... Three levels of accelerometers errors (1) are considered: 10-7 m/s2, 5·10-7 m/s2, 10-6 m/s2. ... accelerometers using accelerometers, = 10-7 m/s2 using accelerometers, = 5 10-7 m/s2 using accelerometers, = 10-6 m/s2 Position ...
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Ссылки http://www.cosmos.ru/conf/2009elw/presentations/presentations_pdf/session2/akim_ELW.pdf -- 311.2 Кб -- 02.03.2009 Похожие документы
... Seminar council . " GRB 030329 optical afterglow observations on the 1.5-m Russian-Turkish telescope RTT150 " . ... We present the results of the GRB 030329 optical afterglow observations on the 1.5-m Russian-Turkish telescope RTT150. ...
... of the sample, within which the hydrogen is measured, is ~5–20 ?m depending on the atomic weight of the sample, its density and ... Effective depth ~5 – 20 mm . ...
... for example TeO2 (0.4-5.2 µm) Effectiveness 60-70% Maximal possible resolving power ... spectral range 2.354.2 µm relatively compact design (~5 kg) no moving parts (except ...
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Ссылки http://www.cosmos.ru/oct4/2007/ppt/03_07_Oleg_Korablev.pdf -- 2392.7 Кб -- 04.12.2007 Похожие документы
... very thin sample - the bigger the "thicker" sample Spectral range: 2.5 - 25 m Spectral resolution: 5 - 10 cm-1 Sources of bio ... External assistance Type / Value Attenuated Total Reflection 2.5 - 25 m5 - 10 cm -1 Notes By now not used in planetary ...
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Ссылки http://www.cosmos.ru/conf/2009elw/presentations/presentations_pdf/session7/grigoriev_ELW.pdf -- 592.4 Кб -- 02.03.2009 Похожие документы
... the MARSES experiment is based on: New Multifrequency Electromagnetic Sensor : A. Small rover HFS (high-frequency sounding) with Antenna size ( 0.5m. B. Small station HFS sounding with Antenna size ( 0.5m. and Low-frequency sounding MARS TEM-48,97 for ...
... 0.1 to 0.8 nm band as follows: Class W/m*2 Ergs/cm*2/s B I < 10E-6 I < 10E-3 C 10E-6 <= I < 10E-5 10E-3 <= I < 10E-2 M 10E-5 <= I < 10E-4 10E-2 <= I < 10E-1 X I >=10E-4 I >=10E-1 ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SOLAR_FLARES/XRAY_FLARES/xray.fmt.rev ...