002 Version 1.0.0 * Support for SBIG cameras using the first public SBIG library * Basic panel for operation with ds9 +--------------------------+ May 22, 2002 Version 1.1.0 * Updated to use libudrv 4.35 +--------------------------+ May 24, 2004 Version 1.2.0 * USB support +--------------------------+ March 1, 2005 Version 1.4.0 * Full ...

... Далее обязательно выравниваем цветовые слои. ... Можно посмотреть каждый цветовой слой отдельно или парой, устанавливая и снимая птички на Show red , green , blue ( рис. ... В идеале левая сторона гистограммы должна иметь одинаковые пики для всех трех цветовых каналов, это мы делаем двигая движки на панели Histogram рядом с каждым цветовым каналом. ... Вообще слои wavelet в некотором роде антагонисты: то, что мы усиливаем движками одного слоя, можно уменьшить, двигая влево, движки соседнего слоя. ...

... LLO and LHO seismometers: H0:PEM-LVEA_SEISX; H0:PEM-LVEA_SEISY; H0:PEM-LVEA_SEISZ; L0:PEMLVEA_SEISX; L0:PEM-LVEA_SEISY; L0:PEM-LVEA_SEISZ Threshold (sigma) 6 5.1 4.2 3.3 15 21 Events exceeding threshold Offset time series events 10 15 96 14687 (on - off) 5 6 4 186 sqrt(on+off) 4.6 6 14 172 100 14873 LLO and LHO mode cleaner control signals: L0:PEL1:IOO-MC_F; H2:IOO-MC_F1 Threshold (sigma) 6 5.1 4.2 3.3 2.85 61 91 ...

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Instruments and Methods 133 Sky temperature resolution by microwave radiometry A.G. Kislyakov State University, Nizhny Novgorod, Russia Introduction The threshold sensitivity of a radiometer is determined by well known equation Karlov & Manenkov, 1966 " hE i = h hn i +1 hn i + N t G0 , 1 G0 1=2 : 1 Here we denote hE ias the minimum detectable increment of radiation spectral density E at a frequency . ... Equation 3 gives a correction to the expression for limit detector sensitivity Kislyakov, 1997. ...

... Usually, the command line that starts the daemon is included in the system startup file, so it is executed only at system boot time; however, the daemon can be stopped and restarted from root at any time. ... In order to allow a sufficient number of samples for the NTP algorithms to reliably discriminate between correctly operating servers and possible intruders, at least four valid messages from at least one server is required before the daemon can not set the local clock. ...

... 18941904; Bespalov P.A. Effective saturation of absorption in a plasma magnetospheric maser. In book: Nonlinear Space Plasma Physics, R.Z. Sagdeev -Editor-in-Chief, American Institute of Physics, 1993, p.339-346]. Magnetospheric plasma maser [Bespalov P.A, Trakhtengerts V.Yu., ... In a magnetospheric plasma maser (MPM) the relatively dense magnetised plasma and the conjugate ends of a magnetic trap form a quasioptical resonator for electromagnetic waves. ...

... HTML defines six levels of headings. ... The numbering style is controlled by the style sheet, e.g. The style sheet specifies whether headers are numbered, and which style is used to render the current sequence number, e.g. arabic, upper alpha, lower alpha, upper roman, lower roman or a numbering scheme appropriate to the current language. ... CLEAR . ... This attribute is used to set the sequence number associated with the header level of the current element to a given number, e.g. SEQNUM=10. ...

... The coding is: C = Toward polarity; B = Mixed polarity; A = Away polarity. 1947 1 acccc ccaaa aaaaa bcccc cbabc ccccb b 2 cccba aabca aaaaa bcccc aaaaa aaa 3 bcbaa aabaa acccc bcccc caaca bcbcc a 4 cacab abaac ccccc ccbaa aaaaa aaaaa 5 aaaaa aaaac ccccc ccccc aaaca ababa a 6 aaaac ccccc cccaa baaba aaaaa aabaa 7 abaac ccccc ccccc bbcaa baaaa aacaa b 8 ccccc ...